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    <title>Recent ucla_epss_rw items</title>
    <link>https://escholarship.org/uc/ucla_epss_rw/rss</link>
    <description>Recent eScholarship items from Open Access Policy Publications and other Recent Works</description>
    <pubDate>Fri, 19 Jun 2026 14:25:42 +0000</pubDate>
    <item>
      <title>Role of tectonic rock damage in erosional processes: A global analysis.</title>
      <link>https://escholarship.org/uc/item/690226kz</link>
      <description>The role of active faults in driving rock uplift is well known, but their influence on rock damage and erosional efficiency remains unclear globally. Using 1744 beryllium-10 (&lt;sup&gt;10&lt;/sup&gt;Be)-derived erosion rates, we show that erosional efficiency is elevated on average within ~15 kilometers of a fault trace and decreases with distance, up to ~100 kilometers. Reverse faults and those longer than 140 kilometers show the strongest effects. This length scale of decay suggests that tectonic damage extends beyond fault-core pulverization on primary faults, possibly including fracturing or grain-to-grain contact weakening due to seismic shaking and distributed deformation on complex fault networks. Machine learning identified fault proximity as a dominant control on erosional efficiency, exceeding precipitation and lithology, particularly when a measure of seismic shaking is included. These findings indicate that active tectonics are associated with erosion not only through uplift...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/690226kz</guid>
      <pubDate>Wed, 3 Jun 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Kuhasubpasin, B</name>
        <uri>https://orcid.org/0009-0002-8538-5220</uri>
      </author>
      <author>
        <name>Moon, S</name>
        <uri>https://orcid.org/0000-0001-5207-1781</uri>
      </author>
      <author>
        <name>Lithgow-Bertelloni, C</name>
        <uri>https://orcid.org/0000-0003-0924-6587</uri>
      </author>
    </item>
    <item>
      <title>Polycyclic Metamorphism, Exhumation, and Recycling of Subduction Complex Rocks, Cedros Island, Baja California</title>
      <link>https://escholarship.org/uc/item/61g510pn</link>
      <description>Abstract  High‐pressure rocks from subduction complexes are key records of the physical and chemical processes that operate on the subduction interface, but interpretation of these records requires accurate structural understanding of where they formed in the subduction zone and the mechanisms by which they were exhumed. We present new geologic mapping, outcrop‐scale observations, and geochronology from subduction‐zone assemblages at Punta Prieta Ridge on Cedros Island, Baja California (Mexico), to investigate the history of subduction, exhumation, and structural assembly of these rocks. The rocks of Punta Prieta Ridge are exposed in the footwalls of high‐ and low‐angle normal faults that carry Cretaceous forearc basin strata and attenuated mantle sections of the Cedros Island Ophiolite in their hangingwalls. The footwall rocks are subduction‐zone assemblages organized into distinct nappes that decrease in metamorphic grade and degree of strain structurally downward. Garnet‐amphibolite...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/61g510pn</guid>
      <pubDate>Mon, 1 Jun 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Wang, Jordan W</name>
      </author>
      <author>
        <name>Kapp, Paul</name>
      </author>
      <author>
        <name>Holder, Robert</name>
      </author>
      <author>
        <name>He, John</name>
      </author>
      <author>
        <name>Hernández‐Uribe, David</name>
      </author>
      <author>
        <name>Worthington, James</name>
      </author>
    </item>
    <item>
      <title>Magnetohydrodynamic control of differential rotation and dynamo transitions: rise of the local magnetic Rossby number</title>
      <link>https://escholarship.org/uc/item/52056776</link>
      <description>ABSTRACT We investigate how the strength of the Lorentz force alters stellar convection zone dynamics in a suite of buoyancy-dominated, 3D, spherical shell convective dynamo models. This is done by varying only the fluid’s electrical conductivity via the non-dimensional magnetic Prandtl number, $Pm$. Because the strength of the dynamo magnetic field and the Lorentz force scale with $Pm$, it is found that the fluid motions and mode of dynamo generation differ across the $0.25 \le Pm \le 10$ range investigated here. For example, we show that strong magnetohydrodynamic effects cause a fundamental change in the surface zonal flows: differential rotation switches from solar-like with prograde equatorial zonal flow for larger electrical conductivities (i.e. stronger dynamo magnetic field) to an anti-solar differential rotation with retrograde equatorial zonal flow at lower electrical conductivities (i.e. weaker magnetic field). This study shows that the value of electrical conductivity...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/52056776</guid>
      <pubDate>Wed, 22 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Soderlund, Krista M</name>
      </author>
      <author>
        <name>Wulff, Paula</name>
      </author>
      <author>
        <name>Käpylä, Petri J</name>
      </author>
      <author>
        <name>Aurnou, Jonathan M</name>
      </author>
    </item>
    <item>
      <title>Tabletop Atmospheric Rivers</title>
      <link>https://escholarship.org/uc/item/4tn7t9hb</link>
      <description>Tabletop Atmospheric Rivers</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4tn7t9hb</guid>
      <pubDate>Wed, 22 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Aurnou, Jonathan M</name>
      </author>
      <author>
        <name>Moscoso, Jordyn E</name>
      </author>
      <author>
        <name>Cavallo, Steven M</name>
      </author>
      <author>
        <name>Chen, Shizhe</name>
      </author>
      <author>
        <name>Church, William J</name>
      </author>
      <author>
        <name>Gonzalez, Alex O</name>
      </author>
      <author>
        <name>Landayan, Ryan</name>
      </author>
      <author>
        <name>Ruppert, James H</name>
      </author>
      <author>
        <name>Tripoli, Rachel E</name>
      </author>
    </item>
    <item>
      <title>Transition from wall modes to multimodality in liquid gallium magnetoconvection</title>
      <link>https://escholarship.org/uc/item/40256498</link>
      <description>Coupled laboratory-numerical experiments of Rayleigh-Bénard convection in liquid gallium subject to a vertical magnetic field are presented. The experiments are carried out in two cylindrical containers with diameter-to-height aspect ratio Γ=1.0 and 2.0 at varying thermal forcing (Rayleigh numbers 105≲Ra≲108) and magnetic field strength (Chandrasekhar numbers 0≲Ch≲3×105). Laboratory measurements and numerical simulations confirm that magnetoconvection in our finite cylindrical tanks onsets via nondrifting wall-attached modes, in good agreement with asymptotic predictions for a semi-infinite domain. With increasing supercriticality, the experimental and numerical thermal measurements and the numerical velocity data reveal transitions between wall mode states with different azimuthal mode numbers and between wall-dominated convection to wall and interior multimodality. These transitions are also reflected in the heat transfer data, which combined with previous studies connect onset...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/40256498</guid>
      <pubDate>Wed, 22 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>徐宇凡</name>
      </author>
      <author>
        <name>Xu, Yufan</name>
      </author>
      <author>
        <name>霍恩, 苏珊娜</name>
      </author>
      <author>
        <name>Horn, Susanne</name>
      </author>
      <author>
        <name>奥诺, 乔纳森</name>
      </author>
      <author>
        <name>Aurnou, Jonathan M</name>
      </author>
    </item>
    <item>
      <title>Eddy-driven Zonal Jet Flows in the Laboratory</title>
      <link>https://escholarship.org/uc/item/3j01t4fg</link>
      <description>Zonal jets are a ubiquitous feature of the circulation of planetary atmospheres, oceans and interiors. Many of the dynamical mechanisms that lead to the formation and evolution of such jets can be reproduced and studied in laboratory experiments, which have proved to be important sources of insight for understanding the nature of planetary jets. Here we introduce some of the key concepts underlying the production and maintenance of patterns of zonal jets in rotating and/or stratified flows. We then review a broad range of laboratory experiments that have helped to test and verify many of the dynamical mechanisms proposed to interpret geophysical jets involving the interaction of eddies and zonal flows. Laboratory experiments continue to have an important role to play in elucidating a quantitative understanding of zonal jets and their interactions with other aspects of planetary circulation systems.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3j01t4fg</guid>
      <pubDate>Wed, 22 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Read, Peter</name>
      </author>
      <author>
        <name>Afanasyev, Yakov</name>
      </author>
      <author>
        <name>Aurnou, Jonathan</name>
      </author>
      <author>
        <name>Lemasquerier, Daphné</name>
      </author>
    </item>
    <item>
      <title>Observed Changes in Mars Soil Thermophysical Properties Due to Rover Wheel Interactions: MER Mini-TES Observations and Applications to Upcoming Lunar Rover Exploration</title>
      <link>https://escholarship.org/uc/item/1dj1h580</link>
      <description>Abstract: 

                  The Mars Exploration Rovers (MER) Spirit and Opportunity each carried a thermal infrared (IR) instrument called the Miniature Thermal Emission Spectrometer (Mini-TES) used to determine rock and soil composition and thermophysical properties. In this work, we investigate how rover operations affect soil thermophysical properties by analyzing Spirit Mini-TES observations of both disturbed and undisturbed soils in Gusev crater. Observations of one location disturbed by rover wheels and two nearby undisturbed locations were acquired multiple times per sol over sols 172–174 and were compared with a thermal model to derive quantitative thermal inertia. We found that the disturbed soils have higher average thermal inertia and lower albedos than nearby undisturbed soils. These results are consistent with an increase in apparent particle size caused by the fine particulate, high-albedo airfall dust layer that coats all undisturbed surfaces in Gusev crater...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1dj1h580</guid>
      <pubDate>Wed, 8 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Byron, Benjamin D</name>
      </author>
      <author>
        <name>Donaldson Hanna, Kerri L</name>
      </author>
      <author>
        <name>Dove, Addie</name>
      </author>
      <author>
        <name>Ruff, Steve W</name>
      </author>
      <author>
        <name>Willams, Jean-Pierre</name>
      </author>
      <author>
        <name>Landis, Margaret</name>
      </author>
      <author>
        <name>Hayne, Paul O</name>
      </author>
      <author>
        <name>Bennett, Kristen A</name>
      </author>
      <author>
        <name>Sunshine, Jessica</name>
      </author>
      <author>
        <name>Tripathi, Prateek</name>
      </author>
    </item>
    <item>
      <title>Melting of MgSiO3 determined by machine learning potentials</title>
      <link>https://escholarship.org/uc/item/5mj553pn</link>
      <description>Melting in the deep rocky portions of planets is important for understanding the thermal evolution of these bodies and the possible generation of magnetic fields in their underlying metallic cores. But the melting temperature of silicates is poorly constrained at the pressures expected in super-Earth exoplanets, the most abundant type of planets in the galaxy. Here, we propose an iterative learning scheme that combines enhanced sampling, feature selection, and deep learning, and develop a unified machine learning potential of ab initio quality valid over a wide pressure-temperature range to determine the melting temperature of MgSiO3. The melting temperature of the high-pressure, post-perovskite phase, important for super-Earths, increases more rapidly with increasing pressure than that of the lower pressure perovskite phase, stable at the base of Earth's mantle. The volume of the liquid closely approaches that of the solid phases at the highest pressure of our study. Our computed...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5mj553pn</guid>
      <pubDate>Fri, 30 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Deng, Jie</name>
      </author>
      <author>
        <name>Niu, Haiyang</name>
      </author>
      <author>
        <name>Hu, Junwei</name>
      </author>
      <author>
        <name>Chen, Mingyi</name>
      </author>
      <author>
        <name>Stixrude, Lars</name>
        <uri>https://orcid.org/0000-0003-3778-2432</uri>
      </author>
    </item>
    <item>
      <title>Quantifying the impacts of rainfall and evaporation on Lake Bonneville</title>
      <link>https://escholarship.org/uc/item/2xp974r1</link>
      <description>Improved understanding of hydroclimatic drivers in water-stressed regions enables more accurate forecasting of future climate change impacts. Lake Bonneville was the largest Pleistocene lake in western North America, with a maximum surface area of ~52,000 km&lt;sup&gt;2&lt;/sup&gt;, before shrinking markedly to become the modern Great Salt Lake. After more than a century of study, the balance between enhanced precipitation and reduced evaporation as drivers of lake growth continues to be debated. Multiple studies identify precipitation as the main factor associated with the highest lake levels, but most proxies provide an estimate of net evaporation and cannot independently resolve precipitation from evaporation. Therefore, factors associated with lake size, growth, and retreat remain uncertain. This study uses the thermodynamically based carbonate clumped isotope geothermometer to estimate temperature, evaporation, and precipitation at Lake Bonneville from 23 to 16 thousand years ago (ka)....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2xp974r1</guid>
      <pubDate>Tue, 6 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Mering, John</name>
      </author>
      <author>
        <name>Arnold, Alexandrea J</name>
      </author>
      <author>
        <name>Chari, Lauren</name>
      </author>
      <author>
        <name>Lee, Hung-I</name>
      </author>
      <author>
        <name>Lerback, Jory</name>
      </author>
      <author>
        <name>Ajoku, Osinachi</name>
      </author>
      <author>
        <name>Ibarra, Daniel E</name>
      </author>
      <author>
        <name>Nelson, Stephen</name>
      </author>
      <author>
        <name>Farnsworth, Alexander</name>
      </author>
      <author>
        <name>Valdes, Paul</name>
      </author>
      <author>
        <name>Tripati, Aradhna</name>
        <uri>https://orcid.org/0000-0002-1695-1754</uri>
      </author>
    </item>
    <item>
      <title>Evaluating the Shinumo-Sespe drainage connection: Arguments against the “old” (70–17 Ma) Grand Canyon models for Colorado Plateau drainage evolution</title>
      <link>https://escholarship.org/uc/item/98z5z5kk</link>
      <description>Abstract
                  The provocative hypothesis that the Shinumo Sandstone in the depths of Grand Canyon was the source for clasts of orthoquartzite in conglomerate of the Sespe Formation of coastal California, if verified, would indicate that a major river system flowed southwest from the Colorado Plateau to the Pacific Ocean prior to opening of the Gulf of California, and would imply that Grand Canyon had been carved to within a few hundred meters of its modern depth at the time of this drainage connection. The proposed Eocene Shinumo-Sespe connection, however, is not supported by detrital zircon nor paleomagnetic-inclination data and is refuted by thermochronology that shows that the Shinumo Sandstone of eastern Grand Canyon was &amp;gt;60 °C (∼1.8 km deep) and hence not incised at this time. A proposed 20 Ma (Miocene) Shinumo-Sespe drainage connection based on clasts in the Sespe Formation is also refuted. We point out numerous caveats and non-unique interpretations of paleomagnetic...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/98z5z5kk</guid>
      <pubDate>Wed, 17 Dec 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Karlstrom, Karl E</name>
      </author>
      <author>
        <name>Jacobson, Carl E</name>
      </author>
      <author>
        <name>Sundell, Kurt E</name>
      </author>
      <author>
        <name>Eyster, Athena</name>
      </author>
      <author>
        <name>Blakey, Ron</name>
      </author>
      <author>
        <name>Ingersoll, Raymond V</name>
      </author>
      <author>
        <name>Mulder, Jacob A</name>
      </author>
      <author>
        <name>Young, Richard A</name>
      </author>
      <author>
        <name>Beard, L Sue</name>
      </author>
      <author>
        <name>Holland, Mark E</name>
      </author>
      <author>
        <name>Shuster, David L</name>
      </author>
      <author>
        <name>Winn, Carmen</name>
      </author>
      <author>
        <name>Crossey, Laura</name>
      </author>
    </item>
    <item>
      <title>Forearc strike-slip displacement as an alternative to subduction erosion, with examples from Mexico and California (sinistral Nacimiento fault)1</title>
      <link>https://escholarship.org/uc/item/8gg8w059</link>
      <description>Slip on the Nacimiento fault of the central Coast Ranges of California has been variably interpreted as dextral, sinistral, or reverse. The currently prevailing interpretation is that the Nacimiento fault represents subduction erosion, by which the central to eastern part of the Cretaceous California batholith was thrust over the western part of the batholith and forearc basin, resulting in juxtaposition of the Salinian batholithic block against the Franciscan Complex, concurrently with Laramide flat-slab subduction (75–55 Ma) and underplating of the Pelona-Orocopia-Rand schist. No modern convergent plate margin includes such overthrusting. The closest modern analog to the likely configuration of the Salinian continental margin near the end of the Laramide deformation is southern Mexico, where arc plutons are exposed near the trench. Although commonly considered an example of subduction erosion, this margin is “missing” parts of the plutonic arc and forearc because they have been...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8gg8w059</guid>
      <pubDate>Wed, 17 Dec 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Ingersoll, Raymond V</name>
      </author>
    </item>
    <item>
      <title>Quantitative Analysis of Volcanic Lithic Fragments</title>
      <link>https://escholarship.org/uc/item/6mg6t3b6</link>
      <description>Textural subcategories of volcanic lithic fragments in sand and sandstone have been correlated qualitatively with volcanic compositional types, but these relationships have not been tested quantitatively. Lathwork grains were assumed to be derived mainly from mafic lavas, microlitic from intermediate lavas, and felsitic (sometimes divided into granular and seriate) from silicic lavas. Vitric volcanic lithic fragments were not initially assigned a composition, but they commonly have been associated with silicic compositions. More precise definitions of volcanic lithic types facilitate the quantification of modal proportions of these types, which can be used to test correlations between lithic type and SiO2 content of volcanic rocks. In order to establish which types of volcanic lithic fragments are produced by volcanic rocks of specific compositions, 94 thin sections from diverse volcanic rocks with 45.57 to 76.93 weight % SiO2 were counted using the Gazzi-Dickinson point-counting...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6mg6t3b6</guid>
      <pubDate>Wed, 17 Dec 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Affolter, Mathew D</name>
      </author>
      <author>
        <name>Ingersoll, Raymond V</name>
      </author>
    </item>
    <item>
      <title>Model for sinistral offset of the Cretaceous magmatic arc of southwestern North America along the Nacimiento fault system</title>
      <link>https://escholarship.org/uc/item/4pc8p51t</link>
      <description>Model for sinistral offset of the Cretaceous magmatic arc of southwestern North America along the Nacimiento fault system</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4pc8p51t</guid>
      <pubDate>Wed, 17 Dec 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Ingersoll, Raymond V</name>
      </author>
    </item>
    <item>
      <title>Kinematics and paleogeology of the western United States and northern Mexico computed from geologic and paleomagnetic data: 0 to 48 Ma</title>
      <link>https://escholarship.org/uc/item/4f70x90w</link>
      <description>Abstract
                  Fault traces and offsets, cross-section length changes, paleomagnetic inclination and declination anomalies, and stress-direction indicators with ages back to 90 Ma are collected from the geologic literature on the western United States and northern Mexico. Finite-element program Restore simulates paleokinematics by weighted least squares and integrates displacements, strains, and rotations back in time, producing paleogeologic maps, as well as maps of velocity, heave rate, strain rate, and stress direction at 6 m.y. intervals. After calibrating three program parameters against neotectonic velocities from geodesy, all classes of data except inclination anomalies are fit reasonably well. The kink in the San Andreas fault near San Gorgonio Pass has been gradually restored by slip on adjacent faults and automated smoothing. Piercing-point pairs successfully restored along the San Andreas–Gulf of California plate boundary include the Pelona and Orocopia...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4f70x90w</guid>
      <pubDate>Wed, 17 Dec 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Bird, Peter</name>
      </author>
      <author>
        <name>Ingersoll, Raymond V</name>
      </author>
    </item>
    <item>
      <title>Evaporitic Preservation of Modern Carotenoid Biomarkers and Halophilic Microorganisms in Mars Analog Hypersaline Environments</title>
      <link>https://escholarship.org/uc/item/0jm9s82j</link>
      <description>Our investigation in Mars-relevant terrestrial environments where biological material is entombed within rapidly precipitated evaporite crystals has given us the ability to evaluate the preservation potential of a hypersaline brine system in advance of interrogating similar environments on Mars. These evaporite minerals, halite (NaCl) and gypsum (CaSO&lt;sub&gt;4&lt;/sub&gt;), have been found to host authigenic fluid inclusions over geologic time, with cellular life and carotenoid pigments that are understudied in the planetary context. Great Salt Lake provides an excellent site to test the ability to detect organic matter in Mars-relevant evaporite crystals. DNA was extracted to determine which microbial clades were present and assess the attenuation of DNA preservation from the host fluid of the lake to the mineral. Raman spectroscopy was used to investigate the presence of pigments that have longer preservation potential than DNA. Compared with the water column, evaporite minerals preserve...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0jm9s82j</guid>
      <pubDate>Wed, 19 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Perl, Scott M</name>
        <uri>https://orcid.org/0000-0001-9228-9996</uri>
      </author>
      <author>
        <name>Baxter, Bonnie K</name>
      </author>
      <author>
        <name>Celestian, Aaron J</name>
      </author>
      <author>
        <name>Tasoff, Preston</name>
      </author>
      <author>
        <name>Seuylemezian, Arman</name>
      </author>
      <author>
        <name>Vaishampayan, Parag A</name>
      </author>
      <author>
        <name>Corsetti, Frank A</name>
      </author>
    </item>
    <item>
      <title>Seismic anisotropy layering in the Martian lowlands crust</title>
      <link>https://escholarship.org/uc/item/3rx5d55w</link>
      <description>The largest seismic event ever detected on Mars occurred on May 4, 2022, likely situated just north of the hemispherical dichotomy, east of the landing site, and south of Cerberus Fossae. This event was unique in that it generated both Love and Rayleigh waves, including fundamental and higher modes, providing us with a rare opportunity to determine whether seismic radial anisotropy is present on Mars. We performed non-linear waveform modeling and used a Niching Genetic Algorithm to find acceptable velocity models. Our analysis revealed that seismic anisotropy is necessary in the top 40&amp;nbsp;km, with the fast direction for seismic wave propagation being horizontal, similar to previous results solely based on fundamental mode surface wave group velocity dispersion. Our new models display layering with varying degrees of anisotropy. We found anisotropic parameter ξ&amp;nbsp;=&amp;nbsp;1.0-1.2 between 5 and 20&amp;nbsp;km depth and ξ&amp;nbsp;=&amp;nbsp;1.2-1.3 at 25–30&amp;nbsp;km depth. No significant...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3rx5d55w</guid>
      <pubDate>Wed, 22 Oct 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Beghein, C</name>
        <uri>https://orcid.org/0000-0002-3158-2213</uri>
      </author>
      <author>
        <name>Li, J</name>
      </author>
    </item>
    <item>
      <title>Toward a Cenozoic history of atmospheric CO2</title>
      <link>https://escholarship.org/uc/item/0tz7h903</link>
      <description>The geological record encodes the relationship between climate and atmospheric carbon dioxide (CO&lt;sub&gt;2&lt;/sub&gt;) over long and short timescales, as well as potential drivers of evolutionary transitions. However, reconstructing CO&lt;sub&gt;2&lt;/sub&gt; beyond direct measurements requires the use of paleoproxies and herein lies the challenge, as proxies differ in their assumptions, degree of understanding, and even reconstructed values. In this study, we critically evaluated, categorized, and integrated available proxies to create a high-fidelity and transparently constructed atmospheric CO&lt;sub&gt;2&lt;/sub&gt; record spanning the past 66 million years. This newly constructed record provides clearer evidence for higher Earth system sensitivity in the past and for the role of CO&lt;sub&gt;2&lt;/sub&gt; thresholds in biological and cryosphere evolution.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0tz7h903</guid>
      <pubDate>Thu, 9 Oct 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Consortium*†, The Cenozoic CO2 Proxy Integration Project</name>
      </author>
      <author>
        <name>Hönisch, Bärbel</name>
      </author>
      <author>
        <name>Royer, Dana L</name>
      </author>
      <author>
        <name>Breecker, Daniel O</name>
      </author>
      <author>
        <name>Polissar, Pratigya J</name>
        <uri>https://orcid.org/0000-0001-5483-1625</uri>
      </author>
      <author>
        <name>Bowen, Gabriel J</name>
      </author>
      <author>
        <name>Henehan, Michael J</name>
      </author>
      <author>
        <name>Cui, Ying</name>
      </author>
      <author>
        <name>Steinthorsdottir, Margret</name>
      </author>
      <author>
        <name>McElwain, Jennifer C</name>
      </author>
      <author>
        <name>Kohn, Matthew J</name>
      </author>
      <author>
        <name>Pearson, Ann</name>
      </author>
      <author>
        <name>Phelps, Samuel R</name>
      </author>
      <author>
        <name>Uno, Kevin T</name>
      </author>
      <author>
        <name>Ridgwell, Andy</name>
        <uri>https://orcid.org/0000-0003-2333-0128</uri>
      </author>
      <author>
        <name>Anagnostou, Eleni</name>
      </author>
      <author>
        <name>Austermann, Jacqueline</name>
      </author>
      <author>
        <name>Badger, Marcus PS</name>
      </author>
      <author>
        <name>Barclay, Richard S</name>
      </author>
      <author>
        <name>Bijl, Peter K</name>
      </author>
      <author>
        <name>Chalk, Thomas B</name>
      </author>
      <author>
        <name>Scotese, Christopher R</name>
      </author>
      <author>
        <name>de la Vega, Elwyn</name>
      </author>
      <author>
        <name>DeConto, Robert M</name>
      </author>
      <author>
        <name>Dyez, Kelsey A</name>
      </author>
      <author>
        <name>Ferrini, Vicki</name>
      </author>
      <author>
        <name>Franks, Peter J</name>
      </author>
      <author>
        <name>Giulivi, Claudia F</name>
      </author>
      <author>
        <name>Gutjahr, Marcus</name>
      </author>
      <author>
        <name>Harper, Dustin T</name>
      </author>
      <author>
        <name>Haynes, Laura L</name>
      </author>
      <author>
        <name>Huber, Matthew</name>
      </author>
      <author>
        <name>Snell, Kathryn E</name>
      </author>
      <author>
        <name>Keisling, Benjamin A</name>
      </author>
      <author>
        <name>Konrad, Wilfried</name>
      </author>
      <author>
        <name>Lowenstein, Tim K</name>
      </author>
      <author>
        <name>Malinverno, Alberto</name>
      </author>
      <author>
        <name>Guillermic, Maxence</name>
      </author>
      <author>
        <name>Mejía, Luz María</name>
      </author>
      <author>
        <name>Milligan, Joseph N</name>
      </author>
      <author>
        <name>Morton, John J</name>
      </author>
      <author>
        <name>Nordt, Lee</name>
      </author>
      <author>
        <name>Whiteford, Ross</name>
      </author>
      <author>
        <name>Roth-Nebelsick, Anita</name>
      </author>
      <author>
        <name>Rugenstein, Jeremy KC</name>
      </author>
      <author>
        <name>Schaller, Morgan F</name>
      </author>
      <author>
        <name>Sheldon, Nathan D</name>
      </author>
      <author>
        <name>Sosdian, Sindia</name>
      </author>
      <author>
        <name>Wilkes, Elise B</name>
      </author>
      <author>
        <name>Witkowski, Caitlyn R</name>
      </author>
      <author>
        <name>Zhang, Yi Ge</name>
      </author>
      <author>
        <name>Anderson, Lloyd</name>
      </author>
      <author>
        <name>Beerling, David J</name>
      </author>
      <author>
        <name>Bolton, Clara</name>
      </author>
      <author>
        <name>Cerling, Thure E</name>
      </author>
      <author>
        <name>Cotton, Jennifer M</name>
      </author>
      <author>
        <name>Da, Jiawei</name>
      </author>
      <author>
        <name>Ekart, Douglas D</name>
      </author>
      <author>
        <name>Foster, Gavin L</name>
      </author>
      <author>
        <name>Greenwood, David R</name>
      </author>
      <author>
        <name>Hyland, Ethan G</name>
      </author>
      <author>
        <name>Jagniecki, Elliot A</name>
      </author>
      <author>
        <name>Jasper, John P</name>
      </author>
      <author>
        <name>Kowalczyk, Jennifer B</name>
        <uri>https://orcid.org/0000-0003-2978-1237</uri>
      </author>
      <author>
        <name>Kunzmann, Lutz</name>
      </author>
      <author>
        <name>Kürschner, Wolfram M</name>
      </author>
      <author>
        <name>Lawrence, Charles E</name>
      </author>
      <author>
        <name>Lear, Caroline H</name>
      </author>
      <author>
        <name>Martínez-Botí, Miguel A</name>
      </author>
      <author>
        <name>Maxbauer, Daniel P</name>
      </author>
      <author>
        <name>Montagna, Paolo</name>
      </author>
      <author>
        <name>Naafs, B David A</name>
      </author>
      <author>
        <name>Rae, James WB</name>
      </author>
      <author>
        <name>Raitzsch, Markus</name>
      </author>
      <author>
        <name>Retallack, Gregory J</name>
      </author>
      <author>
        <name>Ring, Simon J</name>
      </author>
      <author>
        <name>Seki, Osamu</name>
      </author>
      <author>
        <name>Sepúlveda, Julio</name>
      </author>
      <author>
        <name>Sinha, Ashish</name>
      </author>
      <author>
        <name>Tesfamichael, Tekie F</name>
      </author>
      <author>
        <name>Tripati, Aradhna</name>
        <uri>https://orcid.org/0000-0002-1695-1754</uri>
      </author>
      <author>
        <name>van der Burgh, Johan</name>
      </author>
      <author>
        <name>Yu, Jimin</name>
      </author>
      <author>
        <name>Zachos, James C</name>
      </author>
      <author>
        <name>Zhang, Laiming</name>
      </author>
    </item>
    <item>
      <title>Atmospheric drivers of interannual variability from the northern hemisphere seasonal cap on Mars</title>
      <link>https://escholarship.org/uc/item/0fc0w43f</link>
      <description>Atmospheric drivers of interannual variability from the northern hemisphere seasonal cap on Mars</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0fc0w43f</guid>
      <pubDate>Tue, 30 Sep 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Widmer, Jacob M</name>
      </author>
      <author>
        <name>Diniega, Serina</name>
      </author>
      <author>
        <name>Day, Mackenzie</name>
        <uri>https://orcid.org/0000-0003-3998-7749</uri>
      </author>
      <author>
        <name>Cartwright, Samuel FA</name>
      </author>
      <author>
        <name>Alsaeed, Noora</name>
      </author>
    </item>
    <item>
      <title>Euclid</title>
      <link>https://escholarship.org/uc/item/917188fn</link>
      <description>The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Euclid is a medium-class mission in the Cosmic Vision 2015–2025 programme of the European Space Agency (ESA) that will provide high-resolution optical imaging, as well as near-infrared imaging and spectroscopy, over about 14 000 deg&lt;sup&gt;2&lt;/sup&gt; of extragalactic sky. In addition to accurate weak lensing and clustering measurements that probe structure formation over half of the age of the Universe, its primary probes for cosmology, these exquisite data will enable a wide range of science. This paper provides a high-level overview of the mission, summarising the survey characteristics, the various data-processing steps, and data products. We also highlight the main science objectives and expected performance.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/917188fn</guid>
      <pubDate>Mon, 22 Sep 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Mellier, Y</name>
      </author>
      <author>
        <name>Abdurro’uf</name>
      </author>
      <author>
        <name>Barroso, JA Acevedo</name>
      </author>
      <author>
        <name>Achúcarro, A</name>
      </author>
      <author>
        <name>Adamek, J</name>
      </author>
      <author>
        <name>Adam, R</name>
      </author>
      <author>
        <name>Addison, GE</name>
      </author>
      <author>
        <name>Aghanim, N</name>
      </author>
      <author>
        <name>Aguena, M</name>
      </author>
      <author>
        <name>Ajani, V</name>
      </author>
      <author>
        <name>Akrami, Y</name>
      </author>
      <author>
        <name>Al-Bahlawan, A</name>
      </author>
      <author>
        <name>Alavi, A</name>
      </author>
      <author>
        <name>Albuquerque, IS</name>
      </author>
      <author>
        <name>Alestas, G</name>
      </author>
      <author>
        <name>Alguero, G</name>
      </author>
      <author>
        <name>Allaoui, A</name>
      </author>
      <author>
        <name>Allen, SW</name>
      </author>
      <author>
        <name>Allevato, V</name>
      </author>
      <author>
        <name>Alonso-Tetilla, AV</name>
      </author>
      <author>
        <name>Altieri, B</name>
      </author>
      <author>
        <name>Alvarez-Candal, A</name>
      </author>
      <author>
        <name>Alvi, S</name>
      </author>
      <author>
        <name>Amara, A</name>
      </author>
      <author>
        <name>Amendola, L</name>
      </author>
      <author>
        <name>Amiaux, J</name>
      </author>
      <author>
        <name>Andika, IT</name>
      </author>
      <author>
        <name>Andreon, S</name>
      </author>
      <author>
        <name>Andrews, A</name>
      </author>
      <author>
        <name>Angora, G</name>
      </author>
      <author>
        <name>Angulo, RE</name>
      </author>
      <author>
        <name>Annibali, F</name>
      </author>
      <author>
        <name>Anselmi, A</name>
      </author>
      <author>
        <name>Anselmi, S</name>
      </author>
      <author>
        <name>Arcari, S</name>
      </author>
      <author>
        <name>Archidiacono, M</name>
      </author>
      <author>
        <name>Aricò, G</name>
      </author>
      <author>
        <name>Arnaud, M</name>
      </author>
      <author>
        <name>Arnouts, S</name>
      </author>
      <author>
        <name>Asgari, M</name>
      </author>
      <author>
        <name>Asorey, J</name>
      </author>
      <author>
        <name>Atayde, L</name>
      </author>
      <author>
        <name>Atek, H</name>
      </author>
      <author>
        <name>Atrio-Barandela, F</name>
      </author>
      <author>
        <name>Aubert, M</name>
      </author>
      <author>
        <name>Aubourg, E</name>
      </author>
      <author>
        <name>Auphan, T</name>
      </author>
      <author>
        <name>Auricchio, N</name>
      </author>
      <author>
        <name>Aussel, B</name>
      </author>
      <author>
        <name>Aussel, H</name>
      </author>
      <author>
        <name>Avelino, PP</name>
      </author>
      <author>
        <name>Avgoustidis, A</name>
      </author>
      <author>
        <name>Avila, S</name>
      </author>
      <author>
        <name>Awan, S</name>
      </author>
      <author>
        <name>Azzollini, R</name>
      </author>
      <author>
        <name>Baccigalupi, C</name>
      </author>
      <author>
        <name>Bachelet, E</name>
      </author>
      <author>
        <name>Bacon, D</name>
      </author>
      <author>
        <name>Baes, M</name>
      </author>
      <author>
        <name>Bagley, MB</name>
      </author>
      <author>
        <name>Bahr-Kalus, B</name>
      </author>
      <author>
        <name>Balaguera-Antolinez, A</name>
      </author>
      <author>
        <name>Balbinot, E</name>
      </author>
      <author>
        <name>Balcells, M</name>
      </author>
      <author>
        <name>Baldi, M</name>
      </author>
      <author>
        <name>Baldry, I</name>
      </author>
      <author>
        <name>Balestra, A</name>
      </author>
      <author>
        <name>Ballardini, M</name>
      </author>
      <author>
        <name>Ballester, O</name>
      </author>
      <author>
        <name>Balogh, M</name>
      </author>
      <author>
        <name>Bañados, E</name>
      </author>
      <author>
        <name>Barbier, R</name>
      </author>
      <author>
        <name>Bardelli, S</name>
      </author>
      <author>
        <name>Baron, M</name>
      </author>
      <author>
        <name>Barreiro, T</name>
      </author>
      <author>
        <name>Barrena, R</name>
      </author>
      <author>
        <name>Barriere, J-C</name>
      </author>
      <author>
        <name>Barros, BJ</name>
      </author>
      <author>
        <name>Barthelemy, A</name>
      </author>
      <author>
        <name>Bartolo, N</name>
      </author>
      <author>
        <name>Basset, A</name>
      </author>
      <author>
        <name>Battaglia, P</name>
      </author>
      <author>
        <name>Battisti, AJ</name>
      </author>
      <author>
        <name>Baugh, CM</name>
      </author>
      <author>
        <name>Baumont, L</name>
      </author>
      <author>
        <name>Bazzanini, L</name>
      </author>
      <author>
        <name>Beaulieu, J-P</name>
      </author>
      <author>
        <name>Beckmann, V</name>
      </author>
      <author>
        <name>Belikov, AN</name>
      </author>
      <author>
        <name>Bel, J</name>
      </author>
      <author>
        <name>Bellagamba, F</name>
      </author>
      <author>
        <name>Bella, M</name>
      </author>
      <author>
        <name>Bellini, E</name>
      </author>
      <author>
        <name>Benabed, K</name>
      </author>
      <author>
        <name>Bender, R</name>
      </author>
      <author>
        <name>Benevento, G</name>
      </author>
      <author>
        <name>Bennett, CL</name>
      </author>
      <author>
        <name>Benson, K</name>
      </author>
      <author>
        <name>Bergamini, P</name>
      </author>
      <author>
        <name>Bermejo-Climent, JR</name>
      </author>
    </item>
    <item>
      <title>Spatial evidence of cryptic methane cycling and methylotrophic metabolisms along a land–ocean transect in salt marsh sediment</title>
      <link>https://escholarship.org/uc/item/2bp4c2ws</link>
      <description>Spatial evidence of cryptic methane cycling and methylotrophic metabolisms along a land–ocean transect in salt marsh sediment</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2bp4c2ws</guid>
      <pubDate>Wed, 17 Sep 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Krause, Sebastian JE</name>
      </author>
      <author>
        <name>Wipfler, Rebecca</name>
      </author>
      <author>
        <name>Liu, Jiarui</name>
      </author>
      <author>
        <name>Yousavich, David J</name>
      </author>
      <author>
        <name>Robinson, DeMarcus</name>
      </author>
      <author>
        <name>Hoyt, David W</name>
      </author>
      <author>
        <name>Orphan, Victoria J</name>
      </author>
      <author>
        <name>Treude, Tina</name>
      </author>
    </item>
    <item>
      <title>Streamer‐Like Red Line Diffuse Auroras Driven by Time Domain Structures Associated With Electron Injection and Braking Ion Flows</title>
      <link>https://escholarship.org/uc/item/9h66s620</link>
      <description>Auroral streamers are important meso-scale processes that transport plasma and magnetic energy and drive dynamic magnetosphere-ionosphere (MI) coupling and space weather. Although streamers are typically studied using imagers sensitive to energetic ((Formula presented.) 1&amp;nbsp;keV) electron precipitation, such as all-sky imagers, some are associated with low-energy ((Formula presented.) 1&amp;nbsp;keV) precipitation better captured by red-line auroral emissions. This paper reports such streamer-like red-line auroras observed poleward of a black aurora and an auroral torch, associated with a magnetospheric electron injection and braking ion flows. Using conjugate space-ground observations, quasilinear theory, and auroral forward modeling, we establish the first direct linkage between streamer-like red-line auroras and plasma sheet electron pitch-angle scattering by time-domain structures. These results underscore the importance of wave-driven diffuse auroral processes in generating...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9h66s620</guid>
      <pubDate>Wed, 2 Jul 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Shen, Yangyang</name>
      </author>
      <author>
        <name>Zhang, Xu</name>
      </author>
      <author>
        <name>Liang, Jun</name>
      </author>
      <author>
        <name>Artemyev, Anton</name>
      </author>
      <author>
        <name>Angelopoulos, Vassilis</name>
        <uri>https://orcid.org/0000-0001-7024-1561</uri>
      </author>
      <author>
        <name>Spanswick, Emma</name>
      </author>
      <author>
        <name>Lyons, Larry</name>
      </author>
      <author>
        <name>Nishimura, Yukitoshi</name>
      </author>
    </item>
    <item>
      <title>Promises and pitfalls of source terrane prediction from inclusions in detrital zircon</title>
      <link>https://escholarship.org/uc/item/24h2456v</link>
      <description>Understanding the relationship between the assemblage of mineral inclusions trapped by an igneous zircon suite and the composition of the host magma is complicated by processes that preclude simple relationships between, for example, the relative proportions of modal mineral inclusions (e.g., quartz, alkali feldspar, and plagioclase; QAP) and the degree of magma differentiation. However, apatite and ferromagnesian inclusion abundances can be approximately related to the SiO2 content in some magmas, potentially allowing for broad inferences of source rock composition from detrital zircon mineral inclusion suites. This study presents mineral inclusion assemblages in igneous zircon from a wide range of magma compositions, tectono-magmatic settings, and geographic locations to better determine the correlation between major inclusion phases and source rock chemistry. We find that the relationship between apatite and whole rock SiO2 is strongly dependent on the aluminosity (as shown...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/24h2456v</guid>
      <pubDate>Wed, 2 Jul 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Bell, Elizabeth A</name>
      </author>
      <author>
        <name>Kirkpatrick, Heather M</name>
      </author>
      <author>
        <name>Harrison, T Mark</name>
      </author>
    </item>
    <item>
      <title>The Miscibility of Hydrogen and Water in Planetary Atmospheres and Interiors</title>
      <link>https://escholarship.org/uc/item/3r75d8g9</link>
      <description>Abstract: 

               Many planets in the solar system and across the Galaxy have hydrogen-rich atmospheres overlying more heavy element-rich interiors with which they interact for billions of years. Atmosphere–interior interactions are thus crucial to understanding the formation and evolution of these bodies. However, this understanding is still lacking in part because the relevant pressure–temperature conditions are extreme. We conduct molecular dynamics simulations based on density functional theory to investigate how hydrogen and water interact over a wide range of pressure and temperature, encompassing the interiors of Neptune-sized and smaller planets. We determine the critical curve at which a single homogeneous phase exsolves into two separate hydrogen-rich and water-rich phases, finding good agreement with existing experimental data. We find that the temperature along the critical curve increases with increasing pressure and shows the influence of a change in fluid...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3r75d8g9</guid>
      <pubDate>Fri, 11 Apr 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Gupta, Akash</name>
      </author>
      <author>
        <name>Stixrude, Lars</name>
      </author>
      <author>
        <name>Schlichting, Hilke E</name>
        <uri>https://orcid.org/0000-0002-0298-8089</uri>
      </author>
    </item>
    <item>
      <title>Reference genome for the endangered, genetically subdivided, northern tidewater goby, Eucyclogobius newberryi</title>
      <link>https://escholarship.org/uc/item/71h1j5zj</link>
      <description>The federally endangered sister species, Eucyclogobius newberryi (northern tidewater goby, NTG) and E. kristinae (southern tidewater goby) comprise the California endemic genus Eucyclogobius, which historically occurred in all coastal California counties. Isolated lagoons that only intermittently connect to the sea are their primary habitat. Reproduction occurs during lagoon closure, minimizing marine dispersal and generating the most genetically subdivided vertebrate genus on the California coast. We present a new genome assembly for E. newberryi using HiFi long reads and Hi-C chromatin-proximity sequencing. The 980 Mb E. newberryi reference genome has an N50 of 34 Mb with 22 well-described scaffolds comprising 88% of the genome and a complete BUSCO (Benchmarking Universal Single-Copy Orthologs) score of 96.7%. This genome will facilitate studies addressing selection, drift, and metapopulation genetics in subdivided populations, as well as the persistence of the critically endangered...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/71h1j5zj</guid>
      <pubDate>Tue, 1 Apr 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Jacobs, David K</name>
        <uri>https://orcid.org/0000-0002-7252-1601</uri>
      </author>
      <author>
        <name>Kinziger, Andrew</name>
      </author>
      <author>
        <name>Abrecht, Mira</name>
      </author>
      <author>
        <name>McCraney, W Tyler</name>
      </author>
      <author>
        <name>Hà, Benjamin A</name>
      </author>
      <author>
        <name>Spies, Brenton T</name>
      </author>
      <author>
        <name>Heath-Heckman, Elizabeth</name>
      </author>
      <author>
        <name>Marimuhtu, Mohan PA</name>
      </author>
      <author>
        <name>Nguyen, Oanh</name>
      </author>
      <author>
        <name>Fairbairn, Colin W</name>
      </author>
      <author>
        <name>Seligmann, William E</name>
        <uri>https://orcid.org/0000-0002-5762-3095</uri>
      </author>
      <author>
        <name>Escalona, Merly</name>
        <uri>https://orcid.org/0000-0003-0213-4777</uri>
      </author>
      <author>
        <name>Miller, Courtney</name>
      </author>
      <author>
        <name>Shaffer, H Bradley</name>
      </author>
    </item>
    <item>
      <title>Extreme two-phase change of ionospheric electron temperature overshoot during geomagnetic storms</title>
      <link>https://escholarship.org/uc/item/7156c41w</link>
      <description>An intense surge in the equatorial electron temperature (Te) at sunrise, known as the morning Te overshoot, has been one of the defining ionospheric features since its discovery early in the Space Age. Despite decades of study, the behavior of the morning overshoot during geomagnetic storms remains poorly understood. We report a two-stage response of the morning Te overshoot to geomagnetic activity, uncovered by a neural network model. Electron temperatures show an initial enhancement during the storm’s main phase, followed by a drastic depletion exceeding 1000 K and disappearance of the overshoot in the recovery phase. This two-phase change aligns with the early influence of westward prompt penetration electric field, overtaken by the development of the eastward disturbance dynamo later in the storm. These electric field changes affect vertical plasma drifts that redistribute electron densities, modifying ionospheric cooling rates. Our findings provide new insights into the dynamics...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7156c41w</guid>
      <pubDate>Tue, 1 Apr 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Smirnov, Artem</name>
      </author>
      <author>
        <name>Shprits, Yuri</name>
        <uri>https://orcid.org/0000-0002-9625-0834</uri>
      </author>
      <author>
        <name>Lühr, Hermann</name>
      </author>
      <author>
        <name>Pignalberi, Alessio</name>
      </author>
      <author>
        <name>Kronberg, Elena</name>
      </author>
      <author>
        <name>Prol, Fabricio</name>
      </author>
      <author>
        <name>Xiong, Chao</name>
      </author>
    </item>
    <item>
      <title>Remote Sensing of Electron Precipitation Mechanisms enabled by ELFIN Mission Operations and ADCS</title>
      <link>https://escholarship.org/uc/item/50n304k4</link>
      <description>The Electron Loss and Fields INvestigation (ELFIN) mission comprising two 3U+ CubeSats was developed, built, and operated by several generations of undergraduate students at UCLA. The spin-stabilized CubeSats (spin-rate: 21 RPM) produced high-resolution measurements of precipitating, trapped, and backscattered fluxes of electrons and ions in the radiation belts. Launched in September 2018, ELFIN operated successfully until its deorbit just over four years later. Initially, however, mission operations was very challenging and only tapped the full mission potential after a thorough redesign of the operations paradigm. This mid-mission adjustment yielded the higher data downlink volume necessary to acquire a comprehensive data set, therefore enabling ensemble studies with sufficient statistical significance. The new operational framework also led to additional improvements across the mission. Most notably, the Attitude Determination and Control System (ADCS) benefited from more reliable...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/50n304k4</guid>
      <pubDate>Wed, 12 Mar 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Tsai, Ethan</name>
      </author>
      <author>
        <name>Palla, Akhil</name>
      </author>
      <author>
        <name>Norris, Austin</name>
      </author>
      <author>
        <name>King, James</name>
      </author>
      <author>
        <name>Russell, Cindy</name>
      </author>
      <author>
        <name>Ye, Sophie</name>
      </author>
      <author>
        <name>Wu, Jiashu</name>
      </author>
      <author>
        <name>Mao, Jason</name>
      </author>
      <author>
        <name>Jha, Sharvani</name>
      </author>
      <author>
        <name>Young, Chanel</name>
      </author>
      <author>
        <name>Wing, Graham</name>
      </author>
      <author>
        <name>Lian, Kevin</name>
      </author>
      <author>
        <name>Szeto, Aiden</name>
      </author>
      <author>
        <name>Shiffer, James</name>
      </author>
      <author>
        <name>Sankar, Rishi</name>
      </author>
      <author>
        <name>Tota, Kaivalya</name>
      </author>
      <author>
        <name>Liu, Annie</name>
      </author>
      <author>
        <name>Lee, Derek</name>
      </author>
      <author>
        <name>Patil, Uma</name>
      </author>
      <author>
        <name>He, Isabella</name>
      </author>
      <author>
        <name>Tam, Jonathan</name>
      </author>
      <author>
        <name>McDermott, Alex</name>
      </author>
      <author>
        <name>Le, Katrina</name>
      </author>
      <author>
        <name>Kumar, Suyash</name>
      </author>
      <author>
        <name>Nguyen, Kelly</name>
      </author>
      <author>
        <name>Nguyen, Michelle</name>
      </author>
      <author>
        <name>Yap, Chen</name>
      </author>
      <author>
        <name>Xie, Erica</name>
      </author>
      <author>
        <name>Tseng, James</name>
      </author>
      <author>
        <name>Iglesias, Laura</name>
      </author>
      <author>
        <name>Roosnovo, Alexandra</name>
      </author>
      <author>
        <name>Turner, Wynne</name>
      </author>
      <author>
        <name>Curtis, Reed</name>
      </author>
      <author>
        <name>Wilkins, Colin</name>
      </author>
      <author>
        <name>Masongsong, Emmanuel</name>
      </author>
      <author>
        <name>Caron, Ryan</name>
      </author>
      <author>
        <name>Zhang, Xiao-Jia</name>
      </author>
      <author>
        <name>Artemyev, Anton</name>
      </author>
      <author>
        <name>Angelopoulos, Vassilis</name>
        <uri>https://orcid.org/0000-0001-7024-1561</uri>
      </author>
    </item>
    <item>
      <title>Listening to the Magnetosphere: How Best to Make ULF Waves Audible</title>
      <link>https://escholarship.org/uc/item/3jc5q45c</link>
      <description>Observations across the heliosphere typically rely on in situ spacecraft observations producing time-series data. While often this data is analysed visually, it lends itself more naturally to our sense of sound. The simplest method of converting oscillatory data into audible sound is audification—a one-to-one mapping of data samples to audio samples—which has the benefit that no information is lost, thus is a true representation of the original data. However, audification can make some magnetospheric ULF waves observations pass by too quickly for someone to realistically be able to listen to effectively. For this reason, we detail various existing audio time scale modification techniques developed for music, applying these to ULF wave observations by spacecraft and exploring how they affect the properties of the resulting audio. Through a public dialogue we arrive at recommendations for ULF wave researchers on rendering these waves audible and discuss the scientific and educational...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3jc5q45c</guid>
      <pubDate>Wed, 12 Mar 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Archer, Martin O</name>
      </author>
      <author>
        <name>Cottingham, Marek</name>
      </author>
      <author>
        <name>Hartinger, Michael D</name>
      </author>
      <author>
        <name>Shi, Xueling</name>
      </author>
      <author>
        <name>Coyle, Shane</name>
      </author>
      <author>
        <name>Hill, Ethan Duke</name>
      </author>
      <author>
        <name>Fox, Michael FJ</name>
      </author>
      <author>
        <name>Masongsong, Emmanuel V</name>
      </author>
    </item>
    <item>
      <title>Direct observations of cross-scale wave-particle energy transfer in space plasmas</title>
      <link>https://escholarship.org/uc/item/1r84n6w3</link>
      <description>The collisionless plasmas in space and astrophysical environments are intrinsically multiscale in nature, behaving as conducting fluids at macroscales and kinetically at microscales comparable to ion and/or electron gyroradii. A fundamental question in understanding the plasma dynamics is how energy is transported and dissipated across scales. Here, we present spacecraft measurements in the terrestrial foreshock, a region upstream of the bow shock where the solar wind population coexists with the reflected ions. In this region, the fluid-scale, ultralow-frequency waves resonate with the reflected ions to modify the velocity distributions, which in turn cause the growth of the ion-scale, magnetosonic-whistler waves. The latter waves then resonate with the electrons, and the accelerated electrons contribute to the excitation of electron-scale, high-frequency whistler waves. These observations demonstrate that the chain of wave-particle resonances is an efficient mechanism for cross-scale...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1r84n6w3</guid>
      <pubDate>Fri, 14 Feb 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Li, Jing-Huan</name>
      </author>
      <author>
        <name>Zhou, Xu-Zhi</name>
      </author>
      <author>
        <name>Liu, Zhi-Yang</name>
      </author>
      <author>
        <name>Wang, Shan</name>
      </author>
      <author>
        <name>Omura, Yoshiharu</name>
      </author>
      <author>
        <name>Li, Li</name>
      </author>
      <author>
        <name>Yue, Chao</name>
      </author>
      <author>
        <name>Zong, Qiu-Gang</name>
      </author>
      <author>
        <name>Le, Guan</name>
      </author>
      <author>
        <name>Russell, Christopher T</name>
        <uri>https://orcid.org/0000-0003-1639-8298</uri>
      </author>
      <author>
        <name>Burch, James L</name>
      </author>
    </item>
    <item>
      <title>Grain Size Measurements of the Eolian Stimson Formation, Gale Crater, Mars and Implications for Sand Provenance and Paleoatmospheric Conditions</title>
      <link>https://escholarship.org/uc/item/0mk750fk</link>
      <description>The Stimson formation is a late-infilling eolian sandstone in Gale crater, Mars that formed from sand accumulation in a dune field analogous to the modern active Bagnold dune field, enabling a unique opportunity to compare the past to the present dune fields on Mars. Previous work suggested that the Stimson has a coarser grain-size distribution than the active Bagnold dunes based on three images of the Stimson. We analyze grain size in the Naukluft and Emerson plateaus of the Stimson by observing 115 images throughout the formation to classify textures and quantitatively measuring grains in eight representative individual images. Results indicate that the Stimson has a primary grain size mode at &amp;lt;200&amp;nbsp;μm. In addition, more than 50% of the observed Stimson rock targets display a coarser grain population with a long-tailed distribution including grains ∼600–1200&amp;nbsp;μm. The primary grain size mode is similar to that observed in the Bagnold dunes, but the coarse grain size...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0mk750fk</guid>
      <pubDate>Wed, 29 Jan 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Preston, Sarah L</name>
        <uri>https://orcid.org/0000-0002-7571-1056</uri>
      </author>
      <author>
        <name>Siebach, Kirsten L</name>
      </author>
      <author>
        <name>Lapôtre, Mathieu GA</name>
      </author>
      <author>
        <name>Banham, Steven G</name>
      </author>
    </item>
    <item>
      <title>Compound electron acceleration at planetary foreshocks</title>
      <link>https://escholarship.org/uc/item/6v21z5cv</link>
      <description>Shock waves, the interface of supersonic and subsonic plasma flows, are the primary region for charged particle acceleration in multiple space plasma systems, including Earth’s bow shock, which is readily accessible for in-situ measurements. Spacecraft frequently observe relativistic electron populations within this region, characterized by energy levels surpassing those of solar wind electrons by a factor of 10,000 or more. However, mechanisms of such strong acceleration remain elusive. Here we use observations of electrons with energies up to 200 kiloelectron volts and a data-constrained model to reproduce the observed power-law electron spectrum and demonstrate that the acceleration by more than 4 orders of magnitude is a compound process including a complex, multi-step interaction between more commonly known mechanisms and resonant scattering by several distinct plasma wave modes. The proposed model of electron acceleration addresses a decades-long issue of the generation...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6v21z5cv</guid>
      <pubDate>Sat, 18 Jan 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Shi, Xiaofei</name>
        <uri>https://orcid.org/0000-0003-3367-5074</uri>
      </author>
      <author>
        <name>Artemyev, Anton</name>
      </author>
      <author>
        <name>Angelopoulos, Vassilis</name>
        <uri>https://orcid.org/0000-0001-7024-1561</uri>
      </author>
      <author>
        <name>Liu, Terry</name>
      </author>
      <author>
        <name>Wilson III, Lynn B</name>
      </author>
    </item>
    <item>
      <title>Contribution of Ryugu-like material to Earth’s volatile inventory by Cu and Zn isotopic analysis</title>
      <link>https://escholarship.org/uc/item/4680m2vs</link>
      <description>Initial analyses showed that asteroid Ryugu’s composition is close to CI (Ivuna-like) carbonaceous chondrites (CCs) – the chemically most primitive meteorites, characterized by near-solar abundances for most elements. However, some isotopic signatures (for example, Ti, Cr) overlap with other CC groups, so the details of the link between Ryugu and the CI chondrites are not yet fully clear. Here we show that Ryugu and CI chondrites have the same zinc and copper isotopic composition. As the various chondrite groups have very distinct Zn and Cu isotopic signatures, our results point at a common genetic heritage between Ryugu and CI chondrites, ruling out any affinity with other CC groups. Since Ryugu’s pristine samples match the solar elemental composition for many elements, their Zn and Cu isotopic compositions likely represent the best estimates of the solar composition. Earth’s mass-independent Zn isotopic composition is intermediate between Ryugu/CC and non-carbonaceous chondrites...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4680m2vs</guid>
      <pubDate>Thu, 16 Jan 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Paquet, Marine</name>
      </author>
      <author>
        <name>Moynier, Frederic</name>
      </author>
      <author>
        <name>Yokoyama, Tetsuya</name>
      </author>
      <author>
        <name>Dai, Wei</name>
      </author>
      <author>
        <name>Hu, Yan</name>
      </author>
      <author>
        <name>Abe, Yoshinari</name>
      </author>
      <author>
        <name>Aléon, Jérôme</name>
      </author>
      <author>
        <name>O’D. Alexander, Conel M</name>
      </author>
      <author>
        <name>Amari, Sachiko</name>
      </author>
      <author>
        <name>Amelin, Yuri</name>
      </author>
      <author>
        <name>Bajo, Ken-ichi</name>
      </author>
      <author>
        <name>Bizzarro, Martin</name>
      </author>
      <author>
        <name>Bouvier, Audrey</name>
      </author>
      <author>
        <name>Carlson, Richard W</name>
      </author>
      <author>
        <name>Chaussidon, Marc</name>
      </author>
      <author>
        <name>Choi, Byeon-Gak</name>
      </author>
      <author>
        <name>Dauphas, Nicolas</name>
      </author>
      <author>
        <name>Davis, Andrew M</name>
      </author>
      <author>
        <name>Di Rocco, Tommaso</name>
      </author>
      <author>
        <name>Fujiya, Wataru</name>
      </author>
      <author>
        <name>Fukai, Ryota</name>
      </author>
      <author>
        <name>Gautam, Ikshu</name>
      </author>
      <author>
        <name>Haba, Makiko K</name>
      </author>
      <author>
        <name>Hibiya, Yuki</name>
      </author>
      <author>
        <name>Hidaka, Hiroshi</name>
      </author>
      <author>
        <name>Homma, Hisashi</name>
      </author>
      <author>
        <name>Hoppe, Peter</name>
      </author>
      <author>
        <name>Huss, Gary R</name>
      </author>
      <author>
        <name>Ichida, Kiyohiro</name>
      </author>
      <author>
        <name>Iizuka, Tsuyoshi</name>
      </author>
      <author>
        <name>Ireland, Trevor R</name>
      </author>
      <author>
        <name>Ishikawa, Akira</name>
      </author>
      <author>
        <name>Ito, Motoo</name>
      </author>
      <author>
        <name>Itoh, Shoichi</name>
      </author>
      <author>
        <name>Kawasaki, Noriyuki</name>
      </author>
      <author>
        <name>Kita, Noriko T</name>
      </author>
      <author>
        <name>Kitajima, Kouki</name>
      </author>
      <author>
        <name>Kleine, Thorsten</name>
      </author>
      <author>
        <name>Komatani, Shintaro</name>
      </author>
      <author>
        <name>Krot, Alexander N</name>
      </author>
      <author>
        <name>Liu, Ming-Chang</name>
      </author>
      <author>
        <name>Masuda, Yuki</name>
      </author>
      <author>
        <name>McKeegan, Kevin D</name>
      </author>
      <author>
        <name>Morita, Mayu</name>
      </author>
      <author>
        <name>Motomura, Kazuko</name>
      </author>
      <author>
        <name>Nakai, Izumi</name>
      </author>
      <author>
        <name>Nagashima, Kazuhide</name>
      </author>
      <author>
        <name>Nesvorný, David</name>
      </author>
      <author>
        <name>Nguyen, Ann N</name>
      </author>
      <author>
        <name>Nittler, Larry</name>
      </author>
      <author>
        <name>Onose, Morihiko</name>
      </author>
      <author>
        <name>Pack, Andreas</name>
      </author>
      <author>
        <name>Park, Changkun</name>
      </author>
      <author>
        <name>Piani, Laurette</name>
      </author>
      <author>
        <name>Qin, Liping</name>
      </author>
      <author>
        <name>Russell, Sara S</name>
      </author>
      <author>
        <name>Sakamoto, Naoya</name>
      </author>
      <author>
        <name>Schönbächler, Maria</name>
      </author>
      <author>
        <name>Tafla, Lauren</name>
      </author>
      <author>
        <name>Tang, Haolan</name>
      </author>
      <author>
        <name>Terada, Kentaro</name>
      </author>
      <author>
        <name>Terada, Yasuko</name>
      </author>
      <author>
        <name>Usui, Tomohiro</name>
      </author>
      <author>
        <name>Wada, Sohei</name>
      </author>
      <author>
        <name>Wadhwa, Meenakshi</name>
      </author>
      <author>
        <name>Walker, Richard J</name>
      </author>
      <author>
        <name>Yamashita, Katsuyuki</name>
      </author>
      <author>
        <name>Yin, Qing-Zhu</name>
        <uri>https://orcid.org/0000-0002-4445-5096</uri>
      </author>
      <author>
        <name>Yoneda, Shigekazu</name>
      </author>
      <author>
        <name>Young, Edward D</name>
        <uri>https://orcid.org/0000-0002-1299-0801</uri>
      </author>
      <author>
        <name>Yui, Hiroharu</name>
      </author>
      <author>
        <name>Zhang, Ai-Cheng</name>
      </author>
      <author>
        <name>Nakamura, Tomoki</name>
      </author>
      <author>
        <name>Naraoka, Hiroshi</name>
      </author>
      <author>
        <name>Noguchi, Takaaki</name>
      </author>
      <author>
        <name>Okazaki, Ryuji</name>
      </author>
      <author>
        <name>Sakamoto, Kanako</name>
      </author>
      <author>
        <name>Yabuta, Hikaru</name>
      </author>
      <author>
        <name>Abe, Masanao</name>
      </author>
      <author>
        <name>Miyazaki, Akiko</name>
      </author>
      <author>
        <name>Nakato, Aiko</name>
      </author>
      <author>
        <name>Nishimura, Masahiro</name>
      </author>
      <author>
        <name>Okada, Tatsuaki</name>
      </author>
      <author>
        <name>Yada, Toru</name>
      </author>
      <author>
        <name>Yogata, Kasumi</name>
      </author>
      <author>
        <name>Nakazawa, Satoru</name>
      </author>
      <author>
        <name>Saiki, Takanao</name>
      </author>
      <author>
        <name>Tanaka, Satoshi</name>
      </author>
      <author>
        <name>Terui, Fuyuto</name>
      </author>
      <author>
        <name>Tsuda, Yuichi</name>
      </author>
      <author>
        <name>Watanabe, Sei-ichiro</name>
      </author>
      <author>
        <name>Yoshikawa, Makoto</name>
      </author>
      <author>
        <name>Tachibana, Shogo</name>
      </author>
      <author>
        <name>Yurimoto, Hisayoshi</name>
      </author>
    </item>
    <item>
      <title>Evidence for crustal seismic anisotropy at the InSight lander site</title>
      <link>https://escholarship.org/uc/item/8jm4p5nw</link>
      <description>Evidence for crustal seismic anisotropy at the InSight lander site</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8jm4p5nw</guid>
      <pubDate>Wed, 15 Jan 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Li, Jiaqi</name>
      </author>
      <author>
        <name>Beghein, Caroline</name>
        <uri>https://orcid.org/0000-0002-3158-2213</uri>
      </author>
      <author>
        <name>Wookey, James</name>
      </author>
      <author>
        <name>Davis, Paul</name>
      </author>
      <author>
        <name>Lognonné, Philippe</name>
      </author>
      <author>
        <name>Schimmel, Martin</name>
      </author>
      <author>
        <name>Stutzmann, Eleonore</name>
      </author>
      <author>
        <name>Golombek, Matthew</name>
      </author>
      <author>
        <name>Montagner, Jean-Paul</name>
      </author>
      <author>
        <name>Banerdt, William Bruce</name>
      </author>
    </item>
    <item>
      <title>Evaluation of the InSightSeers and DART Boarders mission observer programmes</title>
      <link>https://escholarship.org/uc/item/39q5j2f7</link>
      <description>Evaluation of the InSightSeers and DART Boarders mission observer programmes</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/39q5j2f7</guid>
      <pubDate>Wed, 15 Jan 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Fernando, Benjamin</name>
      </author>
      <author>
        <name>Newman, Claire</name>
      </author>
      <author>
        <name>Daubar, Ingrid J</name>
      </author>
      <author>
        <name>Beghein, Caroline</name>
        <uri>https://orcid.org/0000-0002-3158-2213</uri>
      </author>
      <author>
        <name>Chabot, Nancy L</name>
      </author>
      <author>
        <name>Irving, Jessica CE</name>
      </author>
      <author>
        <name>Johnson, Catherine L</name>
      </author>
      <author>
        <name>Panning, Mark P</name>
      </author>
      <author>
        <name>Plesa, Ana-Catalina</name>
      </author>
      <author>
        <name>Rivkin, Andrew S</name>
      </author>
      <author>
        <name>Smrekar, Sue</name>
      </author>
      <author>
        <name>Banerdt, W Bruce</name>
      </author>
    </item>
    <item>
      <title>Analysis of Cation Composition in Dolomites on the Intact Particles Sampled from Asteroid Ryugu</title>
      <link>https://escholarship.org/uc/item/7sg1v7g0</link>
      <description>Characterization of the elemental distribution of samples with rough surfaces has been strongly desired for the analysis of various natural and artificial materials. Particularly for pristine and rare analytes with micrometer sizes embedded on specimen surfaces, non-invasive and matrix effect-free analysis is required without surface polishing treatment. To satisfy these requirements, we proposed a new method employing the sequential combination of two imaging modalities, i.e., microenergy-dispersive X-ray fluorescence (micro-XRF) and Raman micro-spectroscopy. The applicability of the developed method is tested by the quantitative analysis of cation composition in micrometer-sized carbonate grains on the surfaces of intact particles sampled directly from the asteroid Ryugu. The first step of micro-XRF imaging enabled a quick search for the sparsely scattered and micrometer-sized carbonates by the codistributions of Ca&lt;sup&gt;2+&lt;/sup&gt; and Mn&lt;sup&gt;2+&lt;/sup&gt; on the Mg&lt;sup&gt;2+&lt;/sup&gt;- and...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7sg1v7g0</guid>
      <pubDate>Tue, 31 Dec 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Morita, Mayu</name>
      </author>
      <author>
        <name>Yui, Hiroharu</name>
      </author>
      <author>
        <name>Urashima, Shu-hei</name>
      </author>
      <author>
        <name>Onose, Morihiko</name>
      </author>
      <author>
        <name>Komatani, Shintaro</name>
      </author>
      <author>
        <name>Nakai, Izumi</name>
      </author>
      <author>
        <name>Abe, Yoshinari</name>
      </author>
      <author>
        <name>Terada, Yasuko</name>
      </author>
      <author>
        <name>Homma, Hisashi</name>
      </author>
      <author>
        <name>Motomura, Kazuko</name>
      </author>
      <author>
        <name>Ichida, Kiyohiro</name>
      </author>
      <author>
        <name>Yokoyama, Tetsuya</name>
      </author>
      <author>
        <name>Nagashima, Kazuhide</name>
      </author>
      <author>
        <name>Aléon, Jérôme</name>
      </author>
      <author>
        <name>Alexander, Conel M O’D</name>
      </author>
      <author>
        <name>Amari, Sachiko</name>
      </author>
      <author>
        <name>Amelin, Yuri</name>
      </author>
      <author>
        <name>Bajo, Ken-ichi</name>
      </author>
      <author>
        <name>Bizzarro, Martin</name>
      </author>
      <author>
        <name>Bouvier, Audrey</name>
      </author>
      <author>
        <name>Carlson, Richard W</name>
      </author>
      <author>
        <name>Chaussidon, Marc</name>
      </author>
      <author>
        <name>Choi, Byeon-Gak</name>
      </author>
      <author>
        <name>Dauphas, Nicolas</name>
      </author>
      <author>
        <name>Davis, Andrew M</name>
      </author>
      <author>
        <name>Fujiya, Wataru</name>
      </author>
      <author>
        <name>Fukai, Ryota</name>
      </author>
      <author>
        <name>Gautam, Ikshu</name>
      </author>
      <author>
        <name>Haba, Makiko K</name>
      </author>
      <author>
        <name>Hibiya, Yuki</name>
      </author>
      <author>
        <name>Hidaka, Hiroshi</name>
      </author>
      <author>
        <name>Hoppe, Peter</name>
      </author>
      <author>
        <name>Huss, Gary R</name>
      </author>
      <author>
        <name>Iizuka, Tsuyoshi</name>
      </author>
      <author>
        <name>Ireland, Trevor R</name>
      </author>
      <author>
        <name>Ishikawa, Akira</name>
      </author>
      <author>
        <name>Itoh, Shoichi</name>
      </author>
      <author>
        <name>Kawasaki, Noriyuki</name>
      </author>
      <author>
        <name>Kita, Noriko T</name>
      </author>
      <author>
        <name>Kitajima, Kouki</name>
      </author>
      <author>
        <name>Kleine, Thorsten</name>
      </author>
      <author>
        <name>Krot, Sasha</name>
      </author>
      <author>
        <name>Liu, Ming-Chang</name>
      </author>
      <author>
        <name>Masuda, Yuki</name>
      </author>
      <author>
        <name>Moynier, Frédéric</name>
      </author>
      <author>
        <name>Nguyen, Ann</name>
      </author>
      <author>
        <name>Nittler, Larry</name>
      </author>
      <author>
        <name>Pack, Andreas</name>
      </author>
      <author>
        <name>Park, Changkun</name>
      </author>
      <author>
        <name>Piani, Laurette</name>
      </author>
      <author>
        <name>Qin, Liping</name>
      </author>
      <author>
        <name>Di Rocco, Tommaso</name>
      </author>
      <author>
        <name>Russell, Sara S</name>
      </author>
      <author>
        <name>Sakamoto, Naoya</name>
      </author>
      <author>
        <name>Schönbächler, Maria</name>
      </author>
      <author>
        <name>Tafla, Lauren</name>
      </author>
      <author>
        <name>Tang, Haolan</name>
      </author>
      <author>
        <name>Terada, Kentaro</name>
      </author>
      <author>
        <name>Usui, Tomohiro</name>
      </author>
      <author>
        <name>Wada, Sohei</name>
      </author>
      <author>
        <name>Wadhwa, Meenakshi</name>
      </author>
      <author>
        <name>Walker, Richard J</name>
      </author>
      <author>
        <name>Yamashita, Katsuyuki</name>
      </author>
      <author>
        <name>Yin, Qing-Zhu</name>
        <uri>https://orcid.org/0000-0002-4445-5096</uri>
      </author>
      <author>
        <name>Yoneda, Shigekazu</name>
      </author>
      <author>
        <name>Young, Edward D</name>
        <uri>https://orcid.org/0000-0002-1299-0801</uri>
      </author>
      <author>
        <name>Zhang, Ai-Cheng</name>
      </author>
      <author>
        <name>Nakamura, Tomoki</name>
      </author>
      <author>
        <name>Naraoka, Hiroshi</name>
      </author>
      <author>
        <name>Noguchi, Takaaki</name>
      </author>
      <author>
        <name>Okazaki, Ryuji</name>
      </author>
      <author>
        <name>Sakamoto, Kanako</name>
      </author>
      <author>
        <name>Yabuta, Hikaru</name>
      </author>
      <author>
        <name>Abe, Masanao</name>
      </author>
      <author>
        <name>Miyazaki, Akiko</name>
      </author>
      <author>
        <name>Nakato, Aiko</name>
      </author>
      <author>
        <name>Nishimura, Masahiro</name>
      </author>
      <author>
        <name>Okada, Tatsuaki</name>
      </author>
      <author>
        <name>Yada, Toru</name>
      </author>
      <author>
        <name>Yogata, Kasumi</name>
      </author>
      <author>
        <name>Nakazawa, Satoru</name>
      </author>
      <author>
        <name>Saiki, Takanao</name>
      </author>
      <author>
        <name>Tanaka, Satoshi</name>
      </author>
      <author>
        <name>Terui, Fuyuto</name>
      </author>
      <author>
        <name>Tsuda, Yuichi</name>
      </author>
      <author>
        <name>Watanabe, Sei-ichiro</name>
      </author>
      <author>
        <name>Yoshikawa, Makoto</name>
      </author>
      <author>
        <name>Tachibana, Shogo</name>
      </author>
      <author>
        <name>Yurimoto, Hisayoshi</name>
      </author>
    </item>
    <item>
      <title>Ryugu’s nucleosynthetic heritage from the outskirts of the Solar System</title>
      <link>https://escholarship.org/uc/item/3z11n3n5</link>
      <description>Little is known about the origin of the spectral diversity of asteroids and what it says about conditions in the protoplanetary disk. Here, we show that samples returned from Cb-type asteroid Ryugu have Fe isotopic anomalies indistinguishable from Ivuna-type (CI) chondrites, which are distinct from all other carbonaceous chondrites. Iron isotopes, therefore, demonstrate that Ryugu and CI chondrites formed in a reservoir that was different from the source regions of other carbonaceous asteroids. Growth and migration of the giant planets destabilized nearby planetesimals and ejected some inward to be implanted into the Main Belt. In this framework, most carbonaceous chondrites may have originated from regions around the birthplaces of Jupiter and Saturn, while the distinct isotopic composition of CI chondrites and Ryugu may reflect their formation further away in the disk, owing their presence in the inner Solar System to excitation by Uranus and Neptune.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3z11n3n5</guid>
      <pubDate>Wed, 11 Dec 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Hopp, Timo</name>
      </author>
      <author>
        <name>Dauphas, Nicolas</name>
      </author>
      <author>
        <name>Abe, Yoshinari</name>
      </author>
      <author>
        <name>Aléon, Jérôme</name>
      </author>
      <author>
        <name>Alexander, Conel M O’D</name>
      </author>
      <author>
        <name>Amari, Sachiko</name>
      </author>
      <author>
        <name>Amelin, Yuri</name>
      </author>
      <author>
        <name>Bajo, Ken-ichi</name>
      </author>
      <author>
        <name>Bizzarro, Martin</name>
      </author>
      <author>
        <name>Bouvier, Audrey</name>
      </author>
      <author>
        <name>Carlson, Richard W</name>
      </author>
      <author>
        <name>Chaussidon, Marc</name>
      </author>
      <author>
        <name>Choi, Byeon-Gak</name>
      </author>
      <author>
        <name>Davis, Andrew M</name>
      </author>
      <author>
        <name>Di Rocco, Tommaso</name>
      </author>
      <author>
        <name>Fujiya, Wataru</name>
      </author>
      <author>
        <name>Fukai, Ryota</name>
      </author>
      <author>
        <name>Gautam, Ikshu</name>
      </author>
      <author>
        <name>Haba, Makiko K</name>
      </author>
      <author>
        <name>Hibiya, Yuki</name>
      </author>
      <author>
        <name>Hidaka, Hiroshi</name>
      </author>
      <author>
        <name>Homma, Hisashi</name>
      </author>
      <author>
        <name>Hoppe, Peter</name>
      </author>
      <author>
        <name>Huss, Gary R</name>
      </author>
      <author>
        <name>Ichida, Kiyohiro</name>
      </author>
      <author>
        <name>Iizuka, Tsuyoshi</name>
      </author>
      <author>
        <name>Ireland, Trevor R</name>
      </author>
      <author>
        <name>Ishikawa, Akira</name>
      </author>
      <author>
        <name>Ito, Motoo</name>
      </author>
      <author>
        <name>Itoh, Shoichi</name>
      </author>
      <author>
        <name>Kawasaki, Noriyuki</name>
      </author>
      <author>
        <name>Kita, Noriko T</name>
      </author>
      <author>
        <name>Kitajima, Kouki</name>
      </author>
      <author>
        <name>Kleine, Thorsten</name>
      </author>
      <author>
        <name>Komatani, Shintaro</name>
      </author>
      <author>
        <name>Krot, Alexander N</name>
      </author>
      <author>
        <name>Liu, Ming-Chang</name>
      </author>
      <author>
        <name>Masuda, Yuki</name>
      </author>
      <author>
        <name>McKeegan, Kevin D</name>
      </author>
      <author>
        <name>Morita, Mayu</name>
      </author>
      <author>
        <name>Motomura, Kazuko</name>
      </author>
      <author>
        <name>Moynier, Frédéric</name>
      </author>
      <author>
        <name>Nakai, Izumi</name>
      </author>
      <author>
        <name>Nagashima, Kazuhide</name>
      </author>
      <author>
        <name>Nesvorný, David</name>
      </author>
      <author>
        <name>Nguyen, Ann</name>
      </author>
      <author>
        <name>Nittler, Larry</name>
      </author>
      <author>
        <name>Onose, Morihiko</name>
      </author>
      <author>
        <name>Pack, Andreas</name>
      </author>
      <author>
        <name>Park, Changkun</name>
      </author>
      <author>
        <name>Piani, Laurette</name>
      </author>
      <author>
        <name>Qin, Liping</name>
      </author>
      <author>
        <name>Russell, Sara S</name>
      </author>
      <author>
        <name>Sakamoto, Naoya</name>
      </author>
      <author>
        <name>Schönbächler, Maria</name>
      </author>
      <author>
        <name>Tafla, Lauren</name>
      </author>
      <author>
        <name>Tang, Haolan</name>
      </author>
      <author>
        <name>Terada, Kentaro</name>
      </author>
      <author>
        <name>Terada, Yasuko</name>
      </author>
      <author>
        <name>Usui, Tomohiro</name>
      </author>
      <author>
        <name>Wada, Sohei</name>
      </author>
      <author>
        <name>Wadhwa, Meenakshi</name>
      </author>
      <author>
        <name>Walker, Richard J</name>
      </author>
      <author>
        <name>Yamashita, Katsuyuki</name>
      </author>
      <author>
        <name>Yin, Qing-Zhu</name>
        <uri>https://orcid.org/0000-0002-4445-5096</uri>
      </author>
      <author>
        <name>Yokoyama, Tetsuya</name>
      </author>
      <author>
        <name>Yoneda, Shigekazu</name>
      </author>
      <author>
        <name>Young, Edward D</name>
        <uri>https://orcid.org/0000-0002-1299-0801</uri>
      </author>
      <author>
        <name>Yui, Hiroharu</name>
      </author>
      <author>
        <name>Zhang, Ai-Cheng</name>
      </author>
      <author>
        <name>Nakamura, Tomoki</name>
      </author>
      <author>
        <name>Naraoka, Hiroshi</name>
      </author>
      <author>
        <name>Noguchi, Takaaki</name>
      </author>
      <author>
        <name>Okazaki, Ryuji</name>
      </author>
      <author>
        <name>Sakamoto, Kanako</name>
      </author>
      <author>
        <name>Yabuta, Hikaru</name>
      </author>
      <author>
        <name>Abe, Masanao</name>
      </author>
      <author>
        <name>Miyazaki, Akiko</name>
      </author>
      <author>
        <name>Nakato, Aiko</name>
      </author>
      <author>
        <name>Nishimura, Masahiro</name>
      </author>
      <author>
        <name>Okada, Tatsuaki</name>
      </author>
      <author>
        <name>Yada, Toru</name>
      </author>
      <author>
        <name>Yogata, Kasumi</name>
      </author>
      <author>
        <name>Nakazawa, Satoru</name>
      </author>
      <author>
        <name>Saiki, Takanao</name>
      </author>
      <author>
        <name>Tanaka, Satoshi</name>
      </author>
      <author>
        <name>Terui, Fuyuto</name>
      </author>
      <author>
        <name>Tsuda, Yuichi</name>
      </author>
      <author>
        <name>Watanabe, Sei-ichiro</name>
      </author>
      <author>
        <name>Yoshikawa, Makoto</name>
      </author>
      <author>
        <name>Tachibana, Shogo</name>
      </author>
      <author>
        <name>Yurimoto, Hisayoshi</name>
      </author>
    </item>
    <item>
      <title>Magnetospheric Control of Ionospheric TEC Perturbations via Whistler‐Mode and ULF Waves</title>
      <link>https://escholarship.org/uc/item/7zc8s84m</link>
      <description>The weakly ionized plasma in the Earth's ionosphere is controlled by a complex interplay between solar and magnetospheric inputs from above, atmospheric processes from below, and plasma electrodynamics from within. This interaction results in ionosphere structuring and variability that pose major challenges for accurate ionosphere prediction for global navigation satellite system (GNSS) related applications and space weather research. The ionospheric structuring and variability are often probed using the total electron content (TEC) and its relative perturbations (dTEC). Among dTEC variations observed at high latitudes, a unique modulation pattern has been linked to magnetospheric ultra-low-frequency (ULF) waves, yet its underlying mechanisms remain unclear. Here using magnetically conjugate observations from the THEMIS spacecraft and a ground-based GPS receiver at Fairbanks, Alaska, we provide direct evidence that these dTEC modulations are driven by magnetospheric electron precipitation...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7zc8s84m</guid>
      <pubDate>Tue, 3 Dec 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Shen, Yangyang</name>
      </author>
      <author>
        <name>Verkhoglyadova, Olga P</name>
      </author>
      <author>
        <name>Artemyev, Anton</name>
      </author>
      <author>
        <name>Hartinger, Michael D</name>
      </author>
      <author>
        <name>Angelopoulos, Vassilis</name>
        <uri>https://orcid.org/0000-0001-7024-1561</uri>
      </author>
      <author>
        <name>Shi, Xueling</name>
      </author>
      <author>
        <name>Zou, Ying</name>
      </author>
    </item>
    <item>
      <title>Polyether-based polyurethane electrolyte for lithium metal battery: a perspective</title>
      <link>https://escholarship.org/uc/item/4f23k9dz</link>
      <description>Polyurethane (PU)-based electrolyte has become one of the most important research directions because of its unique repeating 'soft-hard' segment co-polymer structure. Its 'soft segment' composition includes polyethylene oxide, polysiloxane, polycarbonate, cellulose and polyether. Among them, polyether-based polyurethane electrolytes (PPES) have the advantages of simple synthesis, molecular structure optimization and functional group modification, which can greatly improve the ionic conductivity of the system and form a good ion transport interface. To date, a few separate and detailed reviews of advances in PPES have been reported. In this paper, the research progress of PPES is reviewed from the aspects of structural design strategy, molecular synthesis, conductivity modification methods, specific functions and interfacial ion transport behavior in lithium metal batteries (LMBs). In addition, the synthetic route of PPES and the development prospect of PPES are discussed. We also...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4f23k9dz</guid>
      <pubDate>Mon, 2 Dec 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Cui, Peng</name>
      </author>
      <author>
        <name>Li, Yifan</name>
      </author>
      <author>
        <name>Liu, YuXing</name>
      </author>
      <author>
        <name>Wang, Siqi</name>
      </author>
      <author>
        <name>Tang, Xingyu</name>
      </author>
      <author>
        <name>Ye, Yihong</name>
      </author>
      <author>
        <name>Su, Hance</name>
      </author>
      <author>
        <name>Sun, Chun</name>
        <uri>https://orcid.org/0009-0005-1093-2164</uri>
      </author>
    </item>
    <item>
      <title>The effects of bathymetry on the long-term carbon cycle and CCD</title>
      <link>https://escholarship.org/uc/item/5r77d626</link>
      <description>The shape of the ocean floor (bathymetry) and the overlaying sediments provide the largest carbon sink throughout Earth's history, supporting ~one to two orders of magnitude more carbon storage than the oceans and atmosphere combined. While accumulation and erosion of these sediments are bathymetry dependent (e.g., due to pressure, temperature, salinity, ion concentration, and available productivity), no systemic study has quantified how global and basin scale bathymetry, controlled by the evolution of tectonics and mantle convection, affects the long-term carbon cycle. We reconstruct bathymetry spanning the last 80 Myr to describe steady-state changes in ocean chemistry within the Earth system model LOSCAR. We find that both bathymetry reconstructions and representative synthetic tests show that ocean alkalinity, calcite saturation state, and the carbonate compensation depth (CCD) are strongly dependent on changes in shallow bathymetry (ocean floor ≤600 m) and on the distribution...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5r77d626</guid>
      <pubDate>Mon, 25 Nov 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Bogumil, Matthew</name>
      </author>
      <author>
        <name>Mittal, Tushar</name>
      </author>
      <author>
        <name>Lithgow-Bertelloni, Carolina</name>
        <uri>https://orcid.org/0000-0003-0924-6587</uri>
      </author>
    </item>
    <item>
      <title>Species-resolved, single-cell respiration rates reveal dominance of sulfate reduction in a deep continental subsurface ecosystem</title>
      <link>https://escholarship.org/uc/item/6v2534r0</link>
      <description>Rates of microbial processes are fundamental to understanding the significance of microbial impacts on environmental chemical cycling. However, it is often difficult to quantify rates or to link processes to specific taxa or individual cells, especially in environments where there are few cultured representatives with known physiology. Here, we describe the use of the redox-enzyme-sensitive molecular probe RedoxSensor™ Green to measure rates of anaerobic electron transfer physiology (i.e., sulfate reduction and methanogenesis) in individual cells and link those measurements to genomic sequencing of the same single cells. We used this method to investigate microbial activity in hot, anoxic, low-biomass (~10&lt;sup&gt;3&lt;/sup&gt; cells mL&lt;sup&gt;-1&lt;/sup&gt;) groundwater of the Death Valley Regional Flow System, California. Combining this method with electron donor amendment experiments and metatranscriptomics confirmed that the abundant spore formers including &lt;i&gt;Candidatus&lt;/i&gt; Desulforudis audaxviator...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6v2534r0</guid>
      <pubDate>Tue, 5 Nov 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Lindsay, Melody R</name>
      </author>
      <author>
        <name>D’Angelo, Timothy</name>
      </author>
      <author>
        <name>Munson-McGee, Jacob H</name>
      </author>
      <author>
        <name>Saidi-Mehrabad, Alireza</name>
      </author>
      <author>
        <name>Devlin, Molly</name>
      </author>
      <author>
        <name>McGonigle, Julia</name>
      </author>
      <author>
        <name>Goodell, Elizabeth</name>
      </author>
      <author>
        <name>Herring, Melissa</name>
      </author>
      <author>
        <name>Lubelczyk, Laura C</name>
      </author>
      <author>
        <name>Mascena, Corianna</name>
      </author>
      <author>
        <name>Brown, Julia M</name>
      </author>
      <author>
        <name>Gavelis, Greg</name>
      </author>
      <author>
        <name>Liu, Jiarui</name>
      </author>
      <author>
        <name>Yousavich, DJ</name>
      </author>
      <author>
        <name>Hamilton-Brehm, Scott D</name>
      </author>
      <author>
        <name>Hedlund, Brian P</name>
      </author>
      <author>
        <name>Lang, Susan</name>
      </author>
      <author>
        <name>Treude, Tina</name>
      </author>
      <author>
        <name>Poulton, Nicole J</name>
      </author>
      <author>
        <name>Stepanauskas, Ramunas</name>
      </author>
      <author>
        <name>Moser, Duane P</name>
      </author>
      <author>
        <name>Emerson, David</name>
      </author>
      <author>
        <name>Orcutt, Beth N</name>
      </author>
    </item>
    <item>
      <title>The Ni isotopic composition of Ryugu reveals a common accretion region for carbonaceous chondrites</title>
      <link>https://escholarship.org/uc/item/1wj1r5zz</link>
      <description>The isotopic compositions of samples returned from Cb-type asteroid Ryugu and Ivuna-type (CI) chondrites are distinct from other carbonaceous chondrites, which has led to the suggestion that Ryugu/CI chondrites formed in a different region of the accretion disk, possibly around the orbits of Uranus and Neptune. We show that, like for Fe, Ryugu and CI chondrites also have indistinguishable Ni isotope anomalies, which differ from those of other carbonaceous chondrites. We propose that this unique Fe and Ni isotopic composition reflects different accretion efficiencies of small FeNi metal grains among the carbonaceous chondrite parent bodies. The CI chondrites incorporated these grains more efficiently, possibly because they formed at the end of the disk's lifetime, when planetesimal formation was also triggered by photoevaporation of the disk. Isotopic variations among carbonaceous chondrites may thus reflect fractionation of distinct dust components from a common reservoir, implying...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1wj1r5zz</guid>
      <pubDate>Wed, 30 Oct 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Spitzer, Fridolin</name>
      </author>
      <author>
        <name>Kleine, Thorsten</name>
      </author>
      <author>
        <name>Burkhardt, Christoph</name>
      </author>
      <author>
        <name>Hopp, Timo</name>
      </author>
      <author>
        <name>Yokoyama, Tetsuya</name>
      </author>
      <author>
        <name>Abe, Yoshinari</name>
      </author>
      <author>
        <name>Aléon, Jérôme</name>
      </author>
      <author>
        <name>Alexander, Conel M O’D</name>
      </author>
      <author>
        <name>Amari, Sachiko</name>
      </author>
      <author>
        <name>Amelin, Yuri</name>
      </author>
      <author>
        <name>Bajo, Ken-ichi</name>
      </author>
      <author>
        <name>Bizzarro, Martin</name>
      </author>
      <author>
        <name>Bouvier, Audrey</name>
      </author>
      <author>
        <name>Carlson, Richard W</name>
      </author>
      <author>
        <name>Chaussidon, Marc</name>
      </author>
      <author>
        <name>Choi, Byeon-Gak</name>
      </author>
      <author>
        <name>Dauphas, Nicolas</name>
      </author>
      <author>
        <name>Davis, Andrew M</name>
      </author>
      <author>
        <name>Di Rocco, Tommaso</name>
      </author>
      <author>
        <name>Fujiya, Wataru</name>
      </author>
      <author>
        <name>Fukai, Ryota</name>
      </author>
      <author>
        <name>Gautam, Ikshu</name>
      </author>
      <author>
        <name>Haba, Makiko K</name>
      </author>
      <author>
        <name>Hibiya, Yuki</name>
      </author>
      <author>
        <name>Hidaka, Hiroshi</name>
      </author>
      <author>
        <name>Homma, Hisashi</name>
      </author>
      <author>
        <name>Hoppe, Peter</name>
      </author>
      <author>
        <name>Huss, Gary R</name>
      </author>
      <author>
        <name>Ichida, Kiyohiro</name>
      </author>
      <author>
        <name>Iizuka, Tsuyoshi</name>
      </author>
      <author>
        <name>Ireland, Trevor R</name>
      </author>
      <author>
        <name>Ishikawa, Akira</name>
      </author>
      <author>
        <name>Itoh, Shoichi</name>
      </author>
      <author>
        <name>Kawasaki, Noriyuki</name>
      </author>
      <author>
        <name>Kita, Noriko T</name>
      </author>
      <author>
        <name>Kitajima, Kouki</name>
      </author>
      <author>
        <name>Komatani, Shintaro</name>
      </author>
      <author>
        <name>Krot, Alexander N</name>
      </author>
      <author>
        <name>Liu, Ming-Chang</name>
      </author>
      <author>
        <name>Masuda, Yuki</name>
      </author>
      <author>
        <name>Morita, Mayu</name>
      </author>
      <author>
        <name>Moynier, Fréderic</name>
      </author>
      <author>
        <name>Motomura, Kazuko</name>
      </author>
      <author>
        <name>Nakai, Izumi</name>
      </author>
      <author>
        <name>Nagashima, Kazuhide</name>
      </author>
      <author>
        <name>Nguyen, Ann</name>
      </author>
      <author>
        <name>Nittler, Larry</name>
      </author>
      <author>
        <name>Onose, Morihiko</name>
      </author>
      <author>
        <name>Pack, Andreas</name>
      </author>
      <author>
        <name>Park, Changkun</name>
      </author>
      <author>
        <name>Piani, Laurette</name>
      </author>
      <author>
        <name>Qin, Liping</name>
      </author>
      <author>
        <name>Russell, Sara S</name>
      </author>
      <author>
        <name>Sakamoto, Naoya</name>
      </author>
      <author>
        <name>Schönbächler, Maria</name>
      </author>
      <author>
        <name>Tafla, Lauren</name>
      </author>
      <author>
        <name>Tang, Haolan</name>
      </author>
      <author>
        <name>Terada, Kentaro</name>
      </author>
      <author>
        <name>Terada, Yasuko</name>
      </author>
      <author>
        <name>Usui, Tomohiro</name>
      </author>
      <author>
        <name>Wada, Sohei</name>
      </author>
      <author>
        <name>Wadhwa, Meenakshi</name>
      </author>
      <author>
        <name>Walker, Richard J</name>
      </author>
      <author>
        <name>Yamashita, Katsuyuki</name>
      </author>
      <author>
        <name>Yin, Qing-Zhu</name>
        <uri>https://orcid.org/0000-0002-4445-5096</uri>
      </author>
      <author>
        <name>Yoneda, Shigekazu</name>
      </author>
      <author>
        <name>Young, Edward D</name>
        <uri>https://orcid.org/0000-0002-1299-0801</uri>
      </author>
      <author>
        <name>Yui, Hiroharu</name>
      </author>
      <author>
        <name>Zhang, Ai-Cheng</name>
      </author>
      <author>
        <name>Nakamura, Tomoki</name>
      </author>
      <author>
        <name>Naraoka, Hiroshi</name>
      </author>
      <author>
        <name>Noguchi, Takaaki</name>
      </author>
      <author>
        <name>Okazaki, Ryuji</name>
      </author>
      <author>
        <name>Sakamoto, Kanako</name>
      </author>
      <author>
        <name>Yabuta, Hikaru</name>
      </author>
      <author>
        <name>Abe, Masanao</name>
      </author>
      <author>
        <name>Miyazaki, Akiko</name>
      </author>
      <author>
        <name>Nakato, Aiko</name>
      </author>
      <author>
        <name>Nishimura, Masahiro</name>
      </author>
      <author>
        <name>Okada, Tatsuaki</name>
      </author>
      <author>
        <name>Yada, Toru</name>
      </author>
      <author>
        <name>Yogata, Kasumi</name>
      </author>
      <author>
        <name>Nakazawa, Satoru</name>
      </author>
      <author>
        <name>Saiki, Takanao</name>
      </author>
      <author>
        <name>Tanaka, Satoshi</name>
      </author>
      <author>
        <name>Terui, Fuyuto</name>
      </author>
      <author>
        <name>Tsuda, Yuichi</name>
      </author>
      <author>
        <name>Watanabe, Sei-ichiro</name>
      </author>
      <author>
        <name>Yoshikawa, Makoto</name>
      </author>
      <author>
        <name>Tachibana, Shogo</name>
      </author>
      <author>
        <name>Yurimoto, Hisayoshi</name>
      </author>
    </item>
    <item>
      <title>Dual carbonate clumped isotopes (Δ47-Δ48) constrains kinetic effects and timescales in peridotite-associated springs at the Cedars, Northern California</title>
      <link>https://escholarship.org/uc/item/3899f70k</link>
      <description>The Cedars is an area in Northern California with a chain of highly alkaline springs resulting from CO2-charged meteorological water interacting with a peridotite body. Serpentinization resulting from this interaction at depth leads to the sequestration of various carbonate minerals into veins accompanied by a release of Ca2+ and OH– enriched water to the surface, creating an environment which promotes rapid precipitation of CaCO3 at surface springs. This environment enables us to apply the recently developed Δ47-Δ48 dual clumped isotope analysis to probe kinetic isotope effects (KIEs) and timescales of CO2 transformation in a region with the potential for geological CO2 sequestration. We analyzed CaCO3 recovered from various localities and identified significant kinetic fractionations associated with CO2 absorption in a majority of samples, characterized by enrichment in Δ47 values and depletion in Δ48 values relative to equilibrium. Surface floes exhibited the largest KIEs (ΔΔ47:...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3899f70k</guid>
      <pubDate>Tue, 29 Oct 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Parvez, Zeeshan A</name>
      </author>
      <author>
        <name>Lucarelli, Jamie K</name>
      </author>
      <author>
        <name>Matamoros, Irvin W</name>
      </author>
      <author>
        <name>Rubi, Joshua</name>
      </author>
      <author>
        <name>Miguel, Kevin</name>
      </author>
      <author>
        <name>Elliott, Ben</name>
      </author>
      <author>
        <name>Flores, Randy</name>
      </author>
      <author>
        <name>Ulrich, Robert N</name>
      </author>
      <author>
        <name>Eagle, Robert A</name>
      </author>
      <author>
        <name>Watkins, James M</name>
      </author>
      <author>
        <name>Christensen, John N</name>
      </author>
      <author>
        <name>Tripati, Aradhna</name>
        <uri>https://orcid.org/0000-0002-1695-1754</uri>
      </author>
    </item>
    <item>
      <title>Searching for a Solar Source of Magnetic-Field Switchbacks in Parker Solar Probe’s First Encounter</title>
      <link>https://escholarship.org/uc/item/5gv4775n</link>
      <description>Parker Solar Probe observations show ubiquitous magnetic-field reversals closer to the Sun, often referred to as “switchbacks”. The switchbacks have been observed before in the solar wind near 1&amp;nbsp;AU and beyond, but their occurrence was historically rare. PSP measurements below ∼ 0.2&amp;nbsp;AU show that switchbacks are, however, the most prominent structures in the “young” solar wind. In this work, we analyze remote-sensing observations of a small equatorial coronal hole to which PSP was connected during the perihelion of Encounter 1. We investigate whether some of the switchbacks captured during the encounter were of coronal origin by correlating common switchback in situ signatures with remote observations of their expected coronal footpoint. We find strong evidence that timescales present in the corona are relevant to the outflowing, switchback-filled solar wind, as illustrated by strong linear correlation. We also determine that spatial analysis of the observed region is...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5gv4775n</guid>
      <pubDate>Thu, 24 Oct 2024 00:00:00 +0000</pubDate>
      <author>
        <name>de Pablos, D</name>
      </author>
      <author>
        <name>Samanta, T</name>
      </author>
      <author>
        <name>Badman, ST</name>
      </author>
      <author>
        <name>Schwanitz, C</name>
      </author>
      <author>
        <name>Bahauddin, SM</name>
      </author>
      <author>
        <name>Harra, LK</name>
      </author>
      <author>
        <name>Petrie, G</name>
      </author>
      <author>
        <name>Mac Cormack, C</name>
      </author>
      <author>
        <name>Mandrini, CH</name>
      </author>
      <author>
        <name>Raouafi, NE</name>
      </author>
      <author>
        <name>Martinez Pillet, V</name>
      </author>
      <author>
        <name>Velli, M</name>
        <uri>https://orcid.org/0000-0002-2381-3106</uri>
      </author>
    </item>
    <item>
      <title>Low-cost table-top experiments for teaching multi-scale geophysical fluid dynamics</title>
      <link>https://escholarship.org/uc/item/89h1w8m1</link>
      <description>Multi-scale instabilities are ubiquitous in atmospheric and oceanic flows and are essential topics in teaching geophysical fluid dynamics. Yet these topics are often difficult to teach and counter-intuitive to new learners. In this paper, we introduce our state-of-the-art Do-It Yourself Dynamics (DIYnamics) LEGO® robotics kit that allows users to create table-top models of geophysical flows. Deep ocean convection processes are simulated via three experiments – upright convection, thermal wind flows, and baroclinic instability – in order to demonstrate the robust multi-scale modeling capabilities of our kit. Detailed recipes are provided to allow users to reproduce these experiments. Further, dye-visualization measurements show that the table-top experimental results adequately agree with theory. In sum, our DIYnamics setup provides students and educators with an accessible table-top framework by which to model the multi-scale behaviors, inherent in canonical geophysical flows,...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/89h1w8m1</guid>
      <pubDate>Wed, 23 Oct 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Moscoso, Jordyn E</name>
      </author>
      <author>
        <name>Tripoli, Rachel E</name>
      </author>
      <author>
        <name>Chen, Shizhe</name>
      </author>
      <author>
        <name>Church, William J</name>
      </author>
      <author>
        <name>Gonzalez, Henry</name>
      </author>
      <author>
        <name>Hill, Spencer A</name>
      </author>
      <author>
        <name>Khoo, Norris</name>
      </author>
      <author>
        <name>Lonner, Taylor L</name>
      </author>
      <author>
        <name>Aurnou, Jonathan M</name>
        <uri>https://orcid.org/0000-0002-8642-2962</uri>
      </author>
    </item>
    <item>
      <title>Magneto-Stokes flow in a shallow free-surface annulus</title>
      <link>https://escholarship.org/uc/item/1n654610</link>
      <description>In this study, we analyse ‘magneto-Stokes’ flow, a fundamental magnetohydrodynamic (MHD) flow that shares the cylindrical-annular geometry of the Taylor–Couette cell but uses applied electromagnetic forces to circulate a free-surface layer of electrolyte at low Reynolds numbers. The first complete, analytical solution for time-dependent magneto-Stokes flow is presented and validated with coupled laboratory and numerical experiments. Three regimes are distinguished (shallow-layer, transitional and deep-layer flow regimes), and their influence on the efficiency of microscale mixing is clarified. The solution in the shallow-layer limit belongs to a newly identified class of MHD potential flows, and thus induces mixing without the aid of axial vorticity. We show that these shallow-layer magneto-Stokes flows can still augment mixing in distinct Taylor dispersion and advection-dominated mixing regimes. The existence of enhanced mixing across all three distinguished flow regimes is predicted...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1n654610</guid>
      <pubDate>Wed, 23 Oct 2024 00:00:00 +0000</pubDate>
      <author>
        <name>David, Cy S</name>
      </author>
      <author>
        <name>Hester, Eric W</name>
      </author>
      <author>
        <name>Xu, Yufan</name>
      </author>
      <author>
        <name>Aurnou, Jonathan M</name>
        <uri>https://orcid.org/0000-0002-8642-2962</uri>
      </author>
    </item>
    <item>
      <title>Rotating convective turbulence in moderate to high Prandtl number fluids</title>
      <link>https://escholarship.org/uc/item/0d018999</link>
      <description>Rotating convective turbulence in moderate to high Prandtl number fluids</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0d018999</guid>
      <pubDate>Wed, 23 Oct 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Abbate, Jewel A</name>
      </author>
      <author>
        <name>Aurnou, Jonathan M</name>
        <uri>https://orcid.org/0000-0002-8642-2962</uri>
      </author>
    </item>
    <item>
      <title>The Faustini Permanently Shadowed Region on the Moon</title>
      <link>https://escholarship.org/uc/item/6mz6r9b0</link>
      <description>Abstract: 

               Faustini crater (41 km diameter) hosts a large (664 km2) permanently shadowed region (PSR) with a high potential to harbor water-ice deposits. One of the 13 candidate Artemis III landing areas contains a portion of the crater rim and proximal ejecta. The ShadowCam instrument aboard the Korea Pathfinder Lunar Orbiter provides detailed images of the PSR within Faustini. We characterize the terrain and thermal environment within the Faustini PSR from ShadowCam images, Lunar Reconnaissance Orbiter thermal measurements and laser ranging, and thermal modeling. Our mapping revealed three distinct areas of the floor of Faustini based on elevations, slopes, and surface roughness. These units broadly correlate with temperatures; thus, they may be influenced by variations in volatile sublimation. Crater retention and topographic diffusion rates appear to be asymmetric across the floor, likely due to differences in maximum and average temperatures. Several irregular...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6mz6r9b0</guid>
      <pubDate>Wed, 9 Oct 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Williams, Jean-Pierre</name>
        <uri>https://orcid.org/0000-0003-4163-2760</uri>
      </author>
      <author>
        <name>Mahanti, Prasun</name>
      </author>
      <author>
        <name>Robinson, Mark S</name>
      </author>
      <author>
        <name>Wagner, Robert V</name>
      </author>
      <author>
        <name>Chertok, Marley</name>
      </author>
      <author>
        <name>Schörghofer, Norbert</name>
      </author>
      <author>
        <name>Mazarico, Erwan</name>
      </author>
      <author>
        <name>Denevi, Brett W</name>
      </author>
      <author>
        <name>Li, Shuai</name>
      </author>
      <author>
        <name>Paige, David A</name>
      </author>
    </item>
    <item>
      <title>Shadowgraph Measurements of Rotating Convective Planetary Core‐Style Flows</title>
      <link>https://escholarship.org/uc/item/7r79c5v2</link>
      <description>Abstract: 
The local scale of rotating convection, ℓ, is a fundamental parameter in many turbulent geophysical and astrophysical fluid systems, yet it is often poorly constrained. Here we conduct rotating convection laboratory experiments analogous to convecting flows in planetary cores and subsurface oceans to obtain measurements of the local scales of motion. Utilizing silicone oil as the working fluid, we employ shadowgraph imagery to visualize the flow, from which we extract values of the characteristic cross‐axial scale of convective columns and plumes. These measurements are compared to the theoretical values of the critical onset length scale, ℓcrit, and the turbulent length scale, ℓturb. Our experimentally obtained length scale measurements simultaneously agree with both the onset and turbulent scale predictions across three orders of magnitude in convective supercriticality , a correlation that is consistent with inferences made in prior studies. We further explore the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7r79c5v2</guid>
      <pubDate>Wed, 25 Sep 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Abbate, Jewel A</name>
      </author>
      <author>
        <name>Aurnou, Jonathan M</name>
        <uri>https://orcid.org/0000-0002-8642-2962</uri>
      </author>
    </item>
    <item>
      <title>Electrical Conductivity of Subsurface Ocean Analogue Solutions from Molecular Dynamics Simulations</title>
      <link>https://escholarship.org/uc/item/7dc8h5qg</link>
      <description>Investigating the habitability of ocean worlds is a priority of current and future NASA missions. The &lt;i&gt;Europa Clipper&lt;/i&gt; mission will conduct approximately 50 flybys of Jupiter's moon Europa, returning a detailed portrait of its interior from the synthesis of data from its instrument suite. The magnetometer on board has the capability of decoupling Europa's induced magnetic field to high precision, and when these data are inverted, the electrical conductivity profile from the electrically conducting subsurface salty ocean may be constrained. To optimize the interpretation of magnetic induction data near ocean worlds and constrain salinity from electrical conductivity, accurate laboratory electrical conductivity data are needed under the conditions expected in their subsurface oceans. At the high-pressure, low-temperature (HPLT) conditions of icy worlds, comprehensive conductivity data sets are sparse or absent from either laboratory data or simulations. We conducted molecular...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7dc8h5qg</guid>
      <pubDate>Mon, 1 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Psarakis, Catherine A</name>
      </author>
      <author>
        <name>Fidelis, Timothy Tizhe</name>
      </author>
      <author>
        <name>Chin, Keith B</name>
      </author>
      <author>
        <name>Journaux, Baptiste</name>
      </author>
      <author>
        <name>Kavner, Abby</name>
        <uri>https://orcid.org/0000-0002-3895-2459</uri>
      </author>
      <author>
        <name>Sarker, Pranab</name>
      </author>
      <author>
        <name>Styczinski, Marshall J</name>
      </author>
      <author>
        <name>Vance, Steven D</name>
      </author>
      <author>
        <name>Wei, Tao</name>
      </author>
    </item>
    <item>
      <title>Dual carbonate clumped isotope (Δ47-Δ48) measurements constrain different sources of kinetic isotope effects and quasi-equilibrium signatures in cave carbonates</title>
      <link>https://escholarship.org/uc/item/7ff179d1</link>
      <description>Cave carbonate minerals are an important terrestrial paleoclimate archive. A few studies have explored the potential for applying carbonate clumped isotope thermometry to speleothems as a tool for constraining past temperatures. To date, most papers utilizing this method have focused on mass-47 clumped isotope values (Δ47) at a single location and reported that cave carbonate minerals rarely achieve isotopic equilibrium, with kinetic isotope effects (KIEs) attributed to CO2 degassing. More recently, studies have shown that mass-47 and mass-48 CO2 from acid digested carbonate minerals (Δ47 and Δ48) can be used together to assess equilibrium and probe KIEs. Here, we examined 44 natural and synthetic modern cave carbonate mineral samples from 13 localities with varying environmental conditions (ventilation, water level, pCO2, temperature) for (dis)equilibrium using Δ47-Δ48 values, in concert with traditional stable carbon (δ13C) and oxygen (δ18O) isotope ratios. Data showed that...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7ff179d1</guid>
      <pubDate>Wed, 17 Apr 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Parvez, Zeeshan A</name>
      </author>
      <author>
        <name>El-Shenawy, Mohammed I</name>
      </author>
      <author>
        <name>Lucarelli, Jamie K</name>
      </author>
      <author>
        <name>Kim, Sang-Tae</name>
      </author>
      <author>
        <name>Johnson, Kathleen R</name>
      </author>
      <author>
        <name>Wright, Kevin</name>
      </author>
      <author>
        <name>Gebregiorgis, Daniel</name>
      </author>
      <author>
        <name>Montanez, Isabel P</name>
        <uri>https://orcid.org/0000-0003-0492-3796</uri>
      </author>
      <author>
        <name>Wortham, Barbara</name>
      </author>
      <author>
        <name>Asrat, Asfawossen</name>
      </author>
      <author>
        <name>Reinhardt, Eduard</name>
      </author>
      <author>
        <name>Christensen, John N</name>
      </author>
      <author>
        <name>Matamoros, Irvin W</name>
      </author>
      <author>
        <name>Rubi, Joshua</name>
      </author>
      <author>
        <name>Miguel, Kevin</name>
      </author>
      <author>
        <name>Elliott, Ben M</name>
      </author>
      <author>
        <name>Flores, Randy</name>
      </author>
      <author>
        <name>Kovacs, Shawn</name>
      </author>
      <author>
        <name>Eagle, Robert A</name>
      </author>
      <author>
        <name>Tripati, Aradhna</name>
        <uri>https://orcid.org/0000-0002-1695-1754</uri>
      </author>
    </item>
    <item>
      <title>Analytic Model and Magnetohydrodynamic Simulations of Three-dimensional Magnetic Switchbacks</title>
      <link>https://escholarship.org/uc/item/7c50m4r8</link>
      <description>Abstract: 

               Parker Solar Probe observations reveal that the near-Sun space is almost filled with magnetic switchbacks (“switchbacks” hereinafter), which may be a major contributor to the heating and acceleration of solar wind. Here, for the first time, we develop an analytic model of an axisymmetric switchback with uniform magnetic field strength. In this model, three parameters control the geometry of the switchback: height (length along the background magnetic field), width (thickness along radial direction perpendicular to the background field), and the radial distance from the center of switchback to the central axis, which is a proxy of the size of the switchback along the third dimension. We carry out 3D magnetohydrodynamic simulations to investigate the dynamic evolution of the switchback. Comparing simulations conducted with compressible and incompressible codes, we verify that compressibility, i.e., parametric decay instability, is necessary for destabilizing...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7c50m4r8</guid>
      <pubDate>Wed, 10 Apr 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Shi, Chen</name>
        <uri>https://orcid.org/0000-0002-2582-7085</uri>
      </author>
      <author>
        <name>Velli, Marco</name>
      </author>
      <author>
        <name>Toth, Gabor</name>
      </author>
      <author>
        <name>Zhang, Kun</name>
      </author>
      <author>
        <name>Tenerani, Anna</name>
      </author>
      <author>
        <name>Huang, Zesen</name>
      </author>
      <author>
        <name>Sioulas, Nikos</name>
      </author>
      <author>
        <name>van der Holst, Bart</name>
      </author>
    </item>
    <item>
      <title>Stormtime substorm onsets: occurrence and flow channel triggering</title>
      <link>https://escholarship.org/uc/item/1wk1522m</link>
      <description>Bright auroral emissions during geomagnetic storms provide a good opportunity for testing the proposal that substorm onset is frequently triggered by plasma sheet flow bursts that are manifested in the ionosphere as auroral streamers. We have used the broad coverage of the ionospheric mapping of the plasma sheet offered by the high-resolution THEMIS all-sky-imagers (ASIs) and chose the main phases of 9 coronal mass ejection (CME) related and 9 high-speed stream (HSS)-related geomagnetic storms, and identified substorm auroral onsets defined as brightening followed by poleward expansion. We found a detectable streamer heading to near the substorm onset location for all 60 onsets that we identified and were observed well by the ASIs. This indicates that substorm onsets are very often triggered by the intrusion of plasma with lower entropy than the surrounding plasma to the onset region, with the caveat that the ASIs do not give a direct measure of the intruding plasma. The majority...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1wk1522m</guid>
      <pubDate>Fri, 29 Mar 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Lyons, Larry R</name>
      </author>
      <author>
        <name>Zou, Ying</name>
      </author>
      <author>
        <name>Nishimura, Yukitoshi</name>
      </author>
      <author>
        <name>Gallardo-Lacourt, Bea</name>
      </author>
      <author>
        <name>Angelopulos, Vassilis</name>
      </author>
      <author>
        <name>Donovan, Eric F</name>
      </author>
    </item>
    <item>
      <title>Partitioning of Iron Between Liquid and Crystalline Phases of (Mg,Fe)O</title>
      <link>https://escholarship.org/uc/item/80h1w03w</link>
      <description>Abstract: 
The density contrast between crystals and coexisting liquids is key to understanding the evolution of the magma ocean. While crystals remain denser than isochemical liquids in most oxide and silicate systems over the pressure range of Earth's mantle, element partitioning, particularly of abundant heavy elements such as iron, can alter the buoyancy. We use molecular dynamics simulations based on spin‐polarized density functional theory and adiabatic switching to determine the free energy of iron substitution in liquid and crystalline (Mg,Fe)O and the distribution coefficient. We find that iron is strongly incompatible with a distribution coefficient less than 0.3 over the mantle pressure range. We find that the crystal is buoyant with respect to coexisting liquid at pressures exceeding 50&amp;nbsp;GPa. The high‐spin to low‐spin transition has an important influence on the distribution coefficient, which decreases with increasing pressure up to 80&amp;nbsp;GPa, and then increases...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/80h1w03w</guid>
      <pubDate>Wed, 20 Mar 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Braithwaite, James</name>
      </author>
      <author>
        <name>Stixrude, Lars</name>
      </author>
    </item>
    <item>
      <title>Thermal and Tidal Evolution of Uranus with a Growing Frozen Core</title>
      <link>https://escholarship.org/uc/item/5d00b91x</link>
      <description>Abstract: 

               The origin of the very low luminosity of Uranus is unknown, as is the source of the internal tidal dissipation required by the orbits of the Uranian moons. Models of the interior of Uranus often assume that it is inviscid throughout, but recent experiments show that this assumption may not be justified; most of the interior of Uranus lies below the freezing temperature of H2O. We find that the stable solid phase of H2O, which is superionic, has a large viscosity controlled by the crystalline oxygen sublattice. We examine the consequences of finite viscosity by combining ab initio determinations of the thermal conductivity and other material properties of superionic H2O with a thermal evolution model that accounts for heat trapped in the growing frozen core. The high viscosity provides a means of trapping heat in the deep interior while also providing a source of tidal dissipation. The frozen core grows with time because its outer boundary is governed...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5d00b91x</guid>
      <pubDate>Wed, 20 Mar 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Stixrude, Lars</name>
      </author>
      <author>
        <name>Baroni, Stefano</name>
      </author>
      <author>
        <name>Grasselli, Federico</name>
      </author>
    </item>
    <item>
      <title>Thermal and Tidal Evolution of Ice Giants with Growing Frozen Cores: The Case of Neptune</title>
      <link>https://escholarship.org/uc/item/5905w6k7</link>
      <description>Abstract: 
The contrasting internal luminosity of Uranus and Neptune present a challenge to our understanding of the origin and evolution of these bodies, as well as extra-solar ice giants. The thermal evolution of Neptune is known to be nearly consistent with an entirely fluid interior, but this is not a unique solution, and does not account for the tidal dissipation required by the migration of its moons. We examine a model that has been previously shown to explain the thermal and tidal evolution of Uranus: one that features a growing, frozen core. The core traps heat in the interior, affecting the cooling time scale, and provides a source of tidal dissipation. We review the growing, frozen core model, and the computation of thermal and tidal evolution. We then apply this model to Neptune. We find that the growing frozen core model can account for the observed internal luminosity of Neptune and the migration of its moons, in the form of resonances that were either encountered...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5905w6k7</guid>
      <pubDate>Wed, 20 Mar 2024 00:00:00 +0000</pubDate>
      <author>
        <name>James, David A</name>
      </author>
      <author>
        <name>Stixrude, Lars</name>
      </author>
    </item>
    <item>
      <title>Centering Equity in the Nation's Weather, Water, and Climate Services</title>
      <link>https://escholarship.org/uc/item/5g7450vx</link>
      <description>Water, weather, and climate affect everyone. However, their impacts on various communities can be very different based on who has access to essential services and environmental knowledge. Structural discrimination, including racism and other forms of privileging and exclusion, affects people's lives and health, with ripples across all sectors of society. In the United States, the need to equitably provide weather, water, and climate services is uplifted by the Justice40 Initiative (Executive Order 14008), which mandates 40% of the benefits of certain federal climate and clean energy investments flow to disadvantaged communities. To effectively provide such services while centering equity, systemic reform is required. Reform is imperative given increasing weather-related disasters, public health impacts of climate change, and disparities in infrastructure, vulnerabilities, and outcomes. It is imperative that those with positional authority and resources manifest responsibility...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5g7450vx</guid>
      <pubDate>Fri, 1 Mar 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Tripati, Aradhna</name>
        <uri>https://orcid.org/0000-0002-1695-1754</uri>
      </author>
      <author>
        <name>Shepherd, Marshall</name>
      </author>
      <author>
        <name>Morris, Vernon</name>
      </author>
      <author>
        <name>Andrade, Karen</name>
      </author>
      <author>
        <name>Whyte, Kyle Powys</name>
      </author>
      <author>
        <name>David-Chavez, Dominique M</name>
      </author>
      <author>
        <name>Hosbey, Justin</name>
      </author>
      <author>
        <name>Trujillo-Falcón, Joseph E</name>
      </author>
      <author>
        <name>Hunter, Brandon</name>
      </author>
      <author>
        <name>Hence, Deanna</name>
      </author>
      <author>
        <name>Carlis, DaNa</name>
      </author>
      <author>
        <name>Brown, Vankita</name>
      </author>
      <author>
        <name>Parker, William L</name>
      </author>
      <author>
        <name>Geller, Andrew</name>
      </author>
      <author>
        <name>Reich, Alex</name>
      </author>
      <author>
        <name>Glackin, Mary</name>
      </author>
    </item>
    <item>
      <title>Global validation of data-assimilative electron ring current nowcast for space weather applications</title>
      <link>https://escholarship.org/uc/item/4tb3h7tv</link>
      <description>The hazardous plasma environment surrounding Earth poses risks to satellites due to internal charging and surface charging effects. Accurate predictions of these risks are crucial for minimizing damage and preparing for system failures of satellites. To forecast the plasma environment, it is essential to know the current state of the system, as the accuracy of the forecast depends on the accuracy of the initial condition of the forecast. In this study, we use data assimilation techniques to combine observational data and model predictions, and present the first global validation of a data-assimilative electron ring current nowcast during a geomagnetic storm. By assimilating measurements from one satellite and validating the results against another satellite in a different magnetic local time sector, we assess the global response and effectiveness of the data assimilation technique for space weather applications. Using this method, we found that the simulation accuracy can be drastically...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4tb3h7tv</guid>
      <pubDate>Thu, 15 Feb 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Haas, Bernhard</name>
      </author>
      <author>
        <name>Shprits, Yuri Y</name>
        <uri>https://orcid.org/0000-0002-9625-0834</uri>
      </author>
      <author>
        <name>Wutzig, Michael</name>
      </author>
      <author>
        <name>Szabó-Roberts, Mátyás</name>
      </author>
      <author>
        <name>García Peñaranda, Marina</name>
      </author>
      <author>
        <name>Castillo Tibocha, Angelica M</name>
      </author>
      <author>
        <name>Himmelsbach, Julia</name>
      </author>
      <author>
        <name>Wang, Dedong</name>
      </author>
      <author>
        <name>Miyoshi, Yoshizumi</name>
      </author>
      <author>
        <name>Kasahara, Satoshi</name>
      </author>
      <author>
        <name>Keika, Kunihiro</name>
      </author>
      <author>
        <name>Yokota, Shoichiro</name>
      </author>
      <author>
        <name>Shinohara, Iku</name>
      </author>
      <author>
        <name>Hori, Tomo</name>
      </author>
    </item>
    <item>
      <title>Water circulation in Ryugu asteroid affected the distribution of nucleosynthetic isotope anomalies in returned sample</title>
      <link>https://escholarship.org/uc/item/8vj5k7bb</link>
      <description>Studies of material returned from Cb asteroid Ryugu have revealed considerable mineralogical and chemical heterogeneity, stemming primarily from brecciation and aqueous alteration. Isotopic anomalies could have also been affected by delivery of exogenous clasts and aqueous mobilization of soluble elements. Here, we show that isotopic anomalies for mildly soluble Cr are highly variable in Ryugu and CI chondrites, whereas those of Ti are relatively uniform. This variation in Cr isotope ratios is most likely due to physicochemical fractionation between &lt;sup&gt;54&lt;/sup&gt;Cr-rich presolar nanoparticles and Cr-bearing secondary minerals at the millimeter-scale in the bulk samples, likely due to extensive aqueous alteration in their parent bodies that occurred [Formula: see text] after Solar System birth. In contrast, Ti isotopes were marginally affected by this process. Our results show that isotopic heterogeneities in asteroids are not all nebular or accretionary in nature but can also...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8vj5k7bb</guid>
      <pubDate>Sat, 25 Nov 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Yokoyama, Tetsuya</name>
      </author>
      <author>
        <name>Wadhwa, Meenakshi</name>
      </author>
      <author>
        <name>Iizuka, Tsuyoshi</name>
      </author>
      <author>
        <name>Rai, Vinai</name>
      </author>
      <author>
        <name>Gautam, Ikshu</name>
      </author>
      <author>
        <name>Hibiya, Yuki</name>
      </author>
      <author>
        <name>Masuda, Yuki</name>
      </author>
      <author>
        <name>Haba, Makiko K</name>
      </author>
      <author>
        <name>Fukai, Ryota</name>
      </author>
      <author>
        <name>Hines, Rebekah</name>
      </author>
      <author>
        <name>Phelan, Nicole</name>
      </author>
      <author>
        <name>Abe, Yoshinari</name>
      </author>
      <author>
        <name>Aléon, Jérôme</name>
      </author>
      <author>
        <name>Alexander, Conel M O’D</name>
      </author>
      <author>
        <name>Amari, Sachiko</name>
      </author>
      <author>
        <name>Amelin, Yuri</name>
      </author>
      <author>
        <name>Bajo, Ken-ichi</name>
      </author>
      <author>
        <name>Bizzarro, Martin</name>
      </author>
      <author>
        <name>Bouvier, Audrey</name>
      </author>
      <author>
        <name>Carlson, Richard W</name>
      </author>
      <author>
        <name>Chaussidon, Marc</name>
      </author>
      <author>
        <name>Choi, Byeon-Gak</name>
      </author>
      <author>
        <name>Dauphas, Nicolas</name>
      </author>
      <author>
        <name>Davis, Andrew M</name>
      </author>
      <author>
        <name>Di Rocco, Tommaso</name>
      </author>
      <author>
        <name>Fujiya, Wataru</name>
      </author>
      <author>
        <name>Hidaka, Hiroshi</name>
      </author>
      <author>
        <name>Homma, Hisashi</name>
      </author>
      <author>
        <name>Hoppe, Peter</name>
      </author>
      <author>
        <name>Huss, Gary R</name>
      </author>
      <author>
        <name>Ichida, Kiyohiro</name>
      </author>
      <author>
        <name>Ireland, Trevor</name>
      </author>
      <author>
        <name>Ishikawa, Akira</name>
      </author>
      <author>
        <name>Itoh, Shoichi</name>
      </author>
      <author>
        <name>Kawasaki, Noriyuki</name>
      </author>
      <author>
        <name>Kita, Noriko T</name>
      </author>
      <author>
        <name>Kitajima, Koki</name>
      </author>
      <author>
        <name>Kleine, Thorsten</name>
      </author>
      <author>
        <name>Komatani, Shintaro</name>
      </author>
      <author>
        <name>Krot, Alexander N</name>
      </author>
      <author>
        <name>Liu, Ming-Chang</name>
      </author>
      <author>
        <name>McKeegan, Kevin D</name>
      </author>
      <author>
        <name>Morita, Mayu</name>
      </author>
      <author>
        <name>Motomura, Kazuko</name>
      </author>
      <author>
        <name>Moynier, Frédéric</name>
      </author>
      <author>
        <name>Nakai, Izumi</name>
      </author>
      <author>
        <name>Nagashima, Kazuhide</name>
      </author>
      <author>
        <name>Nguyen, Ann</name>
      </author>
      <author>
        <name>Nittler, Larry</name>
      </author>
      <author>
        <name>Onose, Morihiko</name>
      </author>
      <author>
        <name>Pack, Andreas</name>
      </author>
      <author>
        <name>Park, Changkun</name>
      </author>
      <author>
        <name>Piani, Laurette</name>
      </author>
      <author>
        <name>Qin, Liping</name>
      </author>
      <author>
        <name>Russell, Sara</name>
      </author>
      <author>
        <name>Sakamoto, Naoya</name>
      </author>
      <author>
        <name>Schönbächler, Maria</name>
      </author>
      <author>
        <name>Tafla, Lauren</name>
      </author>
      <author>
        <name>Tang, Haolan</name>
      </author>
      <author>
        <name>Terada, Kentaro</name>
      </author>
      <author>
        <name>Terada, Yasuko</name>
      </author>
      <author>
        <name>Usui, Tomohiro</name>
      </author>
      <author>
        <name>Wada, Sohei</name>
      </author>
      <author>
        <name>Walker, Richard J</name>
      </author>
      <author>
        <name>Yamashita, Katsuyuki</name>
      </author>
      <author>
        <name>Yin, Qing-Zhu</name>
        <uri>https://orcid.org/0000-0002-4445-5096</uri>
      </author>
      <author>
        <name>Yoneda, Shigekazu</name>
      </author>
      <author>
        <name>Young, Edward D</name>
        <uri>https://orcid.org/0000-0002-1299-0801</uri>
      </author>
      <author>
        <name>Yui, Hiroharu</name>
      </author>
      <author>
        <name>Zhang, Ai-Cheng</name>
      </author>
      <author>
        <name>Nakamura, Tomoki</name>
      </author>
      <author>
        <name>Naraoka, Hiroshi</name>
      </author>
      <author>
        <name>Noguchi, Takaaki</name>
      </author>
      <author>
        <name>Okazaki, Ryuji</name>
      </author>
      <author>
        <name>Sakamoto, Kanako</name>
      </author>
      <author>
        <name>Yabuta, Hikaru</name>
      </author>
      <author>
        <name>Abe, Masanao</name>
      </author>
      <author>
        <name>Miyazaki, Akiko</name>
      </author>
      <author>
        <name>Nakato, Aiko</name>
      </author>
      <author>
        <name>Nishimura, Masahiro</name>
      </author>
      <author>
        <name>Okada, Tatsuaki</name>
      </author>
      <author>
        <name>Yada, Toru</name>
      </author>
      <author>
        <name>Yogata, Kasumi</name>
      </author>
      <author>
        <name>Nakazawa, Satoru</name>
      </author>
      <author>
        <name>Saiki, Takanao</name>
      </author>
      <author>
        <name>Tanaka, Satoshi</name>
      </author>
      <author>
        <name>Terui, Fuyuto</name>
      </author>
      <author>
        <name>Tsuda, Yuichi</name>
      </author>
      <author>
        <name>Watanabe, Sei-ichiro</name>
      </author>
      <author>
        <name>Yoshikawa, Makoto</name>
      </author>
      <author>
        <name>Tachibana, Shogo</name>
      </author>
      <author>
        <name>Yurimoto, Hisayoshi</name>
      </author>
    </item>
    <item>
      <title>A Search for Technosignatures Around 11,680 Stars with the Green Bank Telescope at 1.15–1.73 GHz</title>
      <link>https://escholarship.org/uc/item/8ds6g05v</link>
      <description>Abstract: 

               We conducted a search for narrowband radio signals over four observing sessions in 2020–2023 with the L-band receiver (1.15–1.73 GHz) of the 100 m diameter Green Bank Telescope. We pointed the telescope in the directions of 62 TESS Objects of Interest, capturing radio emissions from a total of ∼11,680 stars and planetary systems in the ∼9′ beam of the telescope. All detections were either automatically rejected or visually inspected and confirmed to be of anthropogenic nature. We also quantified the end-to-end efficiency of radio SETI pipelines with a signal injection and recovery analysis. The UCLA SETI pipeline recovers 94.0% of the injected signals over the usable frequency range of the receiver and 98.7% of the injections when regions of dense radio frequency interference are excluded. In another pipeline that uses incoherent sums of 51 consecutive spectra, the recovery rate is ∼15 times smaller at ∼6%. The pipeline efficiency affects calculations...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8ds6g05v</guid>
      <pubDate>Wed, 25 Oct 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Margot, Jean-Luc</name>
        <uri>https://orcid.org/0000-0001-9798-1797</uri>
      </author>
      <author>
        <name>Li, Megan G</name>
        <uri>https://orcid.org/0000-0002-3012-4261</uri>
      </author>
      <author>
        <name>Pinchuk, Pavlo</name>
        <uri>https://orcid.org/0000-0003-4736-4728</uri>
      </author>
      <author>
        <name>Myhrvold, Nathan</name>
        <uri>https://orcid.org/0000-0003-3994-5143</uri>
      </author>
      <author>
        <name>Lesyna, Larry</name>
        <uri>https://orcid.org/0000-0003-3970-688X</uri>
      </author>
      <author>
        <name>Alcantara, Lea E</name>
      </author>
      <author>
        <name>Andrakin, Megan T</name>
      </author>
      <author>
        <name>Arunseangroj, Jeth</name>
      </author>
      <author>
        <name>Baclet, Damien S</name>
      </author>
      <author>
        <name>Belk, Madison H</name>
      </author>
      <author>
        <name>Bhadha, Zerxes R</name>
      </author>
      <author>
        <name>Brandis, Nicholas W</name>
      </author>
      <author>
        <name>Carey, Robert E</name>
      </author>
      <author>
        <name>Cassar, Harrison P</name>
      </author>
      <author>
        <name>Chava, Sai S</name>
      </author>
      <author>
        <name>Chen, Calvin</name>
      </author>
      <author>
        <name>Chen, James</name>
      </author>
      <author>
        <name>Cheng, Kellen T</name>
      </author>
      <author>
        <name>Cimbri, Alessia</name>
      </author>
      <author>
        <name>Cloutier, Benjamin</name>
      </author>
      <author>
        <name>Combitsis, Jordan A</name>
      </author>
      <author>
        <name>Couvrette, Kelly L</name>
      </author>
      <author>
        <name>Coy, Brandon P</name>
      </author>
      <author>
        <name>Davis, Kyle W</name>
      </author>
      <author>
        <name>Delcayre, Antoine F</name>
      </author>
      <author>
        <name>Du, Michelle R</name>
      </author>
      <author>
        <name>Feil, Sarah E</name>
      </author>
      <author>
        <name>Fu, Danning</name>
      </author>
      <author>
        <name>Gilmore, Travis J</name>
      </author>
      <author>
        <name>Grahill-Bland, Emery</name>
      </author>
      <author>
        <name>Iglesias, Laura M</name>
      </author>
      <author>
        <name>Juneau, Zoe</name>
      </author>
      <author>
        <name>Karapetian, Anthony G</name>
      </author>
      <author>
        <name>Karfakis, George</name>
      </author>
      <author>
        <name>Lambert, Christopher T</name>
      </author>
      <author>
        <name>Lazbin, Eric A</name>
      </author>
      <author>
        <name>Li, Jian H</name>
      </author>
      <author>
        <name>Li, Zhuofu Chester</name>
      </author>
      <author>
        <name>Liskij, Nicholas M</name>
      </author>
      <author>
        <name>Lopilato, Anthony V</name>
      </author>
      <author>
        <name>Lu, Darren J</name>
      </author>
      <author>
        <name>Ma, Detao</name>
      </author>
      <author>
        <name>Mathur, Vedant</name>
      </author>
      <author>
        <name>Minasyan, Mary H</name>
      </author>
      <author>
        <name>Muller, Maxwell K</name>
      </author>
      <author>
        <name>Nasielski, Mark T</name>
      </author>
      <author>
        <name>Nguyen, Janice T</name>
      </author>
      <author>
        <name>Nicholson, Lorraine M</name>
      </author>
      <author>
        <name>Niemoeller, Samantha</name>
      </author>
      <author>
        <name>Ohri, Divij</name>
      </author>
      <author>
        <name>Padhye, Atharva U</name>
      </author>
      <author>
        <name>Penmetcha, Supreethi V</name>
      </author>
      <author>
        <name>Prakash, Yugantar</name>
      </author>
      <author>
        <name>Qi, Xinyi Cindy</name>
      </author>
      <author>
        <name>Rindt, Liam</name>
      </author>
      <author>
        <name>Sahu, Vedant</name>
      </author>
      <author>
        <name>Scally, Joshua A</name>
      </author>
      <author>
        <name>Scott, Zefyr</name>
      </author>
      <author>
        <name>Seddon, Trevor J</name>
      </author>
      <author>
        <name>Shohet, Lara-Lynn V</name>
      </author>
      <author>
        <name>Sinha, Anchal</name>
      </author>
      <author>
        <name>Sinigiani, Anthony E</name>
      </author>
      <author>
        <name>Song, Jiuxu</name>
      </author>
      <author>
        <name>Stice, Spencer M</name>
      </author>
      <author>
        <name>Tabucol, Nadine M</name>
      </author>
      <author>
        <name>Uplisashvili, Andria</name>
      </author>
      <author>
        <name>Vanga, Krishna</name>
      </author>
      <author>
        <name>Vazquez, Amaury G</name>
      </author>
      <author>
        <name>Vetushko, George</name>
      </author>
      <author>
        <name>Villa, Valeria</name>
      </author>
      <author>
        <name>Vincent, Maria</name>
      </author>
      <author>
        <name>Waasdorp, Ian J</name>
      </author>
      <author>
        <name>Wagaman, Ian B</name>
      </author>
      <author>
        <name>Wang, Amanda</name>
      </author>
      <author>
        <name>Wight, Jade C</name>
      </author>
      <author>
        <name>Wong, Ella</name>
      </author>
      <author>
        <name>Yamaguchi, Natsuko</name>
      </author>
      <author>
        <name>Zhang, Zijin</name>
      </author>
      <author>
        <name>Zhao, Junyang</name>
      </author>
      <author>
        <name>Lynch, Ryan S</name>
        <uri>https://orcid.org/0000-0001-5229-7430</uri>
      </author>
    </item>
    <item>
      <title>Thermal Models of Asteroids with Two-band Combinations of Wide-field Infrared Survey Explorer Cryogenic Data</title>
      <link>https://escholarship.org/uc/item/6fb775zb</link>
      <description>Abstract: 

               We used the reparameterized Near-Earth Asteroid Thermal Model to model observations of a curated set of over 4000 asteroids from the Wide-field Infrared Survey Explorer in two wavelength bands (W2–3 or W3–4) and compared the results to previous results from all four wavelength bands (W1–4). This comparison was done with the goal of elucidating unique aspects of modeling two-band observations so that any potential biases or shortcomings for planned two-band surveys (e.g., the NASA Near-Earth Object Surveyor Mission) can be anticipated and quantified. The W2–3 two-band fits usually yielded slightly smaller diameters than the four-band fits, with a median diameter difference of −10%, with the 5% and 95% quantiles of the distribution at −32% and −1.5%, respectively.&amp;nbsp;We conducted similar comparisons for W3–4, in part because the longest wavelength bands are expected to provide the best two-band results. We found that the W3–4 two-band diameters are slightly...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6fb775zb</guid>
      <pubDate>Wed, 25 Oct 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Whittaker, Emily A</name>
        <uri>https://orcid.org/0000-0002-1518-7475</uri>
      </author>
      <author>
        <name>Margot, Jean-Luc</name>
        <uri>https://orcid.org/0000-0001-9798-1797</uri>
      </author>
      <author>
        <name>Lam, Adrian LH</name>
      </author>
      <author>
        <name>Myhrvold, Nathan</name>
      </author>
    </item>
    <item>
      <title>Equilibrated Gas and Carbonate Standard‐Derived Dual (Δ47 and Δ48) Clumped Isotope Values</title>
      <link>https://escholarship.org/uc/item/27x5g03z</link>
      <description>Carbonate clumped isotope geochemistry has primarily focused on mass spectrometric determination of &lt;i&gt;m/z&lt;/i&gt; 47 CO&lt;sub&gt;2&lt;/sub&gt; for geothermometry, but theoretical calculations and recent experiments indicate paired analysis of the &lt;i&gt;m/z&lt;/i&gt; 47 (&lt;sup&gt;13&lt;/sup&gt;C&lt;sup&gt;18&lt;/sup&gt;O&lt;sup&gt;16&lt;/sup&gt;O) and &lt;i&gt;m/z&lt;/i&gt; 48 (&lt;sup&gt;12&lt;/sup&gt;C&lt;sup&gt;18&lt;/sup&gt;O&lt;sup&gt;18&lt;/sup&gt;O) isotopologues (referred to as  and ) can be used to study non-equilibrium isotope fractionations and refine temperature estimates. We utilize 5,448  and 3,400  replicate measurements of carbonate samples and standards, and 183  and 195  replicate measurements of gas standards from 2015 to 2021 from a multi-year and multi-instrument data set to constrain  and  values for 27 samples and standards, including Devils Hole cave calcite, and study equilibrium -, -temperature, and -temperature relationships. We compare results to previously published findings and calculate equilibrium regressions based on data from multiple laboratories....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/27x5g03z</guid>
      <pubDate>Wed, 18 Oct 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Lucarelli, Jamie K</name>
      </author>
      <author>
        <name>Carroll, Hannah M</name>
      </author>
      <author>
        <name>Ulrich, Robert N</name>
      </author>
      <author>
        <name>Elliott, Ben M</name>
      </author>
      <author>
        <name>Coplen, Tyler B</name>
      </author>
      <author>
        <name>Eagle, Robert A</name>
      </author>
      <author>
        <name>Tripati, Aradhna</name>
        <uri>https://orcid.org/0000-0002-1695-1754</uri>
      </author>
    </item>
    <item>
      <title>Cryptofaunal diversity in fringing reef rhodoliths</title>
      <link>https://escholarship.org/uc/item/520407t8</link>
      <description>Abstract: 
Rhodolith distribution, morphology, and cryptofauna have been minimally studied on fringing reefs. We present the first study to examine both rhodolith distribution and associated cryptofauna in a tropical fringing reef, located along the microtidal, wave-dominated north shore of Moorea, French Polynesia. We find higher abundances of larger, rounder, and more branching rhodoliths in locations where longer waves impact the fringing reef. Among 1879 animals extracted and identified from 145 rhodoliths, ophiuroids, polychaetes, decapod crustaceans, and gastropods are most abundant, with a wide range of additional taxa contributing to diversity. Large and branching rhodoliths contain the greatest number and diversity of cryptofaunal organisms and are the preferred habitat of rigid-bodied, non-burrowing forms. Overall, exposure to waves entering the lagoon through passes appears to be a critical determinant of rhodolith abundance, morphotype, and in turn cryptofaunal composition...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/520407t8</guid>
      <pubDate>Wed, 27 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Abrecht, Mira</name>
      </author>
      <author>
        <name>Peinemann, Viktor Nunes</name>
      </author>
      <author>
        <name>Yazaryan, Ara Kevork</name>
      </author>
      <author>
        <name>Kestler, Madeline</name>
      </author>
      <author>
        <name>DeMattei, Braden Charles</name>
      </author>
      <author>
        <name>Hà, Benjamin A</name>
      </author>
      <author>
        <name>Ryznar, Emily</name>
      </author>
      <author>
        <name>Jacobs, David K</name>
        <uri>https://orcid.org/0000-0002-7252-1601</uri>
      </author>
    </item>
    <item>
      <title>Global physical controls on estuarine habitat distribution during sea level change: Consequences for genetic diversification through time</title>
      <link>https://escholarship.org/uc/item/3qs0m0qg</link>
      <description>Global physical controls on estuarine habitat distribution during sea level change: Consequences for genetic diversification through time</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3qs0m0qg</guid>
      <pubDate>Wed, 27 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Dolby, Greer A</name>
      </author>
      <author>
        <name>Bedolla, Arturo M</name>
      </author>
      <author>
        <name>Bennett, Scott EK</name>
      </author>
      <author>
        <name>Jacobs, David K</name>
        <uri>https://orcid.org/0000-0002-7252-1601</uri>
      </author>
    </item>
    <item>
      <title>Carbon sequestration during core formation implied by complex carbon polymerization</title>
      <link>https://escholarship.org/uc/item/93z6g7md</link>
      <description>Current estimates of the carbon flux between the surface and mantle are highly variable, and the total amount of carbon stored in closed hidden reservoirs is unknown. Understanding the forms in which carbon existed in the molten early Earth is a critical step towards quantifying the carbon budget of Earth's deep interior. Here we employ first-principles molecular dynamics to study the evolution of carbon species as a function of pressure in a pyrolite melt. We find that with increasing pressure, the abundance of CO2 and CO3 species decreases at the expense of CO4 and complex oxo-carbon polymers (CxOy) displaying multiple C-C bonds. We anticipate that polymerized oxo-carbon species were a significant reservoir for carbon in the terrestrial magma ocean. The presence of Fe-C clusters suggests that upon segregation, Fe-rich metal may partition a significant fraction of carbon from the silicate liquid, leading to carbon transport into the Earth's core.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/93z6g7md</guid>
      <pubDate>Wed, 20 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Solomatova, Natalia V</name>
      </author>
      <author>
        <name>Caracas, Razvan</name>
      </author>
      <author>
        <name>Manning, Craig E</name>
      </author>
    </item>
    <item>
      <title>Jump rope vortex in liquid metal convection</title>
      <link>https://escholarship.org/uc/item/82x0n1rg</link>
      <description>Understanding large-scale circulations (LSCs) in turbulent convective systems is important for the study of stars, planets, and in many industrial applications. The canonical model of the LSC is quasi-planar with additional horizontal sloshing and torsional modes [Brown E, Ahlers G (2009) &lt;i&gt;J Fluid Mech&lt;/i&gt; 638:383-400; Funfschilling D, Ahlers G (2004) &lt;i&gt;Phys Rev Lett&lt;/i&gt; 92:194502; Xi HD et al. (2009) &lt;i&gt;Phys Rev Lett&lt;/i&gt; 102:044503; Zhou Q et al. (2009) &lt;i&gt;J Fluid Mech&lt;/i&gt; 630:367-390]. Using liquid gallium as the working fluid, we show, via coupled laboratory-numerical experiments in tanks with aspect ratios greater than unity ([Formula: see text]), that the LSC takes instead the form of a "jump rope vortex," a strongly 3D mode that periodically orbits around the tank following a motion much like a jump rope on a playground. Further experiments show that this jump rope flow also exists in more viscous fluids such as water, albeit with a far smaller signal. Thus, this jump...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/82x0n1rg</guid>
      <pubDate>Wed, 20 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Vogt, Tobias</name>
      </author>
      <author>
        <name>Horn, Susanne</name>
      </author>
      <author>
        <name>Grannan, Alexander M</name>
      </author>
      <author>
        <name>Aurnou, Jonathan M</name>
        <uri>https://orcid.org/0000-0002-8642-2962</uri>
      </author>
    </item>
    <item>
      <title>Geomagnetic polar minima do not arise from steady meridional circulation</title>
      <link>https://escholarship.org/uc/item/2bg3w9kc</link>
      <description>Observations of the Earth's magnetic field have revealed locally pronounced field minima near each pole at the core-mantle boundary (CMB). The existence of the polar magnetic minima has long been attributed to the supposed large-scale overturning circulation of molten metal in the outer core: Fluid upwells within the inner core tangent cylinder toward the poles and then diverges toward lower latitudes when it reaches the CMB, where Coriolis effects sweep the fluid into anticyclonic vortical flows. The diverging near-surface meridional circulation is believed to advectively draw magnetic flux away from the poles, resulting in the low intensity or even reversed polar magnetic fields. However, the interconnections between polar magnetic minima and meridional circulations have not to date been ascertained quantitatively. Here, we quantify the magnetic effects of steady, axisymmetric meridional circulation via numerically solving the axisymmetric magnetohydrodynamic equations for Earth's...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2bg3w9kc</guid>
      <pubDate>Wed, 20 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Cao, Hao</name>
      </author>
      <author>
        <name>Yadav, Rakesh K</name>
      </author>
      <author>
        <name>Aurnou, Jonathan M</name>
        <uri>https://orcid.org/0000-0002-8642-2962</uri>
      </author>
    </item>
    <item>
      <title>Abundant presolar grains and primordial organics preserved in carbon-rich exogenous clasts in asteroid Ryugu</title>
      <link>https://escholarship.org/uc/item/4rf3r6w7</link>
      <description>Preliminary analyses of asteroid Ryugu samples show kinship to aqueously altered CI (Ivuna-type) chondrites, suggesting similar origins. We report identification of C-rich, particularly primitive clasts in Ryugu samples that contain preserved presolar silicate grains and exceptional abundances of presolar SiC and isotopically anomalous organic matter. The high presolar silicate abundance (104 ppm) indicates that the clast escaped extensive alteration. The 5 to 10 times higher abundances of presolar SiC (~235 ppm), N-rich organic matter, organics with N isotopic anomalies (1.2%), and organics with C isotopic anomalies (0.2%) in the primitive clasts compared to bulk Ryugu suggest that the clasts formed in a unique part of the protoplanetary disk enriched in presolar materials. These clasts likely represent previously unsampled outer solar system material that accreted onto Ryugu after aqueous alteration ceased, consistent with Ryugu's rubble pile origin.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4rf3r6w7</guid>
      <pubDate>Tue, 19 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Nguyen, Ann N</name>
      </author>
      <author>
        <name>Mane, Prajkta</name>
      </author>
      <author>
        <name>Keller, Lindsay P</name>
      </author>
      <author>
        <name>Piani, Laurette</name>
      </author>
      <author>
        <name>Abe, Yoshinari</name>
      </author>
      <author>
        <name>Aléon, Jérôme</name>
      </author>
      <author>
        <name>Alexander, Conel M O'D</name>
      </author>
      <author>
        <name>Amari, Sachiko</name>
      </author>
      <author>
        <name>Amelin, Yuri</name>
      </author>
      <author>
        <name>Bajo, Ken-ichi</name>
      </author>
      <author>
        <name>Bizzarro, Martin</name>
      </author>
      <author>
        <name>Bouvier, Audrey</name>
      </author>
      <author>
        <name>Carlson, Richard W</name>
      </author>
      <author>
        <name>Chaussidon, Marc</name>
      </author>
      <author>
        <name>Choi, Byeon-Gak</name>
      </author>
      <author>
        <name>Dauphas, Nicolas</name>
      </author>
      <author>
        <name>Davis, Andrew M</name>
      </author>
      <author>
        <name>Di Rocco, Tommaso</name>
      </author>
      <author>
        <name>Fujiya, Wataru</name>
      </author>
      <author>
        <name>Fukai, Ryota</name>
      </author>
      <author>
        <name>Gautam, Ikshu</name>
      </author>
      <author>
        <name>Haba, Makiko K</name>
      </author>
      <author>
        <name>Hibiya, Yuki</name>
      </author>
      <author>
        <name>Hidaka, Hiroshi</name>
      </author>
      <author>
        <name>Homma, Hisashi</name>
      </author>
      <author>
        <name>Hoppe, Peter</name>
      </author>
      <author>
        <name>Huss, Gary R</name>
      </author>
      <author>
        <name>Ichida, Kiyohiro</name>
      </author>
      <author>
        <name>Iizuka, Tsuyoshi</name>
      </author>
      <author>
        <name>Ireland, Trevor R</name>
      </author>
      <author>
        <name>Ishikawa, Akira</name>
      </author>
      <author>
        <name>Itoh, Shoichi</name>
      </author>
      <author>
        <name>Kawasaki, Noriyuki</name>
      </author>
      <author>
        <name>Kita, Noriko T</name>
      </author>
      <author>
        <name>Kitajima, Kouki</name>
      </author>
      <author>
        <name>Kleine, Thorsten</name>
      </author>
      <author>
        <name>Komatani, Shintaro</name>
      </author>
      <author>
        <name>Krot, Alexander N</name>
      </author>
      <author>
        <name>Liu, Ming-Chang</name>
      </author>
      <author>
        <name>Masuda, Yuki</name>
      </author>
      <author>
        <name>McKeegan, Kevin D</name>
      </author>
      <author>
        <name>Morita, Mayu</name>
      </author>
      <author>
        <name>Motomura, Kazuko</name>
      </author>
      <author>
        <name>Moynier, Frédéric</name>
      </author>
      <author>
        <name>Nakai, Izumi</name>
      </author>
      <author>
        <name>Nagashima, Kazuhide</name>
      </author>
      <author>
        <name>Nesvorný, David</name>
      </author>
      <author>
        <name>Nittler, Larry</name>
      </author>
      <author>
        <name>Onose, Morihiko</name>
      </author>
      <author>
        <name>Pack, Andreas</name>
      </author>
      <author>
        <name>Park, Changkun</name>
      </author>
      <author>
        <name>Qin, Liping</name>
      </author>
      <author>
        <name>Russell, Sara S</name>
      </author>
      <author>
        <name>Sakamoto, Naoya</name>
      </author>
      <author>
        <name>Schönbächler, Maria</name>
      </author>
      <author>
        <name>Tafla, Lauren</name>
      </author>
      <author>
        <name>Tang, Haolan</name>
      </author>
      <author>
        <name>Terada, Kentaro</name>
      </author>
      <author>
        <name>Terada, Yasuko</name>
      </author>
      <author>
        <name>Usui, Tomohiro</name>
      </author>
      <author>
        <name>Wada, Sohei</name>
      </author>
      <author>
        <name>Wadhwa, Meenakshi</name>
      </author>
      <author>
        <name>Walker, Richard J</name>
      </author>
      <author>
        <name>Yamashita, Katsuyuki</name>
      </author>
      <author>
        <name>Yin, Qing-Zhu</name>
        <uri>https://orcid.org/0000-0002-4445-5096</uri>
      </author>
      <author>
        <name>Yokoyama, Tetsuya</name>
      </author>
      <author>
        <name>Yoneda, Shigekazu</name>
      </author>
      <author>
        <name>Young, Edward D</name>
        <uri>https://orcid.org/0000-0002-1299-0801</uri>
      </author>
      <author>
        <name>Yui, Hiroharu</name>
      </author>
      <author>
        <name>Zhang, Ai-Cheng</name>
      </author>
      <author>
        <name>Nakamura, Tomoki</name>
      </author>
      <author>
        <name>Naraoka, Hiroshi</name>
      </author>
      <author>
        <name>Noguchi, Takaaki</name>
      </author>
      <author>
        <name>Okazaki, Ryuji</name>
      </author>
      <author>
        <name>Sakamoto, Kanako</name>
      </author>
      <author>
        <name>Yabuta, Hikaru</name>
      </author>
      <author>
        <name>Abe, Masanao</name>
      </author>
      <author>
        <name>Miyazaki, Akiko</name>
      </author>
      <author>
        <name>Nakato, Aiko</name>
      </author>
      <author>
        <name>Nishimura, Masahiro</name>
      </author>
      <author>
        <name>Okada, Tatsuaki</name>
      </author>
      <author>
        <name>Yada, Toru</name>
      </author>
      <author>
        <name>Yogata, Kasumi</name>
      </author>
      <author>
        <name>Nakazawa, Satoru</name>
      </author>
      <author>
        <name>Saiki, Takanao</name>
      </author>
      <author>
        <name>Tanaka, Satoshi</name>
      </author>
      <author>
        <name>Terui, Fuyuto</name>
      </author>
      <author>
        <name>Tsuda, Yuichi</name>
      </author>
      <author>
        <name>Watanabe, Sei-ichiro</name>
      </author>
      <author>
        <name>Yoshikawa, Makoto</name>
      </author>
      <author>
        <name>Tachibana, Shogo</name>
      </author>
      <author>
        <name>Yurimoto, Hisayoshi</name>
      </author>
    </item>
    <item>
      <title>The cross-over to magnetostrophic convection in planetary dynamo systems</title>
      <link>https://escholarship.org/uc/item/0bp3652j</link>
      <description>Global scale magnetostrophic balance, in which Lorentz and Coriolis forces comprise the leading-order force balance, has long been thought to describe the natural state of planetary dynamo systems. This argument arises from consideration of the linear theory of rotating magnetoconvection. Here we test this long-held tenet by directly comparing linear predictions against dynamo modelling results. This comparison shows that dynamo modelling results are not typically in the global magnetostrophic state predicted by linear theory. Then, in order to estimate at what scale (if any) magnetostrophic balance will arise in nonlinear dynamo systems, we carry out a simple scaling analysis of the Elsasser number &lt;i&gt;Λ&lt;/i&gt;, yielding an improved estimate of the ratio of Lorentz and Coriolis forces. From this, we deduce that there is a magnetostrophic cross-over length scale, [Formula: see text], where &lt;i&gt;Λ&lt;/i&gt;&lt;sub&gt;&lt;i&gt;o&lt;/i&gt;&lt;/sub&gt; is the linear (or traditional) Elsasser number, &lt;i&gt;Rm&lt;/i&gt;&lt;sub&gt;&lt;i&gt;o&lt;/i&gt;&lt;/sub&gt;...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0bp3652j</guid>
      <pubDate>Mon, 18 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Aurnou, JM</name>
        <uri>https://orcid.org/0000-0002-8642-2962</uri>
      </author>
      <author>
        <name>King, EM</name>
      </author>
    </item>
    <item>
      <title>Processing of methane and acetylene ices by galactic cosmic rays and implications to the color diversity of Kuiper Belt objects</title>
      <link>https://escholarship.org/uc/item/659774dv</link>
      <description>Kuiper Belt objects exhibit a wider color range than any other solar system population. The origin of this color diversity is unknown, but likely the result of the prolonged irradiation of organic materials by galactic cosmic rays (GCRs). Here, we combine ultrahigh-vacuum irradiation experiments with comprehensive spectroscopic analyses to examine the color evolution during GCR processing methane and acetylene under Kuiper Belt conditions. This study replicates the colors of a population of Kuiper Belt objects such as Makemake, Orcus, and Salacia. Aromatic structural units carrying up to three rings as in phenanthrene (C&lt;sub&gt;14&lt;/sub&gt;H&lt;sub&gt;10&lt;/sub&gt;), phenalene (C&lt;sub&gt;9&lt;/sub&gt;H&lt;sub&gt;10&lt;/sub&gt;), and acenaphthylene (C&lt;sub&gt;12&lt;/sub&gt;H&lt;sub&gt;8&lt;/sub&gt;), of which some carry structural motives of DNA and RNA connected via unsaturated linkers, were found to play a key role in producing the reddish colors. These studies demonstrate the level of molecular complexity synthesized of GCR processing...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/659774dv</guid>
      <pubDate>Sat, 16 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Zhang, Chaojiang</name>
      </author>
      <author>
        <name>Zhu, Cheng</name>
      </author>
      <author>
        <name>Turner, Andrew M</name>
      </author>
      <author>
        <name>Antonov, Ivan O</name>
      </author>
      <author>
        <name>Garcia, Adrien D</name>
      </author>
      <author>
        <name>Meinert, Cornelia</name>
      </author>
      <author>
        <name>Young, Leslie A</name>
      </author>
      <author>
        <name>Jewitt, David C</name>
      </author>
      <author>
        <name>Kaiser, Ralf I</name>
      </author>
    </item>
    <item>
      <title>3-D synthetic modelling and observations of anisotropy effects on SS precursors: implications for mantle deformation in the transition zone</title>
      <link>https://escholarship.org/uc/item/9cz1w44h</link>
      <description>SUMMARY: 

               The Earth's mantle transition zone (MTZ) plays a key role in the thermal and compositional interactions between the upper and lower mantle. Seismic anisotropy provides useful information about mantle deformation and dynamics across the MTZ. However, seismic anisotropy in the MTZ is difficult to constrain from surface wave or shear wave splitting measurements. Here, we investigate the sensitivity to anisotropy of a body wave method, SS precursors, through 3-D synthetic modelling and apply it to real data. Our study shows that the SS precursors can distinguish the anisotropy originating from three depths: shallow upper mantle (80–220&amp;nbsp;km), deep upper mantle above 410 km, and MTZ (410–660&amp;nbsp;km). Synthetic resolution tests indicate that SS precursors can resolve $\ge $3 per cent azimuthal anisotropy where data have an average signal-to-noise ratio (SNR&amp;nbsp;=&amp;nbsp;7) and sufficient azimuthal coverage. To investigate regional sensitivity, we apply the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9cz1w44h</guid>
      <pubDate>Thu, 14 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Huang, Quancheng</name>
      </author>
      <author>
        <name>Schmerr, Nicholas C</name>
      </author>
      <author>
        <name>Beghein, Caroline</name>
        <uri>https://orcid.org/0000-0002-3158-2213</uri>
      </author>
      <author>
        <name>Waszek, Lauren</name>
      </author>
      <author>
        <name>Maguire, Ross R</name>
      </author>
    </item>
    <item>
      <title>Upper mantle radial anisotropy under the Indian Ocean from higher mode surface waves and a hierarchical transdismensional approach</title>
      <link>https://escholarship.org/uc/item/50c1q9vj</link>
      <description>SUMMARY: 

               We investigated the likelihood of radial anisotropy in the shallow and deep upper mantle, including the mantle transition zone (MTZ) under the Indian Ocean. Seismic anisotropy can be an indicator of mantle deformation through lattice preferred orientation of anisotropic crystals in the mantle. It has thus the potential to illuminate Earth’s dynamic interior, but previous seismic tomography studies have not achieved consensus on the existence of radial anisotropy below ∼250&amp;nbsp;km depth. We developed a fully nonlinear transdimensional hierarchical Bayesian Markov Chain Monte Carlo approach to invert fundamental and higher mode surface wave dispersion data and applied it to a subset of a global Love and Rayleigh wave data set. We obtained posterior model parameter distributions for shear wave velocity (VS) and radial anisotropy ξ under the Indian Ocean. These posterior model distributions were used to calculate the probability of having radial anisotropy...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/50c1q9vj</guid>
      <pubDate>Thu, 14 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Weidner, Erik</name>
      </author>
      <author>
        <name>Beghein, Caroline</name>
        <uri>https://orcid.org/0000-0002-3158-2213</uri>
      </author>
      <author>
        <name>Huang, Quancheng</name>
      </author>
      <author>
        <name>Schmerr, Nicholas</name>
      </author>
    </item>
    <item>
      <title>Focal Mechanism Determination of Event S1222a and Implications for Tectonics Near the Dichotomy Boundary in Southern Elysium Planitia, Mars</title>
      <link>https://escholarship.org/uc/item/0tt0z9mk</link>
      <description>Abstract: 
On 4 May 2022 the InSight seismometer SEIS‐VBB recorded the largest marsquake ever observed, S1222a, with an initial magnitude estimate of  4.6. Understanding the depth and source properties of this event has important implications for the nature of tectonic activity on Mars. Located ∼37° to the southeast of InSight, S1222a is one of the few non‐impact marsquakes that exhibits prominent surface waves. We use waveform modeling of body waves (P and S) and surface waves (Rayleigh and Love) to constrain the focal mechanism, assuming a double‐couple source, and find that S1222a likely resulted from reverse faulting in the crust (source depth near 22&amp;nbsp;km). We estimate the scalar moment to be 2.5&amp;nbsp;×&amp;nbsp;1015–3.5&amp;nbsp;×&amp;nbsp;1015 Nm (magnitude MW 4.2–4.3). Our results suggest active compressional tectonics near the dichotomy boundary on Mars, likely due to thermal contraction from planetary cooling.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0tt0z9mk</guid>
      <pubDate>Thu, 14 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Maguire, R</name>
      </author>
      <author>
        <name>Lekić, V</name>
      </author>
      <author>
        <name>Kim, D</name>
      </author>
      <author>
        <name>Schmerr, N</name>
      </author>
      <author>
        <name>Li, J</name>
      </author>
      <author>
        <name>Beghein, C</name>
        <uri>https://orcid.org/0000-0002-3158-2213</uri>
      </author>
      <author>
        <name>Huang, Q</name>
      </author>
      <author>
        <name>Irving, JCE</name>
      </author>
      <author>
        <name>Karakostas, F</name>
      </author>
      <author>
        <name>Lognonné, P</name>
      </author>
      <author>
        <name>Stähler, SC</name>
      </author>
      <author>
        <name>Banerdt, WB</name>
      </author>
    </item>
    <item>
      <title>Igneous meteorites suggest Aluminium-26 heterogeneity in the early Solar Nebula</title>
      <link>https://escholarship.org/uc/item/9tq260c3</link>
      <description>The short-lived radionuclide aluminium-26 (26Al) isotope is a major heat source for early planetary melting. The aluminium-26 – magnesium-26 (26Al-26Mg) decay system also serves as a high-resolution relative chronometer. In both cases, however, it is critical to establish whether 26Al was homogeneously or heterogeneously distributed throughout the solar nebula. Here we report a precise lead-207 – lead-206 (207Pb-206Pb) isotopic age of 4565.56 ± 0.12 million years (Ma) for the andesitic achondrite Erg Chech 002. Our analysis, in conjunction with published 26Al-26Mg data, reveals that the initial 26Al/27Al in the source material of this achondrite was notably higher than in various other well-preserved and precisely dated achondrites. Here we demonstrate that the current data clearly indicate spatial heterogeneity of 26Al by a factor of 3-4 in the precursor molecular cloud or the protoplanetary disk of the Solar System, likely associated with the late infall of stellar materials...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9tq260c3</guid>
      <pubDate>Mon, 11 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Krestianinov, Evgenii</name>
      </author>
      <author>
        <name>Amelin, Yuri</name>
      </author>
      <author>
        <name>Yin, Qing-Zhu</name>
        <uri>https://orcid.org/0000-0002-4445-5096</uri>
      </author>
      <author>
        <name>Cary, Paige</name>
      </author>
      <author>
        <name>Huyskens, Magdalena H</name>
      </author>
      <author>
        <name>Miller, Audrey</name>
        <uri>https://orcid.org/0000-0001-7374-0622</uri>
      </author>
      <author>
        <name>Dey, Supratim</name>
      </author>
      <author>
        <name>Hibiya, Yuki</name>
      </author>
      <author>
        <name>Tang, Haolan</name>
      </author>
      <author>
        <name>Young, Edward D</name>
        <uri>https://orcid.org/0000-0002-1299-0801</uri>
      </author>
      <author>
        <name>Pack, Andreas</name>
      </author>
      <author>
        <name>Di Rocco, Tommaso</name>
      </author>
    </item>
    <item>
      <title>Energetic Electron Precipitation Driven by Electromagnetic Ion Cyclotron Waves from ELFIN’s Low Altitude Perspective</title>
      <link>https://escholarship.org/uc/item/9v56s8fr</link>
      <description>We review comprehensive observations of electromagnetic ion cyclotron (EMIC) wave-driven energetic electron precipitation using data collected by the energetic electron detector on the Electron Losses and Fields InvestigatioN (ELFIN) mission, two polar-orbiting low-altitude spinning CubeSats, measuring 50-5000&amp;nbsp;keV electrons with good pitch-angle and energy resolution. EMIC wave-driven precipitation exhibits a distinct signature in energy-spectrograms of the precipitating-to-trapped flux ratio: peaks at &amp;gt;0.5&amp;nbsp;MeV which are abrupt (bursty) (lasting ∼17&amp;nbsp;s, or ΔL∼0.56$$\Delta L\sim 0.56$$) with significant substructure (occasionally down to sub-second timescale). We attribute the bursty nature of the precipitation to the spatial extent and structuredness of the wave field at the equator. Multiple ELFIN passes over the same MLT sector allow us to study the spatial and temporal evolution of the EMIC wave - electron interaction region. Case studies employing conjugate...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9v56s8fr</guid>
      <pubDate>Mon, 14 Aug 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Angelopoulos, V</name>
        <uri>https://orcid.org/0000-0001-7024-1561</uri>
      </author>
      <author>
        <name>Zhang, X-J</name>
      </author>
      <author>
        <name>Artemyev, AV</name>
      </author>
      <author>
        <name>Mourenas, D</name>
      </author>
      <author>
        <name>Tsai, E</name>
      </author>
      <author>
        <name>Wilkins, C</name>
      </author>
      <author>
        <name>Runov, A</name>
      </author>
      <author>
        <name>Liu, J</name>
        <uri>https://orcid.org/0000-0002-7489-9384</uri>
      </author>
      <author>
        <name>Turner, DL</name>
      </author>
      <author>
        <name>Li, W</name>
      </author>
      <author>
        <name>Khurana, K</name>
      </author>
      <author>
        <name>Wirz, RE</name>
      </author>
      <author>
        <name>Sergeev, VA</name>
      </author>
      <author>
        <name>Meng, X</name>
      </author>
      <author>
        <name>Wu, J</name>
      </author>
      <author>
        <name>Hartinger, MD</name>
      </author>
      <author>
        <name>Raita, T</name>
      </author>
      <author>
        <name>Shen, Y</name>
      </author>
      <author>
        <name>An, X</name>
        <uri>https://orcid.org/0000-0003-2507-8632</uri>
      </author>
      <author>
        <name>Shi, X</name>
      </author>
      <author>
        <name>Bashir, MF</name>
      </author>
      <author>
        <name>Shen, X</name>
      </author>
      <author>
        <name>Gan, L</name>
      </author>
      <author>
        <name>Qin, M</name>
      </author>
      <author>
        <name>Capannolo, L</name>
      </author>
      <author>
        <name>Ma, Q</name>
        <uri>https://orcid.org/0000-0001-5452-4756</uri>
      </author>
      <author>
        <name>Russell, CL</name>
      </author>
      <author>
        <name>Masongsong, EV</name>
      </author>
      <author>
        <name>Caron, R</name>
      </author>
      <author>
        <name>He, I</name>
      </author>
      <author>
        <name>Iglesias, L</name>
      </author>
      <author>
        <name>Jha, S</name>
      </author>
      <author>
        <name>King, J</name>
      </author>
      <author>
        <name>Kumar, S</name>
      </author>
      <author>
        <name>Le, K</name>
      </author>
      <author>
        <name>Mao, J</name>
      </author>
      <author>
        <name>McDermott, A</name>
      </author>
      <author>
        <name>Nguyen, K</name>
      </author>
      <author>
        <name>Norris, A</name>
      </author>
      <author>
        <name>Palla, A</name>
      </author>
      <author>
        <name>Roosnovo, A</name>
      </author>
      <author>
        <name>Tam, J</name>
      </author>
      <author>
        <name>Xie, E</name>
      </author>
      <author>
        <name>Yap, RC</name>
      </author>
      <author>
        <name>Ye, S</name>
      </author>
      <author>
        <name>Young, C</name>
      </author>
      <author>
        <name>Adair, LA</name>
      </author>
      <author>
        <name>Shaffer, C</name>
      </author>
      <author>
        <name>Chung, M</name>
      </author>
      <author>
        <name>Cruce, P</name>
      </author>
      <author>
        <name>Lawson, M</name>
      </author>
      <author>
        <name>Leneman, D</name>
      </author>
      <author>
        <name>Allen, M</name>
      </author>
      <author>
        <name>Anderson, M</name>
      </author>
      <author>
        <name>Arreola-Zamora, M</name>
      </author>
      <author>
        <name>Artinger, J</name>
      </author>
      <author>
        <name>Asher, J</name>
      </author>
      <author>
        <name>Branchevsky, D</name>
      </author>
      <author>
        <name>Cliffe, M</name>
      </author>
      <author>
        <name>Colton, K</name>
      </author>
      <author>
        <name>Costello, C</name>
      </author>
      <author>
        <name>Depe, D</name>
      </author>
      <author>
        <name>Domae, BW</name>
      </author>
      <author>
        <name>Eldin, S</name>
      </author>
      <author>
        <name>Fitzgibbon, L</name>
      </author>
      <author>
        <name>Flemming, A</name>
      </author>
      <author>
        <name>Frederick, DM</name>
      </author>
      <author>
        <name>Gilbert, A</name>
      </author>
      <author>
        <name>Hesford, B</name>
      </author>
      <author>
        <name>Krieger, R</name>
      </author>
      <author>
        <name>Lian, K</name>
      </author>
      <author>
        <name>McKinney, E</name>
      </author>
      <author>
        <name>Miller, JP</name>
      </author>
      <author>
        <name>Pedersen, C</name>
      </author>
      <author>
        <name>Qu, Z</name>
      </author>
      <author>
        <name>Rozario, R</name>
      </author>
      <author>
        <name>Rubly, M</name>
      </author>
      <author>
        <name>Seaton, R</name>
      </author>
      <author>
        <name>Subramanian, A</name>
      </author>
      <author>
        <name>Sundin, SR</name>
      </author>
      <author>
        <name>Tan, A</name>
      </author>
      <author>
        <name>Thomlinson, D</name>
      </author>
      <author>
        <name>Turner, W</name>
      </author>
      <author>
        <name>Wing, G</name>
      </author>
      <author>
        <name>Wong, C</name>
      </author>
      <author>
        <name>Zarifian, A</name>
      </author>
    </item>
    <item>
      <title>Interchange reconnection as the source of the fast solar wind within coronal holes</title>
      <link>https://escholarship.org/uc/item/73n4x0s9</link>
      <description>The fast solar wind that fills the heliosphere originates from deep within regions of open magnetic field on the Sun called ‘coronal holes’. The energy source responsible for accelerating the plasma is widely debated; however, there is evidence that it is ultimately magnetic in nature, with candidate mechanisms including wave heating1,2 and interchange reconnection3–5. The coronal magnetic field near the solar surface is structured on scales associated with ‘supergranulation’ convection cells, whereby descending flows create intense fields. The energy density in these ‘network’ magnetic field bundles is a candidate energy source for the wind. Here we report measurements of fast solar wind streams from the Parker Solar Probe (PSP) spacecraft6 that provide strong evidence for the interchange reconnection mechanism. We show that the supergranulation structure at the coronal base remains imprinted in the near-Sun solar wind, resulting in asymmetric patches of magnetic ‘switchbacks’7,8...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/73n4x0s9</guid>
      <pubDate>Tue, 18 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Bale, SD</name>
        <uri>https://orcid.org/0000-0002-1989-3596</uri>
      </author>
      <author>
        <name>Drake, JF</name>
      </author>
      <author>
        <name>McManus, MD</name>
      </author>
      <author>
        <name>Desai, MI</name>
      </author>
      <author>
        <name>Badman, ST</name>
      </author>
      <author>
        <name>Larson, DE</name>
      </author>
      <author>
        <name>Swisdak, M</name>
      </author>
      <author>
        <name>Horbury, TS</name>
      </author>
      <author>
        <name>Raouafi, NE</name>
      </author>
      <author>
        <name>Phan, T</name>
      </author>
      <author>
        <name>Velli, M</name>
        <uri>https://orcid.org/0000-0002-2381-3106</uri>
      </author>
      <author>
        <name>McComas, DJ</name>
      </author>
      <author>
        <name>Cohen, CMS</name>
      </author>
      <author>
        <name>Mitchell, D</name>
      </author>
      <author>
        <name>Panasenco, O</name>
      </author>
      <author>
        <name>Kasper, JC</name>
      </author>
    </item>
    <item>
      <title>First observations of core-transiting seismic phases on Mars</title>
      <link>https://escholarship.org/uc/item/18j8b3nz</link>
      <description>We present the first observations of seismic waves propagating through the core of Mars. These observations, made using seismic data collected by the InSight geophysical mission, have allowed us to construct the first seismically constrained models for the elastic properties of Mars' core. We observe core-transiting seismic phase SKS from two farside seismic events detected on Mars and measure the travel times of SKS relative to mantle traversing body waves. SKS travels through the core as a compressional wave, providing information about bulk modulus and density. We perform probabilistic inversions using the core-sensitive relative travel times together with gross geophysical data and travel times from other, more proximal, seismic events to seek the equation of state parameters that best describe the liquid iron-alloy core. Our inversions provide constraints on the velocities in Mars' core and are used to develop the first seismically based estimates of its composition. We show...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/18j8b3nz</guid>
      <pubDate>Sat, 15 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Irving, Jessica CE</name>
      </author>
      <author>
        <name>Lekić, Vedran</name>
      </author>
      <author>
        <name>Durán, Cecilia</name>
      </author>
      <author>
        <name>Drilleau, Mélanie</name>
      </author>
      <author>
        <name>Kim, Doyeon</name>
      </author>
      <author>
        <name>Rivoldini, Attilio</name>
      </author>
      <author>
        <name>Khan, Amir</name>
      </author>
      <author>
        <name>Samuel, Henri</name>
      </author>
      <author>
        <name>Antonangeli, Daniele</name>
      </author>
      <author>
        <name>Banerdt, William Bruce</name>
      </author>
      <author>
        <name>Beghein, Caroline</name>
        <uri>https://orcid.org/0000-0002-3158-2213</uri>
      </author>
      <author>
        <name>Bozdağ, Ebru</name>
      </author>
      <author>
        <name>Ceylan, Savas</name>
      </author>
      <author>
        <name>Charalambous, Constantinos</name>
      </author>
      <author>
        <name>Clinton, John</name>
      </author>
      <author>
        <name>Davis, Paul</name>
      </author>
      <author>
        <name>Garcia, Raphaël</name>
      </author>
      <author>
        <name>Giardini, Domenico</name>
      </author>
      <author>
        <name>Horleston, Anna Catherine</name>
      </author>
      <author>
        <name>Huang, Quancheng</name>
      </author>
      <author>
        <name>Hurst, Kenneth J</name>
      </author>
      <author>
        <name>Kawamura, Taichi</name>
      </author>
      <author>
        <name>King, Scott D</name>
      </author>
      <author>
        <name>Knapmeyer, Martin</name>
      </author>
      <author>
        <name>Li, Jiaqi</name>
      </author>
      <author>
        <name>Lognonné, Philippe</name>
      </author>
      <author>
        <name>Maguire, Ross</name>
      </author>
      <author>
        <name>Panning, Mark P</name>
      </author>
      <author>
        <name>Plesa, Ana-Catalina</name>
      </author>
      <author>
        <name>Schimmel, Martin</name>
      </author>
      <author>
        <name>Schmerr, Nicholas C</name>
      </author>
      <author>
        <name>Stähler, Simon C</name>
      </author>
      <author>
        <name>Stutzmann, Eleonore</name>
      </author>
      <author>
        <name>Xu, Zongbo</name>
      </author>
    </item>
    <item>
      <title>A novel neural network model of Earth’s topside ionosphere</title>
      <link>https://escholarship.org/uc/item/7g86g67n</link>
      <description>The Earth’s ionosphere affects the propagation of signals from the Global Navigation Satellite Systems (GNSS). Due to the non-uniform coverage of available observations and complicated dynamics of the region, developing accurate models of the ionosphere has been a long-standing challenge. Here, we present a Neural network-based model of Electron density in the Topside ionosphere (NET), which is constructed using 19 years of GNSS radio occultation data. The NET model is tested against in situ measurements from several missions and shows excellent agreement with the observations, outperforming the state-of-the-art International Reference Ionosphere (IRI) model by up to an order of magnitude, especially at 100-200 km above the F2-layer peak. This study provides a paradigm shift in ionospheric research, by demonstrating that ionospheric densities can be reconstructed with very high fidelity. The NET model depicts the effects of numerous physical processes governing the topside dynamics...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7g86g67n</guid>
      <pubDate>Tue, 11 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Smirnov, Artem</name>
      </author>
      <author>
        <name>Shprits, Yuri</name>
        <uri>https://orcid.org/0000-0002-9625-0834</uri>
      </author>
      <author>
        <name>Prol, Fabricio</name>
      </author>
      <author>
        <name>Lühr, Hermann</name>
      </author>
      <author>
        <name>Berrendorf, Max</name>
      </author>
      <author>
        <name>Zhelavskaya, Irina</name>
      </author>
      <author>
        <name>Xiong, Chao</name>
      </author>
    </item>
    <item>
      <title>A missing dusk-side loss process in the terrestrial electron ring current</title>
      <link>https://escholarship.org/uc/item/6h64380r</link>
      <description>The Earth’s magnetic field traps charged particles which are transported longitudinally around Earth, generating a near-circular current, known as the ring current. While the ring current has been measured on the ground and space for many decades, the enhancement of the ring current during geomagnetic storms is still not well understood, due to many processes contributing to its dynamics on different time scales. Here, we show that existing ring current models systematically overestimate electron flux observations of 10–50 keV on the nightside during storm onset. By analyzing electron drift trajectories, we show that this systematic overestimation of flux can be explained through a missing loss process which operates in the pre-midnight sector. Quantifying this loss reveals that the theoretical upper limit of loss has to be reached over a broad region of space in order to reproduce the observations. This missing loss may be attributed to inaccuracies in the parameterization of...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6h64380r</guid>
      <pubDate>Tue, 11 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Haas, Bernhard</name>
      </author>
      <author>
        <name>Shprits, Yuri Y</name>
        <uri>https://orcid.org/0000-0002-9625-0834</uri>
      </author>
      <author>
        <name>Allison, Hayley J</name>
      </author>
      <author>
        <name>Wutzig, Michael</name>
      </author>
      <author>
        <name>Wang, Dedong</name>
      </author>
    </item>
    <item>
      <title>Sclerites of the soft coral Ovabunda macrospiculata (Xeniidae) are predominantly the metastable CaCO3 polymorph vaterite</title>
      <link>https://escholarship.org/uc/item/7417k25q</link>
      <description>Soft corals (Cnidaria, Anthozoa, Octocorallia, Alcyonacea) produce internal sclerites of calcium carbonate previously shown to be composed of calcite, the most stable calcium carbonate polymorph. Here we apply multiple imaging and physical chemistry analyses to extracted and in-vivo sclerites of the abundant Red Sea soft coral, Ovabunda macrospiculata, to detail their mineralogy. We show that this species' sclerites are comprised predominantly of the less stable calcium carbonate polymorph vaterite (&amp;gt;&amp;nbsp;95%), with much smaller components of aragonite and calcite. Use of this mineral, which is typically considered to be metastable, by these soft corals has implications for how it is formed as well as how it will persist during the anticipated anthropogenic climate change in the coming decades. This first documentation of vaterite dominating the mineral composition of O. macrospiculata sclerites is likely just the beginning of establishing its presence in other soft corals....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7417k25q</guid>
      <pubDate>Mon, 10 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Drake, Jeana L</name>
      </author>
      <author>
        <name>Benayahu, Yehuda</name>
      </author>
      <author>
        <name>Polishchuk, Iryna</name>
      </author>
      <author>
        <name>Pokroy, Boaz</name>
      </author>
      <author>
        <name>Pinkas, Iddo</name>
      </author>
      <author>
        <name>Mass, Tali</name>
      </author>
    </item>
    <item>
      <title>A phylogenomic perspective on the evolutionary history of the stonefly genus Suwallia (Plecoptera: Chloroperlidae) revealed by ultraconserved genomic elements</title>
      <link>https://escholarship.org/uc/item/5455s0qj</link>
      <description>Evolutionary biologists have long sought to disentangle phylogenetic relationships among taxa spanning the tree of life, an increasingly important task as anthropogenic influences accelerate population declines and species extinctions, particularly in insects. Phylogenetic analyses are commonly used to identify unique evolutionary lineages, to clarify taxonomic designations of the focal taxa, and to inform conservation decisions. Advances in DNA sequencing techniques have increasingly facilitated the ability of researchers to apply genomic methods to phylogenetic analyses, even for non-model organisms. Stoneflies are non-model insects that are important bioindicators of the quality of freshwater habitats and landscape disturbance as they spend the immature stages of their life cycles in fresh water, and the adult stages in terrestrial environments. Phylogenetic relationships within the stonefly genus Suwallia (Insecta: Plecoptera: Chloroperlidae) are poorly understood, and have...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5455s0qj</guid>
      <pubDate>Mon, 10 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Houston, Derek D</name>
      </author>
      <author>
        <name>Satler, Jordan D</name>
      </author>
      <author>
        <name>Stack, Taylor K</name>
      </author>
      <author>
        <name>Carroll, Hannah M</name>
      </author>
      <author>
        <name>Bevan, Alissa M</name>
      </author>
      <author>
        <name>Moya, Autumn L</name>
      </author>
      <author>
        <name>Alexander, Kevin D</name>
      </author>
    </item>
    <item>
      <title>Automated Detection Algorithm for Mesoscale Heated Regions in TWINS Ion Temperature Maps</title>
      <link>https://escholarship.org/uc/item/8td2s68q</link>
      <description>Earth's magnetotail plays a critical role in the dynamics of the magnetosphere, particularly during intervals of geomagnetic activity. To improve our understanding of the ion dynamics in this region, energetic neutral atom (ENA) imaging can provide global measurements to place in situ measurements in context and validate simulations. The NASA Two Wide-angle Imaging Neutral-atom Spectrometers mission provided near-continuous observations using ENA imagers. ENA data can be used to calculate maps of equatorial ion temperatures that often show observations of regions of enhanced temperatures associated with phenomena in the magnetotail such as magnetic reconnection and narrow flow channels. We present an algorithm that can be used to search through a collection of these maps to identify intervals with such enhancements for further study. The algorithm results are validated against two sets of related phenomena: (a) a database of dipolarizing flux bundle (DFB) measurements from THEMIS...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8td2s68q</guid>
      <pubDate>Sat, 8 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Keesee, AM</name>
      </author>
      <author>
        <name>Katus, R</name>
      </author>
      <author>
        <name>Tibbetts, J</name>
      </author>
      <author>
        <name>Liu, J</name>
        <uri>https://orcid.org/0000-0002-7489-9384</uri>
      </author>
      <author>
        <name>Zhang, X</name>
      </author>
      <author>
        <name>Sorathia, KA</name>
      </author>
    </item>
    <item>
      <title>Extreme Energy Spectra of Relativistic Electron Flux in the Outer Radiation Belt</title>
      <link>https://escholarship.org/uc/item/4qm482bq</link>
      <description>Electron diffusion by whistler-mode chorus waves is one of the key processes controlling the dynamics of relativistic electron fluxes in the Earth's radiation belts. It is responsible for the acceleration of sub-relativistic electrons injected from the plasma sheet to relativistic energies as well as for their precipitation and loss into the atmosphere. Based on analytical estimates of chorus wave-driven quasi-linear electron energy and pitch-angle diffusion rates, we provide analytical steady-state solutions to the corresponding Fokker-Planck equation for the relativistic electron distribution and flux. The impact on these steady-state solutions of additional electromagnetic ion cyclotron waves, and of ultralow frequency waves are examined. Such steady-state solutions correspond to hard energy spectra at 1-4&amp;nbsp;MeV, dangerous for satellite electronics, and represent attractors for the system dynamics in the presence of sufficiently strong driving by continuous injections of...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4qm482bq</guid>
      <pubDate>Sat, 8 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Mourenas, D</name>
      </author>
      <author>
        <name>Artemyev, AV</name>
      </author>
      <author>
        <name>Zhang, X‐J</name>
      </author>
      <author>
        <name>Angelopoulos, V</name>
        <uri>https://orcid.org/0000-0001-7024-1561</uri>
      </author>
    </item>
    <item>
      <title>Oxygen isotopes of anhydrous primary minerals show kinship between asteroid Ryugu and comet 81P/Wild2</title>
      <link>https://escholarship.org/uc/item/3jr330z0</link>
      <description>The extraterrestrial materials returned from asteroid (162173) Ryugu consist predominantly of low-temperature aqueously formed secondary minerals and are chemically and mineralogically similar to CI (Ivuna-type) carbonaceous chondrites. Here, we show that high-temperature anhydrous primary minerals in Ryugu and CI chondrites exhibit a bimodal distribution of oxygen isotopic compositions: &lt;sup&gt;16&lt;/sup&gt;O-rich (associated with refractory inclusions) and &lt;sup&gt;16&lt;/sup&gt;O-poor (associated with chondrules). Both the &lt;sup&gt;16&lt;/sup&gt;O-rich and &lt;sup&gt;16&lt;/sup&gt;O-poor minerals probably formed in the inner solar protoplanetary disk and were subsequently transported outward. The abundance ratios of the &lt;sup&gt;16&lt;/sup&gt;O-rich to &lt;sup&gt;16&lt;/sup&gt;O-poor minerals in Ryugu and CI chondrites are higher than in other carbonaceous chondrite groups but are similar to that of comet 81P/Wild2, suggesting that Ryugu and CI chondrites accreted in the outer Solar System closer to the accretion region of comets.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3jr330z0</guid>
      <pubDate>Sat, 8 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Kawasaki, Noriyuki</name>
      </author>
      <author>
        <name>Nagashima, Kazuhide</name>
      </author>
      <author>
        <name>Sakamoto, Naoya</name>
      </author>
      <author>
        <name>Matsumoto, Toru</name>
      </author>
      <author>
        <name>Bajo, Ken-ichi</name>
      </author>
      <author>
        <name>Wada, Sohei</name>
      </author>
      <author>
        <name>Igami, Yohei</name>
      </author>
      <author>
        <name>Miyake, Akira</name>
      </author>
      <author>
        <name>Noguchi, Takaaki</name>
      </author>
      <author>
        <name>Yamamoto, Daiki</name>
      </author>
      <author>
        <name>Russell, Sara S</name>
      </author>
      <author>
        <name>Abe, Yoshinari</name>
      </author>
      <author>
        <name>Aléon, Jérôme</name>
      </author>
      <author>
        <name>Alexander, Conel M O’D</name>
      </author>
      <author>
        <name>Amari, Sachiko</name>
      </author>
      <author>
        <name>Amelin, Yuri</name>
      </author>
      <author>
        <name>Bizzarro, Martin</name>
      </author>
      <author>
        <name>Bouvier, Audrey</name>
      </author>
      <author>
        <name>Carlson, Richard W</name>
      </author>
      <author>
        <name>Chaussidon, Marc</name>
      </author>
      <author>
        <name>Choi, Byeon-Gak</name>
      </author>
      <author>
        <name>Dauphas, Nicolas</name>
      </author>
      <author>
        <name>Davis, Andrew M</name>
      </author>
      <author>
        <name>Di Rocco, Tommaso</name>
      </author>
      <author>
        <name>Fujiya, Wataru</name>
      </author>
      <author>
        <name>Fukai, Ryota</name>
      </author>
      <author>
        <name>Gautam, Ikshu</name>
      </author>
      <author>
        <name>Haba, Makiko K</name>
      </author>
      <author>
        <name>Hibiya, Yuki</name>
      </author>
      <author>
        <name>Hidaka, Hiroshi</name>
      </author>
      <author>
        <name>Homma, Hisashi</name>
      </author>
      <author>
        <name>Hoppe, Peter</name>
      </author>
      <author>
        <name>Huss, Gary R</name>
      </author>
      <author>
        <name>Ichida, Kiyohiro</name>
      </author>
      <author>
        <name>Iizuka, Tsuyoshi</name>
      </author>
      <author>
        <name>Ireland, Trevor R</name>
      </author>
      <author>
        <name>Ishikawa, Akira</name>
      </author>
      <author>
        <name>Ito, Motoo</name>
      </author>
      <author>
        <name>Itoh, Shoichi</name>
      </author>
      <author>
        <name>Kita, Noriko T</name>
      </author>
      <author>
        <name>Kitajima, Kouki</name>
      </author>
      <author>
        <name>Kleine, Thorsten</name>
      </author>
      <author>
        <name>Komatani, Shintaro</name>
      </author>
      <author>
        <name>Krot, Alexander N</name>
      </author>
      <author>
        <name>Liu, Ming-Chang</name>
      </author>
      <author>
        <name>Masuda, Yuki</name>
      </author>
      <author>
        <name>McKeegan, Kevin D</name>
      </author>
      <author>
        <name>Morita, Mayu</name>
      </author>
      <author>
        <name>Motomura, Kazuko</name>
      </author>
      <author>
        <name>Moynier, Frédéric</name>
      </author>
      <author>
        <name>Nakai, Izumi</name>
      </author>
      <author>
        <name>Nguyen, Ann</name>
      </author>
      <author>
        <name>Nittler, Larry</name>
      </author>
      <author>
        <name>Onose, Morihiko</name>
      </author>
      <author>
        <name>Pack, Andreas</name>
      </author>
      <author>
        <name>Park, Changkun</name>
      </author>
      <author>
        <name>Piani, Laurette</name>
      </author>
      <author>
        <name>Qin, Liping</name>
      </author>
      <author>
        <name>Schönbächler, Maria</name>
      </author>
      <author>
        <name>Tafla, Lauren</name>
      </author>
      <author>
        <name>Tang, Haolan</name>
      </author>
      <author>
        <name>Terada, Kentaro</name>
      </author>
      <author>
        <name>Terada, Yasuko</name>
      </author>
      <author>
        <name>Usui, Tomohiro</name>
      </author>
      <author>
        <name>Wadhwa, Meenakshi</name>
      </author>
      <author>
        <name>Walker, Richard J</name>
      </author>
      <author>
        <name>Yamashita, Katsuyuki</name>
      </author>
      <author>
        <name>Yin, Qing-Zhu</name>
        <uri>https://orcid.org/0000-0002-4445-5096</uri>
      </author>
      <author>
        <name>Yokoyama, Tetsuya</name>
      </author>
      <author>
        <name>Yoneda, Shigekazu</name>
      </author>
      <author>
        <name>Young, Edward D</name>
        <uri>https://orcid.org/0000-0002-1299-0801</uri>
      </author>
      <author>
        <name>Yui, Hiroharu</name>
      </author>
      <author>
        <name>Zhang, Ai-Cheng</name>
      </author>
      <author>
        <name>Nakamura, Tomoki</name>
      </author>
      <author>
        <name>Naraoka, Hiroshi</name>
      </author>
      <author>
        <name>Okazaki, Ryuji</name>
      </author>
      <author>
        <name>Sakamoto, Kanako</name>
      </author>
      <author>
        <name>Yabuta, Hikaru</name>
      </author>
      <author>
        <name>Abe, Masanao</name>
      </author>
      <author>
        <name>Miyazaki, Akiko</name>
      </author>
      <author>
        <name>Nakato, Aiko</name>
      </author>
      <author>
        <name>Nishimura, Masahiro</name>
      </author>
      <author>
        <name>Okada, Tatsuaki</name>
      </author>
      <author>
        <name>Yada, Toru</name>
      </author>
      <author>
        <name>Yogata, Kasumi</name>
      </author>
      <author>
        <name>Nakazawa, Satoru</name>
      </author>
      <author>
        <name>Saiki, Takanao</name>
      </author>
      <author>
        <name>Tanaka, Satoshi</name>
      </author>
      <author>
        <name>Terui, Fuyuto</name>
      </author>
      <author>
        <name>Tsuda, Yuichi</name>
      </author>
      <author>
        <name>Watanabe, Sei-ichiro</name>
      </author>
      <author>
        <name>Yoshikawa, Makoto</name>
      </author>
      <author>
        <name>Tachibana, Shogo</name>
      </author>
      <author>
        <name>Yurimoto, Hisayoshi</name>
      </author>
    </item>
    <item>
      <title>Systemic racial disparities in funding rates at the National Science Foundation</title>
      <link>https://escholarship.org/uc/item/0cs6n74d</link>
      <description>Concerns about systemic racism at academic and research institutions have increased over the past decade. Here, we investigate data from the National Science Foundation (NSF), a major funder of research in the United States, and find evidence for pervasive racial disparities. In particular, white principal investigators (PIs) are consistently funded at higher rates than most non-white PIs. Funding rates for white PIs have also been increasing relative to annual overall rates with time. Moreover, disparities occur across all disciplinary directorates within the NSF and are greater for research proposals. The distributions of average external review scores also exhibit systematic offsets based on PI race. Similar patterns have been described in other research funding bodies, suggesting that racial disparities are widespread. The prevalence and persistence of these racial disparities in funding have cascading impacts that perpetuate a cumulative advantage to white PIs across all...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0cs6n74d</guid>
      <pubDate>Sat, 8 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Chen, Christine Yifeng</name>
      </author>
      <author>
        <name>Kahanamoku, Sara S</name>
      </author>
      <author>
        <name>Tripati, Aradhna</name>
        <uri>https://orcid.org/0000-0002-1695-1754</uri>
      </author>
      <author>
        <name>Alegado, Rosanna A</name>
      </author>
      <author>
        <name>Morris, Vernon R</name>
      </author>
      <author>
        <name>Andrade, Karen</name>
      </author>
      <author>
        <name>Hosbey, Justin</name>
      </author>
    </item>
    <item>
      <title>Plasmapause surface wave oscillates the magnetosphere and diffuse aurora</title>
      <link>https://escholarship.org/uc/item/1jf2t0xj</link>
      <description>Energy circulation in geospace lies at the heart of space weather research. In the inner magnetosphere, the steep plasmapause boundary separates the cold dense plasmasphere, which corotates with the planet, from the hot ring current/plasma sheet outside. Theoretical studies suggested that plasmapause surface waves related to the sharp inhomogeneity exist and act as a source of geomagnetic pulsations, but direct evidence of the waves and their role in magnetospheric dynamics have not yet been detected. Here, we show direct observations of a plasmapause surface wave and its impacts during a geomagnetic storm using multi-satellite and ground-based measurements. The wave oscillates the plasmapause in the afternoon-dusk sector, triggers sawtooth auroral displays, and drives outward-propagating ultra-low frequency waves. We also show that the surface-wave-driven sawtooth auroras occurred in more than 90% of geomagnetic storms during 2014–2018, indicating that they are a systematic and...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1jf2t0xj</guid>
      <pubDate>Fri, 7 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>He, Fei</name>
      </author>
      <author>
        <name>Guo, Rui-Long</name>
      </author>
      <author>
        <name>Dunn, William R</name>
      </author>
      <author>
        <name>Yao, Zhong-Hua</name>
      </author>
      <author>
        <name>Zhang, Hua-Sen</name>
      </author>
      <author>
        <name>Hao, Yi-Xin</name>
      </author>
      <author>
        <name>Shi, Quan-Qi</name>
      </author>
      <author>
        <name>Rong, Zhao-Jin</name>
      </author>
      <author>
        <name>Liu, Jiang</name>
        <uri>https://orcid.org/0000-0002-7489-9384</uri>
      </author>
      <author>
        <name>Tian, An-Min</name>
      </author>
      <author>
        <name>Zhang, Xiao-Xin</name>
      </author>
      <author>
        <name>Wei, Yong</name>
      </author>
      <author>
        <name>Zhang, Yong-Liang</name>
      </author>
      <author>
        <name>Zong, Qiu-Gang</name>
      </author>
      <author>
        <name>Pu, Zu-Yin</name>
      </author>
      <author>
        <name>Wan, Wei-Xing</name>
      </author>
    </item>
    <item>
      <title>Genetic structure and historic demography of endangered unarmoured threespine stickleback at southern latitudes signals a potential new management approach</title>
      <link>https://escholarship.org/uc/item/7g66w6p5</link>
      <description>Habitat loss, flood control infrastructure, and drought have left most of southern California and northern Baja California's native freshwater fish near extinction, including the endangered unarmoured threespine stickleback (Gasterosteus aculeatus williamsoni). This subspecies, an unusual morph lacking the typical lateral bony plates of the G. aculeatus complex, occurs at arid southern latitudes in the eastern Pacific Ocean and survives in only three inland locations. Managers have lacked molecular data to answer basic questions about the ancestry and genetic distinctiveness of unarmoured populations. These data could be used to prioritize conservation efforts. We sampled G. aculeatus from 36 localities and used microsatellites and whole genome data to place unarmoured populations within the broader evolutionary context of G. aculeatus across southern California/northern Baja California. We identified three genetic groups with none consisting solely of unarmoured populations....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7g66w6p5</guid>
      <pubDate>Thu, 6 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Turba, Rachel</name>
      </author>
      <author>
        <name>Richmond, Jonathan Q</name>
      </author>
      <author>
        <name>Fitz‐Gibbon, Sorel</name>
      </author>
      <author>
        <name>Morselli, Marco</name>
      </author>
      <author>
        <name>Fisher, Robert N</name>
      </author>
      <author>
        <name>Swift, Camm C</name>
      </author>
      <author>
        <name>Ruiz‐Campos, Gorgonio</name>
      </author>
      <author>
        <name>Backlin, Adam R</name>
      </author>
      <author>
        <name>Dellith, Chris</name>
      </author>
      <author>
        <name>Jacobs, David K</name>
        <uri>https://orcid.org/0000-0002-7252-1601</uri>
      </author>
    </item>
    <item>
      <title>Geospace Concussion: Global Reversal of Ionospheric Vertical Plasma Drift in Response to a Sudden Commencement</title>
      <link>https://escholarship.org/uc/item/0h20c2kw</link>
      <description>An interplanetary shock can abruptly compress the magnetosphere, excite magnetospheric waves and field-aligned currents, and cause a ground magnetic response known as a sudden commencement (SC). However, the transient (&amp;lt;∼1&amp;nbsp;min) response of the ionosphere-thermosphere system during an SC has been little studied due to limited temporal resolution in previous investigations. Here, we report observations of a global reversal of ionospheric vertical plasma motion during an SC on 24 October 2011 using ∼6&amp;nbsp;s resolution Super Dual Auroral Radar Network ground scatter data. The dayside ionosphere suddenly moved downward during the magnetospheric compression due to the SC, lasting for only ∼1&amp;nbsp;min before moving upward. By contrast, the post-midnight ionosphere briefly moved upward then moved downward during the SC. Simulations with a coupled geospace model suggest that the reversed  vertical drift is caused by a global reversal of ionospheric zonal electric field induced...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0h20c2kw</guid>
      <pubDate>Thu, 6 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Shi, Xueling</name>
      </author>
      <author>
        <name>Lin, Dong</name>
      </author>
      <author>
        <name>Wang, Wenbin</name>
      </author>
      <author>
        <name>Baker, Joseph BH</name>
      </author>
      <author>
        <name>Weygand, James M</name>
        <uri>https://orcid.org/0000-0001-7996-2277</uri>
      </author>
      <author>
        <name>Hartinger, Michael D</name>
      </author>
      <author>
        <name>Merkin, Viacheslav G</name>
      </author>
      <author>
        <name>Ruohoniemi, J Michael</name>
      </author>
      <author>
        <name>Pham, Kevin</name>
      </author>
      <author>
        <name>Wu, Haonan</name>
      </author>
      <author>
        <name>Angelopoulos, Vassilis</name>
        <uri>https://orcid.org/0000-0001-7024-1561</uri>
      </author>
      <author>
        <name>McWilliams, Kathryn A</name>
      </author>
      <author>
        <name>Nishitani, Nozomu</name>
      </author>
      <author>
        <name>Shepherd, Simon G</name>
      </author>
    </item>
    <item>
      <title>Community voices: Achieving real diversity in STEM requires the ability to transform institutions</title>
      <link>https://escholarship.org/uc/item/773250g2</link>
      <description>Resilience is often invoked to address systemic marginalization (e.g. racism) in academia but inadvertently maintains harmful systems. We argue that the ability to transform systems, as opposed to persevering within them, must be prioritized to make real, lasting change.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/773250g2</guid>
      <pubDate>Thu, 29 Jun 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Lerback, Jory C</name>
      </author>
      <author>
        <name>Holt, Monique M</name>
      </author>
      <author>
        <name>St. Pierre, Gabriela A Enriquez</name>
      </author>
      <author>
        <name>Putman, Annie</name>
      </author>
      <author>
        <name>Tulley-Cordova, Crystal L</name>
      </author>
      <author>
        <name>Smith, William A</name>
      </author>
      <author>
        <name>Caughman, Liliana</name>
      </author>
      <author>
        <name>Alvarez, Stephanie</name>
      </author>
    </item>
    <item>
      <title>Effects of Subauroral Polarization Streams on the Upper Thermospheric Winds During Non‐Storm Time</title>
      <link>https://escholarship.org/uc/item/3782r787</link>
      <description>Intense sunward (westward) plasma flows, named Subauroral Polarization Stream (SAPS), have been known to occur equatorward of the electron auroras for decades, yet their effect on the upper thermosphere has not been well understood. On the one hand, the large velocity of SAPS results in large momentum exchange upon each ion-neutral collision. On the other hand, the low plasma density associated with SAPS implies a low ion-neutral collision frequency. We investigate the SAPS effect during non-storm time by utilizing a Scanning Doppler Imager (SDI) for monitoring the upper thermosphere, SuperDARN radars for SAPS, all-sky imagers and DMSP Spectrographic Imager for the auroral oval, and GPS receivers for the total electron content. Our observations suggest that SAPS at times drives substantial (&amp;gt;50&amp;nbsp;m/s) westward winds at subauroral latitudes in the dusk-midnight sector, but not always. The occurrence of the westward winds varies with &lt;i&gt;AE&lt;/i&gt; index, plasma content in the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3782r787</guid>
      <pubDate>Thu, 29 Jun 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Zou, Ying</name>
      </author>
      <author>
        <name>Lyons, Larry R</name>
      </author>
      <author>
        <name>Shi, Xueling</name>
      </author>
      <author>
        <name>Liu, Jiang</name>
        <uri>https://orcid.org/0000-0002-7489-9384</uri>
      </author>
      <author>
        <name>Wu, Qian</name>
      </author>
      <author>
        <name>Conde, Mark</name>
      </author>
      <author>
        <name>Shepherd, Simon G</name>
      </author>
      <author>
        <name>Mende, Stephen</name>
      </author>
      <author>
        <name>Zhang, Yongliang</name>
      </author>
      <author>
        <name>Coster, Antea</name>
      </author>
    </item>
    <item>
      <title>Parker Solar Probe Observations of Solar Wind Energetic Proton Beams Produced by Magnetic Reconnection in the Near‐Sun Heliospheric Current Sheet</title>
      <link>https://escholarship.org/uc/item/30x93024</link>
      <description>We report observations of reconnection exhausts in the Heliospheric Current Sheet (HCS) during Parker Solar Probe Encounters 08 and 07, at 16 &lt;i&gt;R&lt;/i&gt; &lt;sub&gt;&lt;i&gt;s&lt;/i&gt;&lt;/sub&gt; and 20 &lt;i&gt;R&lt;/i&gt; &lt;sub&gt;&lt;i&gt;s&lt;/i&gt;&lt;/sub&gt; , respectively. Heliospheric current sheet (HCS) reconnection accelerated protons to almost twice the solar wind speed and increased the proton core energy by a factor of ∼3, due to the Alfvén speed being comparable to the solar wind flow speed at these near-Sun distances. Furthermore, protons were energized to super-thermal energies. During E08, energized protons were found to have leaked out of the exhaust along separatrix field lines, appearing as field-aligned energetic proton beams in a broad region outside the HCS. Concurrent dropouts of strahl electrons, indicating disconnection from the Sun, provide further evidence for the HCS being the source of the beams. Around the HCS in E07, there were also proton beams but without electron strahl dropouts, indicating that their...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/30x93024</guid>
      <pubDate>Thu, 29 Jun 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Phan, TD</name>
      </author>
      <author>
        <name>Verniero, JL</name>
      </author>
      <author>
        <name>Larson, D</name>
      </author>
      <author>
        <name>Lavraud, B</name>
      </author>
      <author>
        <name>Drake, JF</name>
      </author>
      <author>
        <name>Øieroset, M</name>
      </author>
      <author>
        <name>Eastwood, JP</name>
      </author>
      <author>
        <name>Bale, SD</name>
        <uri>https://orcid.org/0000-0002-1989-3596</uri>
      </author>
      <author>
        <name>Livi, R</name>
      </author>
      <author>
        <name>Halekas, JS</name>
      </author>
      <author>
        <name>Whittlesey, PL</name>
      </author>
      <author>
        <name>Rahmati, A</name>
      </author>
      <author>
        <name>Stansby, D</name>
      </author>
      <author>
        <name>Pulupa, M</name>
      </author>
      <author>
        <name>MacDowall, RJ</name>
      </author>
      <author>
        <name>Szabo, PA</name>
      </author>
      <author>
        <name>Koval, A</name>
      </author>
      <author>
        <name>Desai, M</name>
      </author>
      <author>
        <name>Fuselier, SA</name>
      </author>
      <author>
        <name>Velli, M</name>
        <uri>https://orcid.org/0000-0002-2381-3106</uri>
      </author>
      <author>
        <name>Hesse, M</name>
      </author>
      <author>
        <name>Pyakurel, PS</name>
      </author>
      <author>
        <name>Maheshwari, K</name>
      </author>
      <author>
        <name>Kasper, JC</name>
      </author>
      <author>
        <name>Stevens, JM</name>
      </author>
      <author>
        <name>Case, AW</name>
      </author>
      <author>
        <name>Raouafi, NE</name>
      </author>
    </item>
    <item>
      <title>Mitochondrial genome copy number measured by DNA sequencing in human blood is strongly associated with metabolic traits via cell-type composition differences</title>
      <link>https://escholarship.org/uc/item/723919sn</link>
      <description>BackgroundMitochondrial genome copy number (MT-CN) varies among humans and across tissues and is highly heritable, but its causes and consequences are not well understood. When measured by bulk DNA sequencing in blood, MT-CN may reflect a combination of the number of mitochondria per cell and cell-type composition. Here, we studied MT-CN variation in blood-derived DNA from 19184 Finnish individuals using a combination of genome (N = 4163) and exome sequencing (N = 19034) data as well as imputed genotypes (N = 17718).ResultsWe identified two loci significantly associated with MT-CN variation: a common variant at the MYB-HBS1L locus (P = 1.6 × 10−8), which has previously been associated with numerous hematological parameters; and a burden of rare variants in the TMBIM1 gene (P = 3.0 × 10−8), which has been reported to protect against non-alcoholic fatty liver disease. We also found that MT-CN is strongly associated with insulin levels (P = 2.0 × 10−21) and other metabolic syndrome...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/723919sn</guid>
      <pubDate>Wed, 21 Jun 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Ganel, Liron</name>
      </author>
      <author>
        <name>Chen, Lei</name>
      </author>
      <author>
        <name>Christ, Ryan</name>
      </author>
      <author>
        <name>Vangipurapu, Jagadish</name>
      </author>
      <author>
        <name>Young, Erica</name>
        <uri>https://orcid.org/0000-0002-1299-0801</uri>
      </author>
      <author>
        <name>Das, Indraniel</name>
      </author>
      <author>
        <name>Kanchi, Krishna</name>
      </author>
      <author>
        <name>Larson, David</name>
      </author>
      <author>
        <name>Regier, Allison</name>
      </author>
      <author>
        <name>Abel, Haley</name>
      </author>
      <author>
        <name>Kang, Chul Joo</name>
      </author>
      <author>
        <name>Scott, Alexandra</name>
      </author>
      <author>
        <name>Havulinna, Aki</name>
      </author>
      <author>
        <name>Chiang, Charleston WK</name>
      </author>
      <author>
        <name>Service, Susan</name>
      </author>
      <author>
        <name>Freimer, Nelson</name>
        <uri>https://orcid.org/0000-0003-3586-6587</uri>
      </author>
      <author>
        <name>Palotie, Aarno</name>
      </author>
      <author>
        <name>Ripatti, Samuli</name>
      </author>
      <author>
        <name>Kuusisto, Johanna</name>
      </author>
      <author>
        <name>Boehnke, Michael</name>
      </author>
      <author>
        <name>Laakso, Markku</name>
      </author>
      <author>
        <name>Locke, Adam</name>
      </author>
      <author>
        <name>Stitziel, Nathan O</name>
      </author>
      <author>
        <name>Hall, Ira M</name>
      </author>
    </item>
    <item>
      <title>Patterns of Element Incorporation in Calcium Carbonate Biominerals Recapitulate Phylogeny for a Diverse Range of Marine Calcifiers</title>
      <link>https://escholarship.org/uc/item/5tm227wk</link>
      <description>Elemental ratios in biogenic marine calcium carbonates are widely used in geobiology, environmental science, and paleoenvironmental reconstructions. It is generally accepted that the elemental abundance of biogenic marine carbonates reflects a combination of the abundance of that ion in seawater, the physical properties of seawater, the mineralogy of the biomineral, and the pathways and mechanisms of biomineralization. Here we report measurements of a suite of nine elemental ratios (Li/Ca, B/Ca, Na/Ca, Mg/Ca, Zn/Ca, Sr/Ca, Cd/Ca, Ba/Ca, and U/Ca) in 18 species of benthic marine invertebrates spanning a range of biogenic carbonate polymorph mineralogies (low-Mg calcite, high-Mg calcite, aragonite, mixed mineralogy) and of phyla (including Mollusca, Echinodermata, Arthropoda, Annelida, Cnidaria, Chlorophyta, and Rhodophyta) cultured at a single temperature (25°C) and a range of &lt;i&gt;p&lt;/i&gt;CO&lt;sub&gt;2&lt;/sub&gt; treatments (ca. 409, 606, 903, and 2856 ppm). This dataset was used to explore...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5tm227wk</guid>
      <pubDate>Wed, 21 Jun 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Ulrich, Robert N</name>
      </author>
      <author>
        <name>Guillermic, Maxence</name>
      </author>
      <author>
        <name>Campbell, Julia</name>
      </author>
      <author>
        <name>Hakim, Abbas</name>
      </author>
      <author>
        <name>Han, Rachel</name>
      </author>
      <author>
        <name>Singh, Shayleen</name>
      </author>
      <author>
        <name>Stewart, Justin D</name>
      </author>
      <author>
        <name>Román-Palacios, Cristian</name>
      </author>
      <author>
        <name>Carroll, Hannah M</name>
      </author>
      <author>
        <name>De Corte, Ilian</name>
      </author>
      <author>
        <name>Gilmore, Rosaleen E</name>
      </author>
      <author>
        <name>Doss, Whitney</name>
      </author>
      <author>
        <name>Tripati, Aradhna</name>
        <uri>https://orcid.org/0000-0002-1695-1754</uri>
      </author>
      <author>
        <name>Ries, Justin B</name>
      </author>
      <author>
        <name>Eagle, Robert A</name>
      </author>
    </item>
    <item>
      <title>Chromium Isotopic Evidence for Mixing of NC and CC Reservoirs in Polymict Ureilites: Implications for Dynamical Models of the Early Solar System</title>
      <link>https://escholarship.org/uc/item/5ds4s34w</link>
      <description>Nucleosynthetic isotope anomalies show that the first few million years of solar system history were characterized by two distinct cosmochemical reservoirs, CC (carbonaceous chondrites and related differentiated meteorites) and NC (the terrestrial planets and all other groups of chondrites and differentiated meteorites), widely interpreted to correspond to the outer and inner solar system, respectively. At some point, however, bulk CC and NC materials became mixed, and several dynamical models offer explanations for how and when this occurred. We use xenoliths of CC materials in polymict ureilite (NC) breccias to test the applicability of such models. Polymict ureilites represent regolith on ureilitic asteroids but contain carbonaceous chondrite-like xenoliths. We present the first &lt;sup&gt;54&lt;/sup&gt;Cr isotope data for such clasts, which, combined with oxygen and hydrogen isotopes, show that they are unique CC materials that became mixed with NC materials in these breccias. It has...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5ds4s34w</guid>
      <pubDate>Sat, 17 Jun 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Goodrich, Cyrena A</name>
      </author>
      <author>
        <name>Sanborn, Matthew E</name>
      </author>
      <author>
        <name>Yin, Qing-Zhu</name>
        <uri>https://orcid.org/0000-0002-4445-5096</uri>
      </author>
      <author>
        <name>Kohl, Issaku</name>
      </author>
      <author>
        <name>Frank, David</name>
      </author>
      <author>
        <name>Daly, R Terik</name>
      </author>
      <author>
        <name>Walsh, Kevin J</name>
      </author>
      <author>
        <name>Zolensky, Michael E</name>
      </author>
      <author>
        <name>Young, Edward RD</name>
        <uri>https://orcid.org/0000-0002-1299-0801</uri>
      </author>
      <author>
        <name>Jenniskens, Peter</name>
      </author>
      <author>
        <name>Shaddad, Muawia H</name>
      </author>
    </item>
    <item>
      <title>Constraining crustal silica on ancient Earth</title>
      <link>https://escholarship.org/uc/item/8vp0490q</link>
      <description>Accurately quantifying the composition of continental crust on Hadean and Archean Earth is critical to our understanding of the physiography, tectonics, and climate of our planet at the dawn of life. One longstanding paradigm involves the growth of a relatively mafic planetary crust over the first 1 to 2 billion years of Earth history, implying a lack of modern plate tectonics and a paucity of subaerial crust, and consequently lacking an efficient mechanism to regulate climate. Others have proposed a more uniformitarian view in which Archean and Hadean continents were only slightly more mafic than at present. Apart from complications in assessing early crustal composition introduced by crustal preservation and sampling biases, effects such as the secular cooling of Earth's mantle and the biologically driven oxidation of Earth's atmosphere have not been fully investigated. We find that the former complicates efforts to infer crustal silica from compatible or incompatible element...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8vp0490q</guid>
      <pubDate>Mon, 12 Jun 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Keller, C Brenhin</name>
      </author>
      <author>
        <name>Harrison, T Mark</name>
      </author>
    </item>
    <item>
      <title>Reversibility controls on extreme methane clumped isotope signatures from anaerobic oxidation of methane</title>
      <link>https://escholarship.org/uc/item/9c3465pm</link>
      <description>Reversibility controls on extreme methane clumped isotope signatures from anaerobic oxidation of methane</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9c3465pm</guid>
      <pubDate>Wed, 7 Jun 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Liu, Jiarui</name>
      </author>
      <author>
        <name>Harris, Rachel L</name>
      </author>
      <author>
        <name>Ash, Jeanine L</name>
      </author>
      <author>
        <name>Ferry, James G</name>
      </author>
      <author>
        <name>Krause, Sebastian JE</name>
      </author>
      <author>
        <name>Labidi, Jabrane</name>
      </author>
      <author>
        <name>Prakash, Divya</name>
      </author>
      <author>
        <name>Lollar, Barbara Sherwood</name>
      </author>
      <author>
        <name>Treude, Tina</name>
      </author>
      <author>
        <name>Warr, Oliver</name>
      </author>
      <author>
        <name>Young, Edward D</name>
      </author>
    </item>
    <item>
      <title>First Detection of the Powerful Gamma-Ray Burst GRB 221009A by the THEMIS ESA and SST Particle Detectors on 2022 October 9</title>
      <link>https://escholarship.org/uc/item/70r8f1vb</link>
      <description>We present the first results study of the effects of the powerful gamma-ray burst GRB 221009A that occurred on 2022 October 9, and was serendipitously recorded by electron and proton detectors on board the four spacecraft of the NASA THEMIS mission. Long-duration gamma-ray bursts (GRBs) are powerful cosmic explosions, signaling the death of massive stars, and, among them, GRB 221009A is so far the brightest burst ever observed due to its enormous energy (E γ iso ≈ 1055 erg) and proximity (the redshift is z ≈ 0.1505). The THEMIS mission launched in 2008 was designed to study the plasma processes in the Earth’s magnetosphere and the solar wind. The particle flux measurements from the two inner magnetosphere THEMIS probes, THA and THE, and two outer probes (renamed ARTEMIS after 2010), THB and THC, orbiting the Moon captured the dynamics of GRB 221009A with a high time resolution of 4 (up to 8) measurements per second. This allowed us to resolve the fine structure of the GRB and...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/70r8f1vb</guid>
      <pubDate>Wed, 7 Jun 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Agapitov, OV</name>
      </author>
      <author>
        <name>Balikhin, M</name>
      </author>
      <author>
        <name>Hull, AJ</name>
      </author>
      <author>
        <name>Hobara, Y</name>
      </author>
      <author>
        <name>Angelopoulos, V</name>
        <uri>https://orcid.org/0000-0001-7024-1561</uri>
      </author>
      <author>
        <name>Mozer, FS</name>
      </author>
    </item>
    <item>
      <title>Near-equilibrium isotope fractionation during planetesimal evaporation</title>
      <link>https://escholarship.org/uc/item/4m96n098</link>
      <description>Silicon and Mg in differentiated rocky bodies exhibit heavy isotope enrichments that have been attributed to evaporation of partially or entirely molten planetesimals. We evaluate the mechanisms of planetesimal evaporation in the early solar system and the conditions that controled attendant isotope fractionations. Energy balance at the surface of a body accreted within ~1 Myr of CAI formation and heated from within by &lt;sup&gt;26&lt;/sup&gt;Al decay results in internal temperatures exceeding the silicate solidus, producing a transient magma ocean with a thin surface boundary layer of order &amp;lt; 1 meter that would be subject to foundering. Bodies that are massive enough to form magma oceans by radioisotope decay (≥ 0.1% &lt;i&gt;M&lt;/i&gt; &lt;sub&gt;⊕&lt;/sub&gt;) can retain hot rock vapor even in the absence of ambient nebular gas. We find that a steady-state rock vapor forms within minutes to hours and results from a balance between rates of magma evaporation and atmospheric escape. Vapor pressure buildup...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4m96n098</guid>
      <pubDate>Fri, 26 May 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Young, ED</name>
        <uri>https://orcid.org/0000-0002-1299-0801</uri>
      </author>
      <author>
        <name>Shahar, A</name>
      </author>
      <author>
        <name>Nimmo, F</name>
      </author>
      <author>
        <name>Schlichting, HE</name>
        <uri>https://orcid.org/0000-0002-0298-8089</uri>
      </author>
      <author>
        <name>Schauble, EA</name>
        <uri>https://orcid.org/0000-0002-1266-1282</uri>
      </author>
      <author>
        <name>Tang, H</name>
      </author>
      <author>
        <name>Labidi, J</name>
      </author>
    </item>
    <item>
      <title>Effectiveness of vegetation and sound wall-vegetation combination barriers on pollution dispersion from freeways under early morning conditions</title>
      <link>https://escholarship.org/uc/item/8fh9p9ps</link>
      <description>Pollutants in tailpipe emissions can be highly elevated around roadways, and in early mornings the pollution plume can extend hundreds of meters into surrounding neighborhoods. Solid sound walls and vegetation barriers are commonly used to mitigate noise, but they also help mitigate near-road air pollution. Here we assess the effectiveness of barriers consisting of vegetation only and of a combination of vegetation and a solid sound wall (combination barrier) in reducing pollution concentrations downwind of roads, under stable atmospheric stability and calm to light wind conditions. Because there was no practical (no barrier) control site in the area, we primarily compare the two barrier types to each other and explore the importance of atmospheric conditions. Using measurements collected with a mobile platform, we develop concentration decay profiles of ultrafine and fine particles, oxides of nitrogen (NO and NO&lt;sub&gt;2&lt;/sub&gt;) and carbon monoxide downwind of a freeway in California...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8fh9p9ps</guid>
      <pubDate>Thu, 25 May 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Ranasinghe, Dilhara</name>
      </author>
      <author>
        <name>Lee, Eon S</name>
      </author>
      <author>
        <name>Zhu, Yifang</name>
        <uri>https://orcid.org/0000-0002-0591-3322</uri>
      </author>
      <author>
        <name>Frausto-Vicencio, Isis</name>
      </author>
      <author>
        <name>Choi, Wonsik</name>
      </author>
      <author>
        <name>Sun, Wu</name>
      </author>
      <author>
        <name>Mara, Steve</name>
      </author>
      <author>
        <name>Seibt, Ulrike</name>
      </author>
      <author>
        <name>Paulson, Suzanne E</name>
        <uri>https://orcid.org/0000-0003-0855-7615</uri>
      </author>
    </item>
    <item>
      <title>Mechanisms of cnidocyte development in the moon jellyfish Aurelia</title>
      <link>https://escholarship.org/uc/item/2ms347n2</link>
      <description>Stinging cells called cnidocytes are a defining trait of the cnidarians (sea anemones, corals, jellyfish, and their relatives). In hydrozoan cnidarians such as Hydra, cnidocytes develop from interstitial stem cells set aside in the ectoderm. It is less clear how cnidocytes develop outside the Hydrozoa, as other cnidarians appear to lack interstitial stem cells. We addressed this question by studying cnidogenesis in the moon jellyfish (Aurelia) through the visualization of minicollagen-a protein associated with cnidocyte development-as well as transmission electron microscopy. We discovered that developing cnidoblasts are rare or absent in feeding structures rich in mature cnidocytes, such as tentacles and lappets. Using transmission electron microscopy, we determined that the progenitors of cnidocytes have traits consistent with epitheliomuscular cells. Our data suggests a dynamic where cnidocytes develop at high concentrations in the epithelium of more proximal regions, and subsequently...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2ms347n2</guid>
      <pubDate>Thu, 25 May 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Gold, David A</name>
        <uri>https://orcid.org/0000-0003-0135-4022</uri>
      </author>
      <author>
        <name>Lau, Clive Long Fung</name>
      </author>
      <author>
        <name>Fuong, Holly</name>
      </author>
      <author>
        <name>Kao, Gregory</name>
      </author>
      <author>
        <name>Hartenstein, Volker</name>
      </author>
      <author>
        <name>Jacobs, David K</name>
        <uri>https://orcid.org/0000-0002-7252-1601</uri>
      </author>
    </item>
    <item>
      <title>Long‐Lasting Poloidal ULF Waves Observed by Multiple Satellites and High‐Latitude SuperDARN Radars</title>
      <link>https://escholarship.org/uc/item/0td3h2gf</link>
      <description>Poloidal ultra-low frequency (ULF) waves between 5-10 mHz were observed by multiple satellites and three high-latitude Super Dual Auroral Radar Network (SuperDARN) radars during the recovery phase of a moderate geomagnetic storm on Jan 24-27, 2016. The long-lasting ULF waves were observed in the magnetic field and energetic particle flux perturbations during three successive passes by two Geostationary Operational Environmental Satellites (GOES) through the dayside magnetosphere, during which plasmasphere expansion and refilling were observed by two Time History of Events and Macroscale Interactions during Substorms (THEMIS) probes. The radial magnetic field oscillation was in phase (~ 180° out of phase) with the northward (southward) moving proton flux oscillation at 95 keV, consistent with high-energy drift-bounce resonance signatures of protons with second harmonic poloidal standing Alfvén waves. The longitudinal extent of the waves approached 10 hours in local time on the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0td3h2gf</guid>
      <pubDate>Wed, 24 May 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Shi, X</name>
      </author>
      <author>
        <name>Baker, JBH</name>
      </author>
      <author>
        <name>Ruohoniemi, JM</name>
      </author>
      <author>
        <name>Hartinger, MD</name>
      </author>
      <author>
        <name>Murphy, KR</name>
      </author>
      <author>
        <name>Rodriguez, JV</name>
      </author>
      <author>
        <name>Nishimura, Y</name>
      </author>
      <author>
        <name>McWilliams, KA</name>
      </author>
      <author>
        <name>Angelopoulos, V</name>
        <uri>https://orcid.org/0000-0001-7024-1561</uri>
      </author>
    </item>
    <item>
      <title>Direct evidence of surface exposed water ice in the lunar polar regions</title>
      <link>https://escholarship.org/uc/item/2s7392x8</link>
      <description>Water ice may be allowed to accumulate in permanently shaded regions on airless bodies in the inner solar system such as Mercury, the Moon, and Ceres [Watson K, et al. (1961) &lt;i&gt;J Geophys Res&lt;/i&gt; 66:3033-3045]. Unlike Mercury and Ceres, direct evidence for water ice exposed at the lunar surface has remained elusive. We utilize indirect lighting in regions of permanent shadow to report the detection of diagnostic near-infrared absorption features of water ice in reflectance spectra acquired by the Moon Mineralogy Mapper [M (3)] instrument. Several thousand M (3) pixels (∼280 × 280 m) with signatures of water ice at the optical surface (depth of less than a few millimeters) are identified within 20° latitude of both poles, including locations where independent measurements have suggested that water ice may be present. Most ice locations detected in M (3) data also exhibit lunar orbiter laser altimeter reflectance values and Lyman Alpha Mapping Project instrument UV ratio values...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2s7392x8</guid>
      <pubDate>Tue, 23 May 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Li, Shuai</name>
      </author>
      <author>
        <name>Lucey, Paul G</name>
      </author>
      <author>
        <name>Milliken, Ralph E</name>
      </author>
      <author>
        <name>Hayne, Paul O</name>
      </author>
      <author>
        <name>Fisher, Elizabeth</name>
      </author>
      <author>
        <name>Williams, Jean-Pierre</name>
        <uri>https://orcid.org/0000-0003-4163-2760</uri>
      </author>
      <author>
        <name>Hurley, Dana M</name>
      </author>
      <author>
        <name>Elphic, Richard C</name>
      </author>
    </item>
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