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    <title>Recent ucb_eps items</title>
    <link>https://escholarship.org/uc/ucb_eps/rss</link>
    <description>Recent eScholarship items from Department of Earth and Planetary Science</description>
    <pubDate>Wed, 17 Jun 2026 15:03:50 +0000</pubDate>
    <item>
      <title>Compound Mesoscale Convective Systems and Low‐Pressure Systems in Tropical Monsoon Regions: Assessing Their Meteorology and Precipitation</title>
      <link>https://escholarship.org/uc/item/3m7897db</link>
      <description>Abstract Mesoscale convective systems (MCS) and low‐pressure systems (LPS) are both strongly associated with precipitation across the regions where they occur, particularly within global monsoon systems; however, their co‐occurrence and its relationship to precipitation have not been systematically examined. Here, we use LPS and MCS trackers to detect compound MCS and LPS events in five monsoon regions and assess the association of this co‐occurrence with anomalies of winds, precipitation, and other atmospheric variables. Additionally, we investigate the spatial distribution of precipitating MCS and LPS events. Our results show that most (∼60%) MCS and LPS co‐occurrences are located in the lower latitudes, where they contribute up to 40% of annual precipitation. We find that compound events generally produce more extreme precipitation than MCS‐only or LPS‐only events. Furthermore, our assessment of the synoptic and mesoscale composites reveals that the underlying dynamics of compound...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3m7897db</guid>
      <pubDate>Wed, 10 Jun 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Quagraine, Kwesi Twentwewa</name>
      </author>
      <author>
        <name>O’Brien, Travis A</name>
      </author>
      <author>
        <name>Boos, William</name>
        <uri>https://orcid.org/0000-0001-9076-3551</uri>
      </author>
      <author>
        <name>Neelin, J David</name>
      </author>
      <author>
        <name>Tsai, Wei‐Ming</name>
      </author>
      <author>
        <name>Leung, L Ruby</name>
      </author>
      <author>
        <name>Ullrich, Paul A</name>
        <uri>https://orcid.org/0000-0003-4118-4590</uri>
      </author>
      <author>
        <name>Ahmed, Fiaz</name>
      </author>
    </item>
    <item>
      <title>Elongated sandstone concretions record river system evolution across the Cretaceous-Paleogene boundary, Montana, USA</title>
      <link>https://escholarship.org/uc/item/9220730s</link>
      <description>Abstract The Cretaceous–Paleogene (K-Pg) extinction caused significant environmental upheaval, including the disappearance of non-avian dinosaurs and widespread disruption of ecosystems. The Hell Creek and Fort Union formations in the upper Great Plains of North America preserve a record of environmental change across the K-Pg boundary (KPB). Sedimentological studies suggest that the Hell Creek Formation represents a well-drained floodplain, with increased standing water leading to the formation of ponds and peat bogs close to the KPB. This shift has been attributed to the disruption of river systems by short-term extinction-driven flooding in the Western Interior. To test this, we analyze ~2900 paleocurrent measurements from elongate concretions mapped over ~5000 km2 in the Hell Creek area of eastern Montana, USA. These measurements, combined with previously published chronostratigraphic constraints, allow us to trace river system evolution over time. Paleocurrents shift from...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9220730s</guid>
      <pubDate>Wed, 3 Jun 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Hasler, Caroline EJ</name>
      </author>
      <author>
        <name>Renne, Paul R</name>
      </author>
    </item>
    <item>
      <title>Zircon Constraints on the Eruptive Sequence and Magma Evolution of Rhyolites at South Sister Volcano, Oregon</title>
      <link>https://escholarship.org/uc/item/6628x1m2</link>
      <description>Abstract  We present 230 Th‐ 238 U crystallization ages and trace element compositions for zircons spanning the late Pleistocene to Holocene rhyolite eruptive record at South Sister volcano in the central Oregon Cascade Range. Most zircon ages are between 100 and 20&amp;nbsp;ka, with very few in secular equilibrium (&amp;gt;350&amp;nbsp;ka). The weighted mean of zircon ages for the two oldest South Sister rhyolites, 31.5&amp;nbsp;±&amp;nbsp;2.1 and 39.1&amp;nbsp;±&amp;nbsp;2.4&amp;nbsp;ka, are significantly younger than the associated 40 Ar/ 39 Ar ages, 47.4&amp;nbsp;±&amp;nbsp;9.7 and 51.4&amp;nbsp;±&amp;nbsp;9.7&amp;nbsp;ka. We propose that these 40 Ar/ 39 Ar dates, performed on plagioclase separates, are compromised by a subtle amount of excess Ar and therefore the younger weighted mean zircon ages yield more reliable eruption ages. These results imply that the interval of rhyolite eruption at South Sister during the late Pleistocene was both shorter and more productive than previously thought and that eruption at South Sister...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6628x1m2</guid>
      <pubDate>Thu, 21 May 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Dechert, Annika E</name>
        <uri>https://orcid.org/0009-0008-3859-0284</uri>
      </author>
      <author>
        <name>Andersen, Nathan L</name>
      </author>
      <author>
        <name>Dufek, Josef</name>
      </author>
      <author>
        <name>Jilly, Christine E</name>
      </author>
    </item>
    <item>
      <title>The Magmatic‐Hydrothermal System of the Three Sisters Volcanic Cluster, Oregon, Imaged From Field Gravity Measurements</title>
      <link>https://escholarship.org/uc/item/0221t41j</link>
      <description>Abstract From 2019 to 2024, gravity surveys were conducted at the Three Sisters volcanic cluster (TSVC), measuring 246 gravity sites using a spring relative gravimeter. We calculated the residual Bouguer anomaly and identified three main zones with negative anomalies, ranging from −4 to −8&amp;nbsp;mGal, located southwest and west of South Sister, within an area that has been uplifting for the past two decades. After inversion, we obtain a 3D density model of the subsurface and identify low‐density bodies extending from the surface down to 3&amp;nbsp;km. We estimate a total of 15&amp;nbsp;k of crustal bodies with density close to 2&amp;nbsp;g/ that could store up to 5&amp;nbsp;k of water, forming an extensive hydrothermal system beneath the TSVC. We explore the possible combinations of melt compositions and temperatures that could create a bulk density close to our reference crustal density (2.5&amp;nbsp;g/) using MELTS thermodynamic simulations. Our results indicate that a magmatic mush with as little...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0221t41j</guid>
      <pubDate>Thu, 21 May 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Le Mével, Hélène</name>
      </author>
      <author>
        <name>Andersen, Nathan L</name>
      </author>
      <author>
        <name>Dechert, Annika E</name>
        <uri>https://orcid.org/0009-0008-3859-0284</uri>
      </author>
      <author>
        <name>Dufek, Josef</name>
      </author>
    </item>
    <item>
      <title>The Transition From Melt Accumulation to Eruption Initiation Recorded by Orthopyroxene Fe‐Mg Diffusion Timescales in Late Holocene Rhyolites, South Sister Volcano, Oregon Cascade Range</title>
      <link>https://escholarship.org/uc/item/7tc9m760</link>
      <description>Abstract South Sister volcano, Oregon Cascade Range, USA, has repeatedly erupted rhyolite since ca.&amp;nbsp;40&amp;nbsp;ka. The youngest such eruptions are the ca. 2&amp;nbsp;ka Rock Mesa and Devils Chain rhyolites, erupted several hundred years apart from two multi‐vent complexes separated by 3–6&amp;nbsp;km. Fe‐Mg interdiffusion models of orthopyroxene rims from both rhyolites produce timescales up to several‐thousand years, but dominantly decades‐to‐centuries. Notably, the timescales of step‐normal zoned orthopyroxene rims (i.e., normally zoned with a steep chemical gradient) from the Rock Mesa rhyolite are longer than those of reversely zoned crystals, whereas the Devils Chain produced mostly decadal timescales for both zoning types. Despite the proximity and broadly similar products of these episodes, their respective timescales indicate distinct sequences of events leading up to each eruption. The Rock Mesa timescales record centuries of magma chamber growth followed by decades of predominantly...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7tc9m760</guid>
      <pubDate>Tue, 5 May 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Andersen, Nathan L</name>
      </author>
      <author>
        <name>Dechert, Annika E</name>
      </author>
      <author>
        <name>Ruth, Dawn CS</name>
      </author>
      <author>
        <name>Sas, May</name>
      </author>
      <author>
        <name>Chouinard, Julie</name>
      </author>
      <author>
        <name>Dufek, Josef</name>
      </author>
    </item>
    <item>
      <title>Mid-Infrared, Optically Active Black Phosphorus Thin Films on Centimeter Scale</title>
      <link>https://escholarship.org/uc/item/06z1h4zb</link>
      <description>Black phosphorus (BP) is a narrow bandgap (∼0.3 eV) semiconductor with a great potential for optoelectronic devices in the mid-infrared wavelength. However, it has been challenging to achieve a high-quality scalable BP thin film. Here we present the successful synthesis of optically active BP films on a centimeter scale. We utilize the pulsed laser deposition of amorphous red phosphorus, another allotrope of phosphorus, followed by a high-pressure treatment at ∼8 GPa to induce a phase conversion into BP crystals. The crystalline quality was improved through thermal annealing, resulting in the observation of photoluminescence emission at mid-infrared wavelengths. We demonstrate high-pressure conversion on a centimeter scale with a continuous film with a thickness of ∼18 nm using a flat-belt-type high-pressure apparatus. This synthesis procedure presents a promising route to obtain optical-quality BP films, enabling the exploration of integrated optoelectronic device applications...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/06z1h4zb</guid>
      <pubDate>Fri, 24 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Higashitarumizu, Naoki</name>
      </author>
      <author>
        <name>Kawashima, Tetsuya</name>
      </author>
      <author>
        <name>Smart, Thomas</name>
      </author>
      <author>
        <name>Yalisove, Reed</name>
      </author>
      <author>
        <name>Ho, Chun Yuen</name>
      </author>
      <author>
        <name>Madsen, Morten</name>
      </author>
      <author>
        <name>Chrzan, Daryl C</name>
      </author>
      <author>
        <name>Scott, Mary C</name>
      </author>
      <author>
        <name>Jeanloz, Raymond</name>
        <uri>https://orcid.org/0000-0002-3519-7929</uri>
      </author>
      <author>
        <name>Yusa, Hitoshi</name>
      </author>
      <author>
        <name>Javey, Ali</name>
        <uri>https://orcid.org/0000-0001-7214-7931</uri>
      </author>
    </item>
    <item>
      <title>Toward a Climate OSSE Framework for Satellite Mission Design</title>
      <link>https://escholarship.org/uc/item/2qc2q0p1</link>
      <description>Abstract The rich history of observing system simulation experiments (OSSEs) does not yet include a well-established framework for using climate models. The need for a climate OSSE is triggered by the need to quantify the value of a particular measurement for reducing the uncertainty in climate predictions, which differ from numerical weather predictions in that they depend on future atmospheric composition rather than the current state of the weather. However, both weather and climate modeling communities share a need for motivating major observing system investments. Here, we outline a new framework for climate OSSEs that leverages the use of machine learning to calibrate climate model physics against existing satellite data. We demonstrate its application using NASA’s GISS-E3 model to objectively quantify the value of potential future improvements in spaceborne measurements of Earth’s planetary boundary layer. A mature climate OSSE framework should be able to quantitatively...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2qc2q0p1</guid>
      <pubDate>Mon, 20 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Fridlind, Ann M</name>
      </author>
      <author>
        <name>Elsaesser, Gregory S</name>
      </author>
      <author>
        <name>van Lier-Walqui, Marcus</name>
      </author>
      <author>
        <name>Cesana, Grégory V</name>
      </author>
      <author>
        <name>Weatherhead, Elizabeth</name>
      </author>
      <author>
        <name>Tselioudis, George</name>
      </author>
      <author>
        <name>Schmidt, Gavin</name>
      </author>
      <author>
        <name>Barahona, Donifan</name>
      </author>
      <author>
        <name>Cairns, Brian</name>
      </author>
      <author>
        <name>Collins, William D</name>
        <uri>https://orcid.org/0000-0002-4463-9848</uri>
      </author>
      <author>
        <name>Considine, David B</name>
      </author>
      <author>
        <name>Cucurull, Lidia</name>
      </author>
      <author>
        <name>DiGirolamo, Larry</name>
      </author>
      <author>
        <name>Emory, Amber</name>
      </author>
      <author>
        <name>Hasekamp, Otto</name>
      </author>
      <author>
        <name>He, Shan</name>
      </author>
      <author>
        <name>Kramer, Ryan</name>
      </author>
      <author>
        <name>Lebsock, Matthew</name>
      </author>
      <author>
        <name>Lee, Tsengdar</name>
      </author>
      <author>
        <name>Leroy, Stephen</name>
      </author>
      <author>
        <name>Lin, Wuyin</name>
      </author>
      <author>
        <name>Lugauer, Steven</name>
      </author>
      <author>
        <name>Miller, Daniel</name>
      </author>
      <author>
        <name>Mülmenstädt, Johannes</name>
      </author>
      <author>
        <name>Oreopoulos, Lazaros</name>
      </author>
      <author>
        <name>Posselt, Derek J</name>
      </author>
      <author>
        <name>Zelinka, Mark D</name>
      </author>
    </item>
    <item>
      <title>Circularization of 23S rRNA but not 16S rRNA within archaeal ribosomes</title>
      <link>https://escholarship.org/uc/item/7n2480xq</link>
      <description>BackgroundProcessing of archaeal 16S and 23S rRNAs is believed to involve excision of individual rRNAs from polycistronic precursors, circularization of excised rRNAs, and re-linearization before the incorporation into ribosomes. However, all the knowledge is derived from several isolated species, leaving open the possibility that different processes may occur in other archaeal groups.ResultsHere, we investigate rRNAs from diverse and mostly uncultivated archaea. Sequencing of total cellular RNA from eight phylum-level lineages indicates that archaeal circular 23S rRNA transcript abundances vastly exceed those of linear counterparts, and linear versions are often undetectable. As the majority of rRNAs derive from mature ribosomes, the data suggest that ribosomes contain circular 23S rRNAs. Thus, we directly sequence RNA extracted from isolated ribosomes of a model archaeon, Methanosarcina acetivorans, and confirm that the 23S rRNAs in the ribosomes are circular. Structural modeling...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7n2480xq</guid>
      <pubDate>Fri, 17 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Shi, Ling-Dong</name>
      </author>
      <author>
        <name>Penev, Petar I</name>
      </author>
      <author>
        <name>Nissley, Amos J</name>
      </author>
      <author>
        <name>Nayak, Dipti D</name>
      </author>
      <author>
        <name>Sachdeva, Rohan</name>
      </author>
      <author>
        <name>Cate, Jamie HD</name>
      </author>
      <author>
        <name>Banfield, Jillian F</name>
      </author>
    </item>
    <item>
      <title>Elastic resistive force theory: development and applications to flexible intruders</title>
      <link>https://escholarship.org/uc/item/2rj6h0ps</link>
      <description>Dry granular intrusion and extraction occur commonly for off-road vehicles, foundation work, and plant uprooting. Although many models exist to describe such scenarios, reduced-order models such as granular resistive force theory (RFT), offer a good balance between accuracy and computational cost. RFT efficiently approximates the resistive force experienced by an intruder moving through a granular medium as a function of the intruder's velocity direction, geometry, and material parameters. However, due to the explicitly velocity-dependent nature of its formulation, it fails at modeling static conditions, the force build-up that occurs before flow, and stagnant points on moving intruders. We propose elastic RFT to remedy these shortcomings. Elastic RFT intrinsically models both granular elasticity and flow adjacent to intruders by splitting intruder motion into separate parts corresponding to elastic and plastic granular deformation. This allows force to build up elastically before...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2rj6h0ps</guid>
      <pubDate>Wed, 8 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Yılmaz, Lale</name>
      </author>
      <author>
        <name>Douglas, Madison</name>
      </author>
      <author>
        <name>Perron, J Taylor</name>
      </author>
      <author>
        <name>Kamrin, Ken</name>
      </author>
    </item>
    <item>
      <title>Evaluating Atmospheric River Impacts on Energy and Moisture Transport in the Arctic Using Different Detection Algorithms</title>
      <link>https://escholarship.org/uc/item/2rd999pf</link>
      <description>Abstract  Atmospheric rivers (ARs) significantly impact the Arctic climate system by enhancing atmospheric heat and moisture transport and altering the local energy budget. Developing AR detection tools (ARDTs) is critical yet challenging. This study evaluates 12 ARDTs in the Arctic to assess their performance in representing atmospheric heat (represented by moist static energy) and moisture transport, as well as surface downward longwave radiation (LWD) and precipitation impacts, spanning 2000 to 2019 using ERA5 reanalysis. We find that AR occurrence frequency in the Arctic varies widely, from less than 1% to over 13%, depending on the ARDT. This variability leads to differences in contributions to poleward atmospheric heat (&amp;lt;1%–33%) and moisture (&amp;lt;1%–49%) transport. The highest AR frequency, and corresponding contributions to atmospheric heat and moisture transport, occurs over the Atlantic sector during non‐summer seasons for most ARDTs. This region aligns with the primary...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2rd999pf</guid>
      <pubDate>Thu, 2 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Zhang, Chen</name>
      </author>
      <author>
        <name>Cassano, John J</name>
      </author>
      <author>
        <name>Seefeldt, Mark W</name>
      </author>
      <author>
        <name>Tung, Wen‐wen</name>
      </author>
      <author>
        <name>Mahesh, Ankur</name>
      </author>
      <author>
        <name>Collins, William D</name>
        <uri>https://orcid.org/0000-0002-4463-9848</uri>
      </author>
    </item>
    <item>
      <title>Depth of nutrient uptake by deep-rooted plants is regulated by water availability</title>
      <link>https://escholarship.org/uc/item/14w4h314</link>
      <description>The capacity of some plants to access water and nutrients at depths greater than one meter is a critical functional trait that confers resistance to drought and impacts both belowground and shallow soil processes. Here, we report water and strontium isotopic data from an alpine meadow transect showing the correlation between water and nutrient acquisition depths. The isotopic compositions of Sr (&lt;sup&gt;87&lt;/sup&gt;Sr/&lt;sup&gt;86&lt;/sup&gt;Sr ratio) and water in rock and soil, and in plant leaf tissues, reveal that deeper-rooted plants acquire a higher proportion of water, Sr, and cation nutrients that are derived from the saprolite, a zone of silicate weathering, than shallow-rooted grass. A three-decade dendrochemical record reveals that reductions of wet precipitation drive deep-rooted plants to acquire cation nutrients from deeper saprolite or bedrock regions. Thus, the depth of cation nutrient acquisition by deep-rooted plant species at this site is tightly coupled with, and likely determined...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/14w4h314</guid>
      <pubDate>Mon, 30 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Li, Langlang</name>
      </author>
      <author>
        <name>Christensen, John N</name>
      </author>
      <author>
        <name>Bill, Markus</name>
        <uri>https://orcid.org/0000-0001-7002-2174</uri>
      </author>
      <author>
        <name>Dong, Wenming</name>
        <uri>https://orcid.org/0000-0003-2074-8887</uri>
      </author>
      <author>
        <name>Wu, Yuxin</name>
        <uri>https://orcid.org/0000-0002-6953-0179</uri>
      </author>
      <author>
        <name>Beutler, Curtis</name>
      </author>
      <author>
        <name>Sprenger, Matthias</name>
        <uri>https://orcid.org/0000-0003-1221-2767</uri>
      </author>
      <author>
        <name>Gulick, Brian W</name>
      </author>
      <author>
        <name>Bone, Sharon E</name>
      </author>
      <author>
        <name>Faybishenko, Boris</name>
        <uri>https://orcid.org/0000-0003-0085-8499</uri>
      </author>
      <author>
        <name>Sanders, John</name>
      </author>
      <author>
        <name>Chou, Chunwei</name>
      </author>
      <author>
        <name>Henderson, Amanda</name>
      </author>
      <author>
        <name>Bouskill, Nicholas J</name>
      </author>
      <author>
        <name>Williams, Kenneth H</name>
        <uri>https://orcid.org/0000-0002-3568-1155</uri>
      </author>
      <author>
        <name>Gilbert, Benjamin</name>
      </author>
    </item>
    <item>
      <title>A Method for Rapid and Precise Triple Oxygen Isotope Measurements via High-Temperature Conversion to CO Followed by Nickel-Catalyzed CO to CO2 Conversion and Laser Spectroscopy</title>
      <link>https://escholarship.org/uc/item/6f55j3rr</link>
      <description>Triple oxygen isotopic compositions (&lt;sup&gt;16&lt;/sup&gt;O, &lt;sup&gt;17&lt;/sup&gt;O, &lt;sup&gt;18&lt;/sup&gt;O) have conventionally been measured via isotope ratio mass spectrometry using O&lt;sub&gt;2&lt;/sub&gt; as an analyte. Conversion of sample oxygen to O&lt;sub&gt;2&lt;/sub&gt; typically utilizes fluorination chemistry or catalytic equilibration between CO&lt;sub&gt;2&lt;/sub&gt; and O&lt;sub&gt;2&lt;/sub&gt;. Recently, laser spectroscopy has become a viable alternative for triple oxygen isotope (Δ'&lt;sup&gt;17&lt;/sup&gt;O) measurements due to its ease and rapid throughput. Laser spectrometers are currently available for Δ'&lt;sup&gt;17&lt;/sup&gt;O analysis of either H&lt;sub&gt;2&lt;/sub&gt;O or CO&lt;sub&gt;2&lt;/sub&gt; as the analyte gas. So far, these instruments have been used to measure Δ'&lt;sup&gt;17&lt;/sup&gt;O of water, carbonate (CO&lt;sub&gt;2&lt;/sub&gt; liberated by acid digestion), and atmospheric CO&lt;sub&gt;2&lt;/sub&gt; samples. We present a new method for high-precision Δ'&lt;sup&gt;17&lt;/sup&gt;O analysis of CO&lt;sub&gt;2&lt;/sub&gt; via tunable infrared laser direct absorption spectroscopy that is compatible with a wider...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6f55j3rr</guid>
      <pubDate>Fri, 13 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Ellis, Nicholas M</name>
      </author>
      <author>
        <name>Kafaie, Kian R</name>
      </author>
      <author>
        <name>Wehr, Rick</name>
      </author>
      <author>
        <name>Nelson, David D</name>
      </author>
      <author>
        <name>Herndon, Scott C</name>
      </author>
      <author>
        <name>Yang, Wenbo</name>
      </author>
      <author>
        <name>Dawson, Todd E</name>
        <uri>https://orcid.org/0000-0002-6871-3440</uri>
      </author>
      <author>
        <name>Stolper, Daniel A</name>
      </author>
    </item>
    <item>
      <title>Tonian paleomagnetic poles from South China are consistent with progressive plate tectonic motion over the North Pole: COMMENT</title>
      <link>https://escholarship.org/uc/item/3td3k9nk</link>
      <description>Tonian paleomagnetic poles from South China are consistent with progressive plate tectonic motion over the North Pole: COMMENT</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3td3k9nk</guid>
      <pubDate>Fri, 13 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Swanson-Hysell, Nicholas L</name>
        <uri>https://orcid.org/0000-0003-3215-4648</uri>
      </author>
    </item>
    <item>
      <title>Applicability of the Mie–Grüneisen Equation of State Model to Warm Dense Matter Conditions</title>
      <link>https://escholarship.org/uc/item/5q48038r</link>
      <description>ABSTRACT  The Mie–Grüneisen (MG) model provides a linear relation between thermal pressure (pressure relative to a reference temperature) and the corresponding thermal energy, which is widely used to interpolate and extrapolate equations of state (EOS) beyond experimental data. However, its applicability to warm dense matter (WDM) conditions, where strong coupling and ionization become significant, remains poorly constrained. Here we assess the validity of the MG approximation using first‐principles simulations of representative materials—MgO, H, He, Si, CH 2 and others—spanning the condensed and WDM regimes. Combining finite‐temperature density functional theory molecular dynamics (DFT‐MD) with path integral Monte Carlo (PIMC), we compute consistent pressure and energy relations over a wide range of densities and temperatures. We show that the proportionality between thermal pressure and thermal energy is linear function of density but does depend on temperature, allowing us...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5q48038r</guid>
      <pubDate>Wed, 11 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>González‐Cataldo, Felipe</name>
      </author>
      <author>
        <name>Militzer, Burkhard</name>
      </author>
    </item>
    <item>
      <title>No Warm-Phase Invigoration of Convection Detected during GoAmazon</title>
      <link>https://escholarship.org/uc/item/80g49179</link>
      <description>Abstract It has been proposed that air pollution increases the updraft speeds of warm-phase convective clouds by reducing their supersaturation and, thereby, enhancing their buoyancy. Observations from the GoAmazon field campaign, sampled using subjective criteria, have been offered as evidence for this warm-phase invigoration. Here, we reexamine those GoAmazon observations using objective sampling criteria and find no indication that air pollution increases warm-phase updraft speeds. In addition, the observations yield no statistically significant relationship between aerosol concentrations and either moist-convective vertical velocity or reflectivity in either the lower or upper troposphere.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/80g49179</guid>
      <pubDate>Tue, 10 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Öktem, Rusen</name>
      </author>
      <author>
        <name>Romps, David M</name>
      </author>
      <author>
        <name>Varble, Adam C</name>
      </author>
    </item>
    <item>
      <title>Pinned Clouds over Industrial Sources of Heat during TRACER</title>
      <link>https://escholarship.org/uc/item/4wf6v1h8</link>
      <description>Abstract An analysis of stereo-camera data from the Tracking Aerosol Convection Interactions Experiment (TRACER) campaign in Houston, Texas, reveals the existence of pinned clouds sitting atop industrial heat sources. These are not plumes of vapor and condensate emanating from stacks: The pinned shallow cumuli have cloud bases at about the lifting condensation of near-surface air. On many mornings, the pinned clouds are the only shallow cumuli in the field of view of the stereo cameras, persisting by themselves for at least an hour. On those mornings, the lower atmosphere straddles the boundary between stable and unstable, and the waste heat from industrial facilities is able to pin moist convection overhead. When solar heating of the surface becomes sufficient later in the morning, those mornings transition to having widespread shallow moist convection. Occurring within the field of view of the stereo cameras and other TRACER instruments, these pinned clouds represent steady...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4wf6v1h8</guid>
      <pubDate>Tue, 10 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Öktem, Rusen</name>
      </author>
      <author>
        <name>Giangrande, Scott E</name>
      </author>
      <author>
        <name>Romps, David M</name>
      </author>
    </item>
    <item>
      <title>The NASA Psyche Mission: The First up-Close Exploration of a Metal-Rich World</title>
      <link>https://escholarship.org/uc/item/1fv2v6jd</link>
      <description>The NASA Psyche Mission: The First up-Close Exploration of a Metal-Rich World</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1fv2v6jd</guid>
      <pubDate>Sat, 14 Feb 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Bell, James F</name>
      </author>
      <author>
        <name>Elkins-Tanton, Lindy</name>
      </author>
      <author>
        <name>Polanskey, Carol A</name>
      </author>
    </item>
    <item>
      <title>Integrating fiber-optic seismic arrays into earthquake early warning systems with the dEPIC framework</title>
      <link>https://escholarship.org/uc/item/8pd361dw</link>
      <description>Distributed Acoustic Sensing (DAS) can enhance earthquake early warning (EEW) by transforming existing fiber-optic cables into dense seismic arrays, including in offshore areas with sparse instrumentation. We present dEPIC (DAS–Earthquake Point-source Integrated Code), the first operational DAS-integrated EEW framework, deployed on a submarine cable in Monterey Bay, California, and designed to operate independently or jointly with ShakeAlert’s EPIC algorithm. dEPIC combines GPU-accelerated machine-learning phase picking, grid-search location, and empirical magnitude estimation, with real-time quality metrics to suppress unstable solutions. In event replays and continuous data tests, dEPIC detected both onshore and offshore earthquakes accurately with sub-second processing time. The modular, edge-computing design enables adaptation to future DAS deployments to improve existing EEW systems like ShakeAlert.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8pd361dw</guid>
      <pubDate>Wed, 28 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Gou, Yuancong</name>
        <uri>https://orcid.org/0000-0001-6313-0564</uri>
      </author>
      <author>
        <name>Nof, Ran N</name>
      </author>
      <author>
        <name>Pardini, Brian</name>
      </author>
      <author>
        <name>Allen, Richard M</name>
        <uri>https://orcid.org/0000-0003-4293-9772</uri>
      </author>
    </item>
    <item>
      <title>SeaFOAM: A Year-Long DAS Deployment in Monterey Bay, California</title>
      <link>https://escholarship.org/uc/item/51t0823t</link>
      <description>Abstract Distributed acoustic sensing (DAS) is being explored in a variety of environments as a promising technology for the recording of seismic signals in dense array configurations. There is a particular interest for deploying DAS arrays on the ocean floor, presenting formidable challenges for conventional seismology. Taking advantage of the availability of a dark fiber on the Monterey Bay Accelerated Research System (MARS) 52&amp;nbsp;km offshore cable at Monterey Bay, California, in July 2022, we installed a DAS interrogator at the shore end of the cable with the intention of acquiring continuous data for a period of one year. Here, we describe the experiment and present examples of observations over the first six months of the deployment.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/51t0823t</guid>
      <pubDate>Wed, 28 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Romanowicz, Barbara</name>
        <uri>https://orcid.org/0000-0002-6208-6044</uri>
      </author>
      <author>
        <name>Allen, Richard</name>
        <uri>https://orcid.org/0000-0003-4293-9772</uri>
      </author>
      <author>
        <name>Brekke, Knute</name>
      </author>
      <author>
        <name>Chen, Li-Wei</name>
        <uri>https://orcid.org/0000-0002-9403-4505</uri>
      </author>
      <author>
        <name>Gou, Yuancong</name>
        <uri>https://orcid.org/0000-0001-6313-0564</uri>
      </author>
      <author>
        <name>Henson, Ivan</name>
      </author>
      <author>
        <name>Marty, Julien</name>
      </author>
      <author>
        <name>Neuhauser, Doug</name>
      </author>
      <author>
        <name>Pardini, Brian</name>
      </author>
      <author>
        <name>Taira, Taka’aki</name>
      </author>
      <author>
        <name>Thompson, Stephen</name>
      </author>
      <author>
        <name>Zhang, Junli</name>
      </author>
      <author>
        <name>Zuzlewski, Stephane</name>
      </author>
    </item>
    <item>
      <title>Mantle-like Sr isotopes in a Sturtian cap carbonate in Oman</title>
      <link>https://escholarship.org/uc/item/3h979891</link>
      <description>Abstract Twice in the Cryogenian Period (720–635 Ma), during the Sturtian and Marinoan glaciations, ice sheets extended to equatorial latitudes for millions of years. These climate extremes have been interpreted to record the Snowball climate state, in which all of Earth’s oceans were covered with ice. During a Snowball Earth, the hydrological cycle would have been curtailed and silicate weathering greatly reduced. In this scenario, deep ocean chemistry should have evolved toward mantle values through hydrothermal exchange at mid-ocean ridges. Specifically, seawater strontium isotopes (87Sr/86Sr) are predicted to exhibit unradiogenic mantle-like values. However, cap carbonates that overlie the Cryogenian glacial deposits have yielded radiogenic 87Sr/86Sr values similar to those of seawater prior to glaciation, inconsistent with the central geochemical prediction of the Snowball Earth hypothesis. Here we report the discovery of 87Sr/86Sr values of 0.7034 in marine carbonate and...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3h979891</guid>
      <pubDate>Wed, 14 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Macdonald, Francis A</name>
        <uri>https://orcid.org/0000-0001-8416-4894</uri>
      </author>
      <author>
        <name>Renger, Ellery</name>
      </author>
      <author>
        <name>Tasistro-Hart, Adrian R</name>
      </author>
      <author>
        <name>Byerly, Benjamin L</name>
      </author>
      <author>
        <name>Jackson, Matthew G</name>
      </author>
      <author>
        <name>Bergmann, Kristin D</name>
      </author>
      <author>
        <name>Horner, Tristan J</name>
      </author>
      <author>
        <name>Crockford, Peter W</name>
      </author>
    </item>
    <item>
      <title>Annual-to-millennial fluctuations in the physical properties of crystal-rich magma storage zones.</title>
      <link>https://escholarship.org/uc/item/9j38506c</link>
      <description>Basaltic melts may variably disaggregate macrocrysts (large crystals) from crystal mushes during the assembly of magma bodies beneath ocean-island volcanoes. The entrained macrocrysts modulate the crystallinity, density, and rheology of magmas, parameters that control magma system architecture and eruptive dynamics. However, the timescales, drivers, and consequences of inconstant crystal mush incorporation into carrier melts require quantification. Here, we use a suite of plagioclase-rich basalts to show that the entrainment efficiency (the ability for melts to disaggregate and entrain macrocrysts from crystal mushes) is temporally variable on inter-eruption timescales at ocean-island volcanoes. Macrocryst cargoes are predominantly out of equilibrium with their carrier melts in both chemistries and mass proportions (ratios of different macrocryst phases). Geochemical and petrological evidence reveals that macrocryst mass proportions are established in a density-stratified melt-rich...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9j38506c</guid>
      <pubDate>Thu, 8 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Higgins, Oliver</name>
      </author>
      <author>
        <name>Stock, Michael</name>
      </author>
      <author>
        <name>Geist, Dennis</name>
      </author>
      <author>
        <name>Neave, David</name>
      </author>
      <author>
        <name>Buisman, Iris</name>
      </author>
      <author>
        <name>Bernard, Benjamin</name>
      </author>
      <author>
        <name>Gleeson, Matthew</name>
      </author>
    </item>
    <item>
      <title>Complex Dependence of Calcite Crack Kinetics on Salinity: The Role of DLVO and Hydration Forces</title>
      <link>https://escholarship.org/uc/item/9c07568w</link>
      <description>Abstract Subcritical crack growth (SCG) plays an important role in many geological processes such as delayed earth rupture and rock weathering. The complex dependency of SCG on the in‐crack fluid chemistry, however, is still poorly understood. In this study, we utilize the newly developed surface force‐based fracture theory (SFFT) to elucidate the relative contributions of surface forces and solute transport to the crack growth kinetics of calcite in NaCl solutions. Expanding on Barenblatt's cohesive crack model, SFFT introduces an effective stress intensity at the crack tip that encompasses all the relevant intermolecular forces across the crack in addition to the external far‐field stresses. The nonlinear system of equations portraying the crack opening profile, the solute distribution in a propagating crack, and the crack growth velocity are numerically solved via an implicit scheme. After carefully calibrating the model for calcite‐water systems, the SFFT is used to predict...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9c07568w</guid>
      <pubDate>Mon, 15 Dec 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Dadras, Hooman</name>
      </author>
      <author>
        <name>Eskandari‐Ghadi, Mehdi</name>
      </author>
      <author>
        <name>Nakagawa, Seiji</name>
        <uri>https://orcid.org/0000-0002-9347-0903</uri>
      </author>
      <author>
        <name>Gilbert, Benjamin</name>
      </author>
      <author>
        <name>Zhang, Yida</name>
      </author>
    </item>
    <item>
      <title>Huge ensembles – Part 2: Properties of a huge ensemble of hindcasts generated with spherical Fourier neural operators</title>
      <link>https://escholarship.org/uc/item/53f2p5xt</link>
      <description>Abstract. In Part&amp;nbsp;1, we created an ensemble based on spherical Fourier neural operators. As initial condition perturbations, we used bred vectors, and as model perturbations, we used multiple checkpoints trained independently from scratch. Based on diagnostics that assess the ensemble's physical fidelity, our ensemble has comparable performance to operational weather forecasting systems. However, it requires orders-of-magnitude fewer computational resources. Here in Part 2, we generate a huge ensemble (HENS), with 7424 members initialized each day of summer 2023. We enumerate the technical requirements for running huge ensembles at this scale. HENS precisely samples the tails of the forecast distribution and presents a detailed sampling of internal variability. HENS has two primary applications: (1)&amp;nbsp;as a large dataset with which to study the statistics and drivers of extreme weather and (2)&amp;nbsp;as a weather forecasting system. For extreme climate statistics, HENS samples...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/53f2p5xt</guid>
      <pubDate>Mon, 17 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Mahesh, Ankur</name>
      </author>
      <author>
        <name>Collins, William D</name>
        <uri>https://orcid.org/0000-0002-4463-9848</uri>
      </author>
      <author>
        <name>Bonev, Boris</name>
      </author>
      <author>
        <name>Brenowitz, Noah</name>
      </author>
      <author>
        <name>Cohen, Yair</name>
      </author>
      <author>
        <name>Harrington, Peter</name>
      </author>
      <author>
        <name>Kashinath, Karthik</name>
      </author>
      <author>
        <name>Kurth, Thorsten</name>
      </author>
      <author>
        <name>North, Joshua</name>
        <uri>https://orcid.org/0000-0001-7631-8021</uri>
      </author>
      <author>
        <name>O'Brien, Travis A</name>
        <uri>https://orcid.org/0000-0002-6643-1175</uri>
      </author>
      <author>
        <name>Pritchard, Michael</name>
      </author>
      <author>
        <name>Pruitt, David</name>
      </author>
      <author>
        <name>Risser, Mark</name>
        <uri>https://orcid.org/0000-0003-1956-1783</uri>
      </author>
      <author>
        <name>Subramanian, Shashank</name>
      </author>
      <author>
        <name>Willard, Jared</name>
      </author>
    </item>
    <item>
      <title>Huge ensembles – Part 1: Design of ensemble weather forecasts using spherical Fourier neural operators</title>
      <link>https://escholarship.org/uc/item/09f7p278</link>
      <description>Abstract. Simulating low-likelihood high-impact extreme weather events in a warming world is a significant and challenging task for current ensemble forecasting systems. While these systems presently use up to 100 members, larger ensembles could enrich the sampling of internal variability. They may capture the long tails associated with climate hazards better than traditional ensemble sizes. Due to computational constraints, it is infeasible to generate huge ensembles (comprised of 1000–10 000 members) with traditional, physics-based numerical models. In this two-part paper, we replace traditional numerical simulations with machine learning (ML) to generate hindcasts of huge ensembles. In Part&amp;nbsp;1, we construct an ensemble weather forecasting system based on spherical Fourier neural operators (SFNOs), and we discuss important design decisions for constructing such an ensemble. The ensemble represents model uncertainty through perturbed-parameter techniques, and it represents...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/09f7p278</guid>
      <pubDate>Mon, 17 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Mahesh, Ankur</name>
      </author>
      <author>
        <name>Collins, William D</name>
        <uri>https://orcid.org/0000-0002-4463-9848</uri>
      </author>
      <author>
        <name>Bonev, Boris</name>
      </author>
      <author>
        <name>Brenowitz, Noah</name>
      </author>
      <author>
        <name>Cohen, Yair</name>
      </author>
      <author>
        <name>Elms, Joshua</name>
      </author>
      <author>
        <name>Harrington, Peter</name>
      </author>
      <author>
        <name>Kashinath, Karthik</name>
      </author>
      <author>
        <name>Kurth, Thorsten</name>
      </author>
      <author>
        <name>North, Joshua</name>
        <uri>https://orcid.org/0000-0001-7631-8021</uri>
      </author>
      <author>
        <name>O'Brien, Travis</name>
        <uri>https://orcid.org/0000-0002-6643-1175</uri>
      </author>
      <author>
        <name>Pritchard, Michael</name>
      </author>
      <author>
        <name>Pruitt, David</name>
      </author>
      <author>
        <name>Risser, Mark</name>
        <uri>https://orcid.org/0000-0003-1956-1783</uri>
      </author>
      <author>
        <name>Subramanian, Shashank</name>
      </author>
      <author>
        <name>Willard, Jared</name>
      </author>
    </item>
    <item>
      <title>Another Other: An Unlikely Path to a Future United World-and What That Future Would Think about Us</title>
      <link>https://escholarship.org/uc/item/9hp611qp</link>
      <description>We are separated from the future by a chasm of imagined apocalypses and miracles. We are separated from the technological foundation of our society by a chasm of scale between the individual self and the global manufacturing network. And we are separated from each other by chasms of bias and fear. Despite - or maybe because of - some of our looming apocalypses, our future selves might be less separated from technology and from each other. Population decline, the creation of self-sustaining Throughline communities, and the eventual discovery of alien life create possible futures populated with viewpoints that might see us, the Before Time people, as barbarians or, conversely, as technological gods.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9hp611qp</guid>
      <pubDate>Wed, 8 Oct 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Elkins-Tanton, Lindy</name>
      </author>
    </item>
    <item>
      <title>Oman was on the northern margin of a wide late Tonian Mozambique Ocean</title>
      <link>https://escholarship.org/uc/item/8gw0c7x2</link>
      <description>The closure of the Mozambique Ocean defines the final assembly of the megacontinent Gondwana and is associated with a vast region of crustal growth in the Arabian-Nubian Shield. Despite this central paleogeographic position, there are few constraints on the position of terranes within and bounding the Mozambique Ocean. We report paleomagnetic data from ca. 726 Ma dikes exposed in southern Oman. Well-resolved magnetite magnetization is constrained to be primary by a conglomerate test on mafic clasts within overlying Cryogenian diamictite. The resulting paleomagnetic pole indicates that Oman was at a paleolatitude of 37 ± 2.5°N and was rotated ∼80° counterclockwise from its present-day orientation. This position is consistent with Oman forming a contiguous plate with the India and South China cratons on the northern margin of the Mozambique Ocean in a distinct tectonic domain from Arabian-Nubian arcs to the south. This position reveals an ∼5500-km-wide oceanic realm prior to subsequent...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8gw0c7x2</guid>
      <pubDate>Wed, 8 Oct 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Swanson-Hysell, Nicholas L</name>
        <uri>https://orcid.org/0000-0003-3215-4648</uri>
      </author>
      <author>
        <name>Zhang, Yiming</name>
      </author>
      <author>
        <name>Macdonald, Francis A</name>
      </author>
      <author>
        <name>Koran, Isabel</name>
      </author>
      <author>
        <name>Tasistro-Hart, Adrian R</name>
      </author>
      <author>
        <name>Jay, Annabel F</name>
      </author>
    </item>
    <item>
      <title>Evolution of iron formation to ore during Ediacaran to early Paleozoic tectonic stability</title>
      <link>https://escholarship.org/uc/item/6144d9hp</link>
      <description>Evolution of iron formation to ore during Ediacaran to early Paleozoic tectonic stability</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6144d9hp</guid>
      <pubDate>Wed, 24 Sep 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Fuentes, Anthony J</name>
        <uri>https://orcid.org/0000-0003-2902-5204</uri>
      </author>
      <author>
        <name>Courtney-Davies, Liam</name>
        <uri>https://orcid.org/0000-0002-7362-1786</uri>
      </author>
      <author>
        <name>Flowers, Rebecca</name>
        <uri>https://orcid.org/0000-0001-6563-1143</uri>
      </author>
      <author>
        <name>Zhang, Yiming</name>
        <uri>https://orcid.org/0000-0002-1407-302X</uri>
      </author>
      <author>
        <name>Swanson-Hysell, Nicholas</name>
        <uri>https://orcid.org/0000-0003-3215-4648</uri>
      </author>
    </item>
    <item>
      <title>Mobility, Thickness, and Hydraulic Diffusivity of the Slow‐Moving Monroe Landslide in California Revealed by L‐Band Satellite Radar Interferometry</title>
      <link>https://escholarship.org/uc/item/6tj548m6</link>
      <description>Active landslides cause fatalities and property losses worldwide. Landslide behaviors can be enigmatic in natural landscapes and therefore require high-quality observations of their kinematics to improve our ability to predict landslide behavior. Here we use geodetic interferometric synthetic aperture radar (InSAR) observations to characterize the geometry and the spatio-temporal deformation of the slow-moving, deep-seated Monroe landslide in northern California between 2007 and 2017. InSAR phase discontinuities show that the landslide is bounded by discrete strike-slip faults at the lateral margins and segregated into distinct kinematic elements by normal and thrust faults. We find that the Monroe landslide has been moving consistently, with a maximum rate of about 0.7 m/year in the narrowest longitudinal center of the transport zone. The thickest landslide mass is estimated to be in a zone located between subsiding and the uplifting kinematic elements at the lower transport...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6tj548m6</guid>
      <pubDate>Wed, 10 Sep 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Hu, Xie</name>
      </author>
      <author>
        <name>Bürgmann, Roland</name>
      </author>
      <author>
        <name>Lu, Zhong</name>
      </author>
      <author>
        <name>Handwerger, Alexander L</name>
        <uri>https://orcid.org/0000-0001-9235-3871</uri>
      </author>
      <author>
        <name>Wang, Teng</name>
      </author>
      <author>
        <name>Miao, Runze</name>
      </author>
    </item>
    <item>
      <title>Deep learning forecasts the spatiotemporal evolution of fluid-induced microearthquakes</title>
      <link>https://escholarship.org/uc/item/8153192k</link>
      <description>Microearthquakes generated by subsurface fluid injection record the evolving stress state and permeability of reservoirs. Forecasting their spatiotemporal evolution is therefore critical for applications such as enhanced geothermal systems, carbon dioxide sequestration and other geoengineering applications. Here we propose a transformer neural network model that ingests hydraulic stimulation history and prior microearthquake observations to forecast four key quantities: cumulative microearthquake count, cumulative logarithmic seismic moment, and the 50th- and 95th-percentile extents of the microearthquake cloud. Applied to the EGS Collab Experiment 1 dataset, the model achieves R2 &amp;gt; 0.98 for the 1-s forecast horizon and R2 &amp;gt; 0.88 for the 15-s forecast horizon across all targets, and supplies uncertainty estimates through a learned standard deviation term. These accurate, uncertainty-quantified forecasts enable real-time inference of fracture propagation and permeability...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8153192k</guid>
      <pubDate>Mon, 8 Sep 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Chung, Jaehong</name>
      </author>
      <author>
        <name>Manga, Michael</name>
        <uri>https://orcid.org/0000-0003-3286-4682</uri>
      </author>
      <author>
        <name>Kneafsey, Timothy</name>
        <uri>https://orcid.org/0000-0002-3926-8587</uri>
      </author>
      <author>
        <name>Mukerji, Tapan</name>
      </author>
      <author>
        <name>Hu, Mengsu</name>
        <uri>https://orcid.org/0000-0002-8853-2022</uri>
      </author>
    </item>
    <item>
      <title>Methanogenesis and Acetogenesis in Hydrogenotrophy with Carbonate Minerals: Dependence on Mineral Surface Area, Biofilm Growth, and Microbial Community</title>
      <link>https://escholarship.org/uc/item/1z86p6sq</link>
      <description>The production, storage, and use of hydrogen are anticipated to grow substantially to achieve energy and climate goals. Consequently, microbial communities in many terrestrial and subsurface Earth environments could be exposed to elevated hydrogen concentrations. Hydrogen stimulates metabolic processes that reduce aqueous chemical species, such as bicarbonate or sulfate, that can exchange with solid mineral phases, but the controls on microbial hydrogenotrophy with mineral sources of electron acceptors are not fully understood. Herein, we applied laboratory experiments and biogeochemical modeling to study the response of a natural microbial community to an elevated partial pressure of hydrogen in the presence of carbonate minerals of varying composition, solubility, and size. Experimental incubations and simulation results showed that hydrogen consumption by microbial communities was initially dominated by sulfate reduction and, subsequently, transitioned to acetogenesis and methanogenesis....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1z86p6sq</guid>
      <pubDate>Mon, 8 Sep 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Qi, Yarong</name>
      </author>
      <author>
        <name>Borglin, Sharon</name>
      </author>
      <author>
        <name>Li, Langlang</name>
      </author>
      <author>
        <name>Dong, Wenming</name>
        <uri>https://orcid.org/0000-0003-2074-8887</uri>
      </author>
      <author>
        <name>Bill, Markus</name>
        <uri>https://orcid.org/0000-0001-7002-2174</uri>
      </author>
      <author>
        <name>Hao, Zhao</name>
        <uri>https://orcid.org/0000-0003-0677-8529</uri>
      </author>
      <author>
        <name>Pallud, Céline</name>
      </author>
      <author>
        <name>Gilbert, Benjamin</name>
      </author>
    </item>
    <item>
      <title>Decomposing Cloud Radiative Feedbacks by Cloud-Top Phase</title>
      <link>https://escholarship.org/uc/item/86g4c655</link>
      <description>Abstract: 

Changes in cloud scattering properties and emissivity that arise from atmospheric warming cause substantial radiative feedbacks in model projections of anthropogenic climate change, and the relative importance of the underlying mechanisms is poorly understood. One leading hypothesis is that ice-to-liquid conversions cause clouds to optically thicken, producing a major negative feedback. We test this hypothesis by developing a method to decompose cloud radiative feedbacks by cloud-top phase. The method is applied to an ensemble of six state-of-the-art global climate models run with prescribed sea surface temperature. In these simulations, the global mean of the net cloud scattering and emissivity feedback from cloud-phase conversions ranges from −0.17 to −0.01 W m−2 K−1, while the overall net cloud feedback ranges from 0.02 to 0.91 W m−2 K−1. The multimodel mean of the cloud scattering and emissivity feedback from cloud-phase conversions is approximately 19% of the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/86g4c655</guid>
      <pubDate>Thu, 4 Sep 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Wall, Casey J</name>
      </author>
      <author>
        <name>Paynter, David</name>
      </author>
      <author>
        <name>Qin, Yi</name>
      </author>
      <author>
        <name>Debolskiy, Matvey</name>
      </author>
      <author>
        <name>Duffy, Margaret L</name>
      </author>
      <author>
        <name>Michibata, Takuro</name>
      </author>
      <author>
        <name>Duran, Brandon M</name>
        <uri>https://orcid.org/0000-0001-5427-8700</uri>
      </author>
      <author>
        <name>Lutsko, Nicholas J</name>
      </author>
      <author>
        <name>Ma, Po-Lun</name>
      </author>
      <author>
        <name>Medeiros, Brian</name>
      </author>
      <author>
        <name>Storelvmo, Trude</name>
      </author>
      <author>
        <name>Zhao, Ming</name>
      </author>
    </item>
    <item>
      <title>Stable isotope equilibria in the dihydrogen-water-methane-ethane-propane system. Part 2: Experimental determination of hydrogen isotopic equilibrium for ethane-H2 from 30 to 200&amp;nbsp;°C and propane-H2 from 75 to 200&amp;nbsp;°C</title>
      <link>https://escholarship.org/uc/item/6cn4r406</link>
      <description>The stable isotopic compositions of light n-alkanes, including methane, ethane, and propane, are often used to identify the sources and thermal maturity of natural gas samples. Though stable isotopic compositions of these molecules are commonly assumed to be controlled by kinetic isotope effects, recent studies have proposed both carbon and hydrogen isotopic equilibrium may also occur in some samples. Assessing whether samples are in isotopic equilibrium requires knowledge of light alkane equilibrium fractionation factors over geologically relevant temperatures for formation and storage (up to ∼300&amp;nbsp;°C). In this study, we report experimental results of hydrogen isotopic equilibrium between ethane and H2 from 30 to 200&amp;nbsp;°C and propane and H2 from 75 to 200&amp;nbsp;°C. We compare these results with high-level theoretical calculations and provide a preferred polynomial fit to describe equilibrium fractionation factors. Comparison of these fractionation factors with a compilation...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6cn4r406</guid>
      <pubDate>Tue, 2 Sep 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Turner, Andrew C</name>
      </author>
      <author>
        <name>Korol, Roman</name>
      </author>
      <author>
        <name>Bill, Markus</name>
        <uri>https://orcid.org/0000-0001-7002-2174</uri>
      </author>
      <author>
        <name>Stolper, Daniel A</name>
      </author>
    </item>
    <item>
      <title>Termination of Laurentia's Rapid Plate Motion at the Start of the Grenvillian Orogeny</title>
      <link>https://escholarship.org/uc/item/45r1s9ht</link>
      <description>Late Mesoproterozoic to Neoproterozoic sedimentary sequences within the Lake Superior region preserve critical paleogeographic records of the position of Laurentia spanning from the end of Midcontinent Rift extension through to the end of the Grenvillian Orogeny. Temporally calibrated paleomagnetic poles from these sequences are essential for resolving Laurentia's plate motion during these tectonic events. The (Formula presented.) 5&amp;nbsp;km thick ca. 1,080 to 1,045&amp;nbsp;Ma fluviolacustrine Oronto Group was deposited during thermal subsidence following rifting prior to onset of Grenvillian contractional deformation in the region. Prior paleomagnetic work has focused on the basal Freda Formation (ca. 1,075&amp;nbsp;Ma) leaving a long temporal gap in poles from that time until the ca. 990&amp;nbsp;Ma pole of the unconformably overlying Jacobsville Formation. A new U-Pb detrital zircon maximum depositional age for the upper Freda Formation of 1,051.6 (Formula presented.) 1.1&amp;nbsp;Ma indicates...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/45r1s9ht</guid>
      <pubDate>Wed, 20 Aug 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Fuentes, Anthony J</name>
      </author>
      <author>
        <name>Fairchild, Luke M</name>
      </author>
      <author>
        <name>Hodgin, Eben B</name>
      </author>
      <author>
        <name>Alemu, Tadesse</name>
      </author>
      <author>
        <name>Swanson‐Hysell, Nicholas</name>
      </author>
    </item>
    <item>
      <title>Impacts of the Large Seasonal Cycle of Upwelling Zone Sea Surface Temperatures on the Atmosphere</title>
      <link>https://escholarship.org/uc/item/35d292d7</link>
      <description>Abstract The amplitude of the annual cycle of sea surface temperatures (SSTs) within the tropics is the largest in the eastern Atlantic and Pacific Oceans. Upwelling activity in these regions is maximum during late boreal summer and autumn, resulting in cool SSTs, and minimum in spring, leading to warm SSTs. The fundamental question of how this large seasonal cycle affects the atmosphere has received relatively little scientific attention. In this study, we use perturbed-SST experiments in an atmosphere model to identify the effects of the seasonal cycle of upwelling zone SSTs on the atmospheric state. Although annual-mean upwelling zone SSTs are cool, preventing their convective coupling with the free troposphere for much of the year, their boreal spring warmth can activate precipitating convection. We find that in this season, upwelling zone SSTs affect the atmosphere by 1) altering the intensity and position of the local intertropical convergence zone and 2) inducing a thermally...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/35d292d7</guid>
      <pubDate>Fri, 15 Aug 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Ramesh, Nandini</name>
      </author>
      <author>
        <name>Boos, William R</name>
        <uri>https://orcid.org/0000-0001-9076-3551</uri>
      </author>
    </item>
    <item>
      <title>Response of Atmospheric River Width and Intensity to Aquaplanet Warming: A Detection Algorithm‐ and Background Moisture‐Independent Approach</title>
      <link>https://escholarship.org/uc/item/1sq9b6r5</link>
      <description>Abstract The width of an atmospheric river (AR) is an important parameter when evaluating its impact. Although previous research suggests ARs will widen with global warming, a precise response has been muddled by the large sensitivity of width to a diverse set of AR detection techniques (ARDTs). Here, we propose a methodology that removes the influence of the ARDT by modeling AR‐integrated vapor transport (IVT) profiles as idealized exponential curves with free parameters given by background IVT, intensity above background IVT, and profile width. Notably, our definition for AR profile width does not include any explicit numerical thresholds, relative or absolute, for IVT. We apply our approach to a series of idealized aquaplanet experiments, first with a baseline sea surface temperature (SST) distribution, and then with +2K, +4K, and +6K uniform warming, so as to determine the contributions of each free parameter to AR width. We also apply our approach to high‐resolution atmosphere‐only...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1sq9b6r5</guid>
      <pubDate>Thu, 14 Aug 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Baek, Seung H</name>
      </author>
      <author>
        <name>McClenny, Elizabeth E</name>
      </author>
      <author>
        <name>Ullrich, Paul A</name>
        <uri>https://orcid.org/0000-0003-4118-4590</uri>
      </author>
      <author>
        <name>Quagraine, Kwesi T</name>
      </author>
      <author>
        <name>Collins, William D</name>
        <uri>https://orcid.org/0000-0002-4463-9848</uri>
      </author>
    </item>
    <item>
      <title>Principles of stereo reconstruction of aerial objects using stationary cameras</title>
      <link>https://escholarship.org/uc/item/2p33x62d</link>
      <description>An overview is given here of the principles and mathematics of stereo reconstruction of objects in the sky using stationary cameras with an emphasis on meteorological applications. Through its Atmospheric Radiation Measurement program, the Department of Energy has operated stereo-photogrammetric cameras since 2017 as part of an effort to measure the life-cycle properties of clouds. At the core of that technology is stereo reconstruction, which calculates the real-world position of an object from the location of the object’s image in two cameras’ photographs. Here, stereo reconstruction is stripped down to its basic elements and presented using conventions tailored to applications in atmospheric science. In addition, the resulting equations are used to illustrate the high sensitivity of reconstructed cloud positions to errors in the cameras’ Euler angles. The interested reader will find here a self-contained guide to performing stereo reconstructions using distortion-corrected...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2p33x62d</guid>
      <pubDate>Tue, 22 Jul 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Romps, David M</name>
      </author>
    </item>
    <item>
      <title>Upper bounds for 21st-century surface air temperatures in the Western United States</title>
      <link>https://escholarship.org/uc/item/8rk322qm</link>
      <description>The last decade has seen a large number of severe heatwaves that were unprecedented in the observational record, highlighting challenges associated with observationally-based statistical quantification of the likelihood and magnitude of future extreme temperatures. An alternative to such probabilistic assessments is identification of upper bounds that quantify the hottest surface air temperatures that can possibly be achieved by the end of the 21st century. Theory, simulations, and observational analyses support the existence of a finite upper bound for surface air temperature; however, estimates for future upper-bound values that are realistic and usable for planning remain unavailable. Here, we combine atmospheric theory with large ensembles of dynamically downscaled projections to estimate historical and end-of-century upper bounds for surface air temperatures. A number of physical mechanisms can influence upper bounds, and at the end of the 21st century, estimates based on...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8rk322qm</guid>
      <pubDate>Tue, 15 Jul 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Risser, Mark D</name>
        <uri>https://orcid.org/0000-0003-1956-1783</uri>
      </author>
      <author>
        <name>Feldman, Daniel R</name>
      </author>
      <author>
        <name>Boos, William R</name>
        <uri>https://orcid.org/0000-0001-9076-3551</uri>
      </author>
      <author>
        <name>Rahimi, Stefan</name>
      </author>
    </item>
    <item>
      <title>Earthquake focal mechanisms with distributed acoustic sensing</title>
      <link>https://escholarship.org/uc/item/68p1m10d</link>
      <description>Earthquake focal mechanisms provide critical in-situ insights about the subsurface faulting geometry and stress state. For frequent small earthquakes (magnitude&amp;lt; 3.5), their focal mechanisms are routinely determined using first-arrival polarities picked on the vertical component of seismometers. Nevertheless, their quality is usually limited by the azimuthal coverage of the local seismic network. The emerging distributed acoustic sensing (DAS) technology, which can convert pre-existing telecommunication cables into arrays of strain/strain-rate meters, can potentially fill the azimuthal gap and enhance constraints on the nodal plane orientation through its long sensing range and dense spatial sampling. However, determining first-arrival polarities on DAS is challenging due to its single-component sensing and low signal-to-noise ratio for direct body waves. Here, we present a data-driven method that measures P-wave polarities on a DAS array based on cross-correlations between...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/68p1m10d</guid>
      <pubDate>Tue, 15 Jul 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Li, Jiaxuan</name>
      </author>
      <author>
        <name>Zhu, Weiqiang</name>
        <uri>https://orcid.org/0000-0003-2889-1493</uri>
      </author>
      <author>
        <name>Biondi, Ettore</name>
      </author>
      <author>
        <name>Zhan, Zhongwen</name>
      </author>
    </item>
    <item>
      <title>Erratum to “Leveraging Submarine DAS Arrays for Offshore Earthquake Early Warning: A Case Study in Monterey Bay, California”</title>
      <link>https://escholarship.org/uc/item/2z80f5nh</link>
      <description>Erratum to “Leveraging Submarine DAS Arrays for Offshore Earthquake Early Warning: A Case Study in Monterey Bay, California”</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2z80f5nh</guid>
      <pubDate>Tue, 15 Jul 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Gou, Yuancong</name>
        <uri>https://orcid.org/0000-0001-6313-0564</uri>
      </author>
      <author>
        <name>Allen, Richard M</name>
        <uri>https://orcid.org/0000-0003-4293-9772</uri>
      </author>
      <author>
        <name>Zhu, Weiqiang</name>
        <uri>https://orcid.org/0000-0003-2889-1493</uri>
      </author>
      <author>
        <name>Taira, Taka’aki</name>
      </author>
      <author>
        <name>Chen, Li-Wei</name>
        <uri>https://orcid.org/0000-0002-9403-4505</uri>
      </author>
    </item>
    <item>
      <title>Leveraging Submarine DAS Arrays for Offshore Earthquake Early Warning: A Case Study in Monterey Bay, California</title>
      <link>https://escholarship.org/uc/item/1rd181nc</link>
      <description>Detecting offshore earthquakes in real time is challenging for traditional land-based seismic networks due to insufficient station coverage. Application of distributed acoustic sensing (DAS) to submarine cables has the potential to extend the reach of seismic networks and thereby improve real-time earthquake detection and earthquake early warning (EEW). We present a complete workflow of a modified point-source EEW algorithm, which includes a machine-learning-based model for P-and S-wave phase picking, a grid-search location method, and a locally calibrated empirical magnitude estimation equation. Examples are shown with offshore earthquakes from the SeaFOAM DAS project using a 52-km-long submarine cable in Monterey Bay, California, demonstrating the robustness of the proposed workflow. When comparing to the current onshore network, we can expect up to 6 s additional warning time for earthquakes in the offshore San Gregorio fault zone, representing a substantial improvement to...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1rd181nc</guid>
      <pubDate>Tue, 15 Jul 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Gou, Yuancong</name>
        <uri>https://orcid.org/0000-0001-6313-0564</uri>
      </author>
      <author>
        <name>Allen, Richard M</name>
        <uri>https://orcid.org/0000-0003-4293-9772</uri>
      </author>
      <author>
        <name>Zhu, Weiqiang</name>
        <uri>https://orcid.org/0000-0003-2889-1493</uri>
      </author>
      <author>
        <name>Taira, Taka’aki</name>
      </author>
      <author>
        <name>Chen, Li-Wei</name>
        <uri>https://orcid.org/0000-0002-9403-4505</uri>
      </author>
    </item>
    <item>
      <title>A Unified Analytical Model for Pressure Solution With Fully Coupled Diffusion and Reaction</title>
      <link>https://escholarship.org/uc/item/5fg9h0d5</link>
      <description>Abstract Geophysical models for pressure solution are typically developed for diffusion‐controlled or reaction‐controlled scenarios. We present a unified analytical model that considers fully coupled diffusion and reaction during pressure solution. The model recovers the diffusion‐controlled and reaction‐controlled models in the literature as specific limiting cases. When diffusion and reaction exhibit comparable influences, we validate the proposed model against independent numerical simulations. The proposed model is then employed in interpreting experimental measurements, demonstrating a better agreement compared to previous interpretations.
Plain Language Summary When solid grains are compressed against each other in an aqueous environment, minerals at the grain‐to‐grain contact dissolve more easily because of the higher stress. This process is known as pressure solution, which involves dissolution reactions and diffusive solute transport. We have developed an analytical model...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5fg9h0d5</guid>
      <pubDate>Tue, 24 Jun 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Wang, Ziyan</name>
        <uri>https://orcid.org/0000-0002-8941-8926</uri>
      </author>
      <author>
        <name>Gilbert, Benjamin</name>
      </author>
    </item>
    <item>
      <title>The Causes and Consequences of Ordovician Cooling</title>
      <link>https://escholarship.org/uc/item/17z1p4qm</link>
      <description>A long-term cooling trend through the Ordovician Period, from 487 to 443 Ma, is recorded by oxygen isotope data. Tropical ocean basins in the Early Ordovician were hot, which led to low oxygen concentrations in the surface ocean due to the temperature dependence of oxygen solubility. Elevated temperatures also increased metabolic demands such that hot shallow water environments had limited animal diversity as recorded by microbially dominated carbonates. As the oceans cooled through the Ordovician, animal biodiversity increased, leading to the Great Ordovician Biodiversification Event. The protracted nature of the cooling suggests that it was the product of progressive changes in tectonic boundary conditions. Low-latitude arc-continent collisions through this period may have increased global weatherability and decreased atmospheric CO2 levels. Additionally, decreasing continental arc magmatism could have lowered CO2 outgassing fluxes. The Ordovician long-term cooling trend culminated...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/17z1p4qm</guid>
      <pubDate>Wed, 18 Jun 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Bergmann, Kristin D</name>
      </author>
      <author>
        <name>Macdonald, Francis A</name>
        <uri>https://orcid.org/0000-0001-8416-4894</uri>
      </author>
      <author>
        <name>Swanson-Hysell, Nicholas L</name>
        <uri>https://orcid.org/0000-0003-3215-4648</uri>
      </author>
    </item>
    <item>
      <title>Constraints on Fe-Ca metasomatism in mineralized mantle rocks: Insights from in-situ geochemistry and thermodynamic modeling</title>
      <link>https://escholarship.org/uc/item/5015t7v3</link>
      <description>Ultramafic-hosted seafloor massive sulfide deposits have been reported in present-day oceanic settings for nearly thirty years. However, the development of comprehensive genetic models that account for deep-seated hydrothermal processes is largely hindered by the limited availability of seafloor observations and their reliance on large-scale geophysical studies. The Platta nappe (Swiss Alps) preserves a Jurassic hydrothermal system (the Marmorera-Cotschen Hydrothermal System; MCHS), where Cu-Fe-Co-Zn-Ni mineralization is associated with Fe-Ca silicates (ilvaite, hydrogarnet, and diopside). Petrographic analyses and thermodynamic modeling indicate that Fe-Ca metasomatism occurred between 300 and 360 °C and at low fO2 (from FMQ −6 to +1), likely coeval with early-stage serpentinization. The composition of Fe-Ca silicates (Co, Ni, and REE contents, measured by in-situ LA-ICP-MS) indicates fluid-rock interaction from an ultramafic-dominated system to an open-system, involving fluids...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5015t7v3</guid>
      <pubDate>Tue, 27 May 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Coltat, R</name>
      </author>
      <author>
        <name>Patten, CGC</name>
      </author>
      <author>
        <name>Padrón-Navarta, JA</name>
      </author>
      <author>
        <name>Hochscheid, F</name>
      </author>
      <author>
        <name>Ulrich, M</name>
      </author>
      <author>
        <name>Branquet, Y</name>
      </author>
      <author>
        <name>Boulvais, P</name>
      </author>
      <author>
        <name>Garrido, CJ</name>
      </author>
    </item>
    <item>
      <title>Experimental Pathways for Detecting Double Superionicity in Planetary Ices</title>
      <link>https://escholarship.org/uc/item/9399z630</link>
      <description>The ice giant planets Uranus and Neptune are assumed to contain large amounts of planetary ices such as water, methane, and ammonia. The properties of mixtures of such ices at the extreme pressures and temperatures of planetary interiors are not yet well understood. Ab initio computer simulations have predicted that a number of ices exhibit a hydrogen superionic state and a doubly superionic state. Since the latter state has not yet been generated with experiments, we outline here two possible pathways for reaching and detecting such a state with dynamic compression experiments. We suggest X-ray diffraction as the principal tool for detecting when the material becomes doubly superionic and the sublattice of one of the heavy nuclei melts. That would require a temperature of (Formula presented.) 3500 K and pressures greater than (Formula presented.) 200 GPa for H (Formula presented.) NO (Formula presented.), which we use as an example material here. Such conditions can be reached...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9399z630</guid>
      <pubDate>Wed, 21 May 2025 00:00:00 +0000</pubDate>
      <author>
        <name>de Villa, Kyla</name>
      </author>
      <author>
        <name>González‐Cataldo, Felipe</name>
      </author>
      <author>
        <name>Militzer, Burkhard</name>
      </author>
    </item>
    <item>
      <title>Tracing short-lived hydrothermal circulation systems and water–rock interactions around small-scale intrusions</title>
      <link>https://escholarship.org/uc/item/25w9r3h3</link>
      <description>Tracing short-lived hydrothermal circulation systems and water–rock interactions around small-scale intrusions</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/25w9r3h3</guid>
      <pubDate>Wed, 21 May 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Abbey, Alyssa L</name>
      </author>
      <author>
        <name>Randolph-Flagg, Noah</name>
      </author>
      <author>
        <name>de Villa, Kyla</name>
      </author>
      <author>
        <name>Kim, Sora L</name>
        <uri>https://orcid.org/0000-0002-4900-3101</uri>
      </author>
      <author>
        <name>Shuster, David L</name>
      </author>
    </item>
    <item>
      <title>Performance of bEPIC Through the 2024 M &amp;nbsp;7.0 Mendocino Earthquake Sequence</title>
      <link>https://escholarship.org/uc/item/85s4k1pk</link>
      <description>On 5 December 2024, an M 7.0 earthquake ruptured offshore of Cape Mendocino, California, generating felt shaking along the coast and prompting the issuance of earthquake early warning alerts and a tsunami warning. Contemporaneous to the earthquake sequence, bEPIC, an update to the ShakeAlert early warning algorithm Earthquake Point-source Integrated Code (EPIC), was undergoing development tests in real-time. The observed earthquake sequence provided a rich dataset of earthquakes in which we could test the performance of bEPIC. bEPIC improved epicenter estimates with an average 29.7 km reduction in location error compared to EPIC solutions for matched events. The improvement in location also improved per event magnitude estimates. Although EPIC on average overestimated the maximum magnitude of the earthquakes in the sequence by 0.37 magnitude units, bEPIC more closely aligned with our ground-truth catalog with a much lower overestimate of only 0.05 magnitude units. Despite including...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/85s4k1pk</guid>
      <pubDate>Wed, 7 May 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Williamson, Amy</name>
      </author>
      <author>
        <name>Lux, Angela</name>
      </author>
      <author>
        <name>Allen, Richard M</name>
        <uri>https://orcid.org/0000-0003-4293-9772</uri>
      </author>
    </item>
    <item>
      <title>Author Correction: A map of the rubisco biochemical landscape</title>
      <link>https://escholarship.org/uc/item/3nx3821h</link>
      <description>Correction to: Naturehttps://doi.org/10.1038/s41586-024-08455-0 Published online 22 January 2025 In the version of the article initially published, the affiliations of Hana A. Chang (Department of Plant and Microbial Biology, University of California Berkeley, Berkeley, CA, USA) and Ron Milo (Department of Plant and Environmental Sciences, Weizmann Institute of Science, Rehovot, Israel) were incorrect and have now been amended in the HTML and PDF versions of the article.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3nx3821h</guid>
      <pubDate>Thu, 1 May 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Prywes, Noam</name>
      </author>
      <author>
        <name>Phillips, Naiya R</name>
      </author>
      <author>
        <name>Oltrogge, Luke M</name>
      </author>
      <author>
        <name>Lindner, Sebastian</name>
      </author>
      <author>
        <name>Taylor-Kearney, Leah J</name>
      </author>
      <author>
        <name>Tsai, Yi-Chin Candace</name>
      </author>
      <author>
        <name>de Pins, Benoit</name>
      </author>
      <author>
        <name>Cowan, Aidan E</name>
      </author>
      <author>
        <name>Chang, Hana A</name>
      </author>
      <author>
        <name>Wang, Renée Z</name>
        <uri>https://orcid.org/0000-0003-3994-3244</uri>
      </author>
      <author>
        <name>Hall, Laina N</name>
      </author>
      <author>
        <name>Bellieny-Rabelo, Daniel</name>
      </author>
      <author>
        <name>Nisonoff, Hunter M</name>
      </author>
      <author>
        <name>Weissman, Rachel F</name>
      </author>
      <author>
        <name>Flamholz, Avi I</name>
      </author>
      <author>
        <name>Ding, David</name>
      </author>
      <author>
        <name>Bhatt, Abhishek Y</name>
      </author>
      <author>
        <name>Mueller-Cajar, Oliver</name>
      </author>
      <author>
        <name>Shih, Patrick M</name>
      </author>
      <author>
        <name>Milo, Ron</name>
      </author>
      <author>
        <name>Savage, David F</name>
      </author>
    </item>
    <item>
      <title>Daily microbial rhythms of the surface ocean interrupted by the new moon—a lipidomic study</title>
      <link>https://escholarship.org/uc/item/0zz2t0g4</link>
      <description>Lipids are essential biomolecules for cell physiology and are commonly used as biomarkers to elucidate biogeochemical processes over a large range of environments and timescales. Here, we use high-temporal-resolution lipidomic analysis to characterize the surface ocean community in the productive upwelling region overlying the Monterey Bay Canyon. We observed a strong diel signal with a drawdown of lipids at night and an increase during the day that seemed to correspond to wholesale removal of lipids from the surface ocean as opposed to internal metabolism. Individual lipid species were organized into coregulated groups that were interpreted as representing different phytoplankton guilds. Concentrations of long-chained triacylglycerols (TAGs) showed unique patterns over the course of five days. TAGs were used to estimate the amount of energy cycled through the surface ocean. These calculations revealed diurnal carbon cycling that was on scales comparable to net primary production....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0zz2t0g4</guid>
      <pubDate>Wed, 23 Apr 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Hwang, Jiwoon</name>
      </author>
      <author>
        <name>Hayward, Alexander</name>
      </author>
      <author>
        <name>Sofen, Laura E</name>
      </author>
      <author>
        <name>Pitz, Kathleen J</name>
      </author>
      <author>
        <name>Chavez, Francisco P</name>
      </author>
      <author>
        <name>Edwards, Bethanie R</name>
      </author>
    </item>
    <item>
      <title>Experimental determination of hydrogen isotopic equilibrium in the system H2O(l)-H2(g) from 3 to 90&amp;nbsp;°C</title>
      <link>https://escholarship.org/uc/item/95x7v4jp</link>
      <description>Molecular hydrogen (H2) is found in a variety of settings on and in the Earth from low-temperature sediments to hydrothermal vents, and is actively being considered as an energy resource for the transition to a green energy future. The hydrogen isotopic composition of H2, given as D/H ratios or δD, varies in nature by hundreds of per mil from&amp;nbsp;∼−800&amp;nbsp;‰ in hydrothermal and sedimentary systems to ∼+450&amp;nbsp;‰ in the stratosphere. This range reflects a variety of processes, including kinetic isotope effects associated with formation and destruction and equilibration with water, the latter proceeding at fast (order year) timescales at low temperatures (&amp;lt;100&amp;nbsp;°C). At isotopic equilibrium, the D/H fractionation factor between liquid water and hydrogen (DαH2O(l)-H2(g)) is a function of temperature and can thus be used as a geothermometer for H2 formation or re-equilibration temperatures. Multiple studies have produced theoretical calculations for hydrogen isotopic equilibrium...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/95x7v4jp</guid>
      <pubDate>Tue, 22 Apr 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Hochscheid, Flora</name>
      </author>
      <author>
        <name>Turner, Andrew C</name>
      </author>
      <author>
        <name>Lotem, Noam</name>
      </author>
      <author>
        <name>Bill, Markus</name>
        <uri>https://orcid.org/0000-0001-7002-2174</uri>
      </author>
      <author>
        <name>Stolper, Daniel A</name>
      </author>
    </item>
    <item>
      <title>The Sr isotope geochemistry of oceanic ultramafic-hosted mineralizations</title>
      <link>https://escholarship.org/uc/item/2k86c62t</link>
      <description>The source of metals involved in the formation of oceanic ultramafic-hosted hydrothermal Cu-Fe-Co-Zn-Ni mineralization remains poorly constrained. Here, we focus on a fossil ultramafic-hosted hydrothermal mineralized system preserved in the Platta nappe (SE Switzerland), where mantle rocks were exhumed along detachment faults to the seafloor during Jurassic rifting. The Cu-Fe-Co-Zn-Ni mineralization, associated with Fe-Ca-metasomatism (ilvaite-hydroandradite-diopside), represents an analogue of the root zone of present-day hydrothermal systems formed at mid-ocean ridges (e.g., Rainbow hydrothermal field at the Mid-Atlantic Ridge). We apply the Sr isotope geochemistry to Fe-Ca silicates and secondary, alteration products that include serpentinites, altered mafic and carbonated rocks to constrain the source(s) of metals and to characterize the plumbing system. The Fe-Ca silicates and carbonates have Sr isotope ratios close to that of Jurassic seawater, suggesting a near seafloor,...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2k86c62t</guid>
      <pubDate>Tue, 22 Apr 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Hochscheid, F</name>
      </author>
      <author>
        <name>Coltat, R</name>
      </author>
      <author>
        <name>Ulrich, M</name>
      </author>
      <author>
        <name>Munoz, M</name>
      </author>
      <author>
        <name>Manatschal, G</name>
      </author>
      <author>
        <name>Boulvais, P</name>
      </author>
    </item>
    <item>
      <title>Building better biochronology: New fossils and 40Ar/39Ar radioisotopic dates from Central Anatolia</title>
      <link>https://escholarship.org/uc/item/6bn262bj</link>
      <description>Türkiye's geographic position between Europe, Asia, and Africa gives it pivotal importance for understanding the local, interregional, and intercontinental dynamics of Neogene vertebrate evolution. Although rich in vertebrate fossil deposits spanning the Middle and Late Miocene, associated geochronology has been limited by the lack of available volcanic materials that allow radioisotopic dating and geochemical correlation. As a result, calibrating mammalian evolution has been largely restricted to the semicircular application of paleomagnetic inferences combined with temporally ill-constrained and geographically remote biochronological deductions. For example, fossils from three Greek localities and one Anatolian locality assigned to the primate genus &lt;i&gt;Ouranopithecus&lt;/i&gt; lack datable samples, leaving its ages poorly constrained. Chronological calibration based on the &lt;sup&gt;40&lt;/sup&gt;Ar/&lt;sup&gt;39&lt;/sup&gt;Ar results reported here demonstrates how a fauna-focused, precision geochronology...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6bn262bj</guid>
      <pubDate>Fri, 11 Apr 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Tholt, Andrew</name>
      </author>
      <author>
        <name>Başoğlu, Okşan</name>
      </author>
      <author>
        <name>Bektaş, Yener</name>
      </author>
      <author>
        <name>Bernor, Raymond</name>
      </author>
      <author>
        <name>Carlson, Joshua P</name>
        <uri>https://orcid.org/0009-0006-1857-2738</uri>
      </author>
      <author>
        <name>Dağ, Ömer</name>
      </author>
      <author>
        <name>Doğan, Uğur</name>
      </author>
      <author>
        <name>Erkman, Ahmet Cem</name>
      </author>
      <author>
        <name>Kaya, Ferhat</name>
      </author>
      <author>
        <name>Kaymakçı, Nuretdin</name>
      </author>
      <author>
        <name>Kırmızıoğlu, Pınar Gözlük</name>
      </author>
      <author>
        <name>Meijers, Maud JM</name>
      </author>
      <author>
        <name>Parıldar, Özge Kahya</name>
      </author>
      <author>
        <name>Pehlevan, Cesur</name>
      </author>
      <author>
        <name>Şimşek, Emrah</name>
      </author>
      <author>
        <name>White, Tim</name>
      </author>
      <author>
        <name>Renne, Paul</name>
        <uri>https://orcid.org/0000-0003-1769-5235</uri>
      </author>
    </item>
    <item>
      <title>Co‐Occurring Atmospheric Features and Their Contributions to Precipitation Extremes</title>
      <link>https://escholarship.org/uc/item/5161h0xn</link>
      <description>Abstract Object‐based identification algorithms for atmospheric features are commonly utilized to attribute global precipitation. This study employs a systematic approach to examine feature co‐occurrences and their relationships to mean and extreme precipitation. Four features are identified using existing data sets for atmospheric rivers (ARs), mesoscale convective systems (MCSs), low‐pressure systems (LPSs), and fronts (FTs). Often, a single atmospheric phenomenon satisfies the criteria set by multiple feature identification algorithms, yielding an association between precipitation and multiple features. Over the extra‐tropics, the number of features attributed to a single event typically increases with precipitation intensity. Over two‐thirds of the precipitation is from co‐occurring features, with a considerable fraction related to AR‐FT co‐occurrences. Over the tropics, about one‐quarter of precipitation is associated with co‐occurring features, with LPS‐MCS co‐occurrences...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5161h0xn</guid>
      <pubDate>Thu, 10 Apr 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Tsai, Wei‐Ming</name>
      </author>
      <author>
        <name>Duan, Suqin</name>
      </author>
      <author>
        <name>O’Brien, Travis A</name>
      </author>
      <author>
        <name>Catto, Jennifer L</name>
      </author>
      <author>
        <name>Ullrich, Paul A</name>
        <uri>https://orcid.org/0000-0003-4118-4590</uri>
      </author>
      <author>
        <name>Zhou, Yang</name>
        <uri>https://orcid.org/0000-0003-2835-4081</uri>
      </author>
      <author>
        <name>Leung, L Ruby</name>
      </author>
      <author>
        <name>Feng, Zhe</name>
      </author>
      <author>
        <name>Boos, William R</name>
        <uri>https://orcid.org/0000-0001-9076-3551</uri>
      </author>
      <author>
        <name>Suhas, DL</name>
      </author>
      <author>
        <name>Ahmed, Fiaz</name>
      </author>
      <author>
        <name>Neelin, J David</name>
      </author>
    </item>
    <item>
      <title>Earthquake Early Warning: Advances, Scientific Challenges, and Societal Needs</title>
      <link>https://escholarship.org/uc/item/7226f497</link>
      <description>Earthquake Early Warning: Advances, Scientific Challenges, and Societal Needs</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7226f497</guid>
      <pubDate>Wed, 9 Apr 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Allen, Richard M</name>
        <uri>https://orcid.org/0000-0003-4293-9772</uri>
      </author>
      <author>
        <name>Melgar, Diego</name>
      </author>
    </item>
    <item>
      <title>Ancient ocean coastal deposits imaged on Mars</title>
      <link>https://escholarship.org/uc/item/76x357qg</link>
      <description>The northern lowlands of early Mars could have contained a significant quantity of liquid water. However, the ocean hypothesis remains controversial due to the lack of conclusive evidence from the Martian subsurface. We use data from the Zhurong Rover Penetrating Radar on the southern Utopia Planitia to identify subsurface dipping reflectors indicative of an ancient prograding shoreline. The reflectors dip unidirectionally with inclinations in the range 6° to 20° and are imaged to a thickness of 10 to 35 m along an uninterrupted 1.3 km northward shoreline-perpendicular traverse. The consistent dip inclinations, absence of dissection by fluvial channels along the extended traverse, and low permittivity of the sediments are consistent with terrestrial coastal deposits-and discount fluvial, aeolian, or magmatic origins favored elsewhere on Mars. The structure, thickness, and length of the section support voluminous supply of onshore sediments into a large body of water, rather than...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/76x357qg</guid>
      <pubDate>Thu, 3 Apr 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Li, Jianhui</name>
      </author>
      <author>
        <name>Liu, Hai</name>
      </author>
      <author>
        <name>Meng, Xu</name>
      </author>
      <author>
        <name>Duan, Diwen</name>
      </author>
      <author>
        <name>Lu, Haijing</name>
      </author>
      <author>
        <name>Zhang, Jinhai</name>
      </author>
      <author>
        <name>Zhang, Fengshou</name>
      </author>
      <author>
        <name>Elsworth, Derek</name>
      </author>
      <author>
        <name>Cardenas, Benjamin T</name>
      </author>
      <author>
        <name>Manga, Michael</name>
      </author>
      <author>
        <name>Zhou, Bin</name>
      </author>
      <author>
        <name>Fang, Guangyou</name>
      </author>
    </item>
    <item>
      <title>Marine sulphate captures a Paleozoic transition to a modern terrestrial weathering environment</title>
      <link>https://escholarship.org/uc/item/3sz798g0</link>
      <description>The triple oxygen isotope composition of sulphate minerals has been used to constrain the evolution of Earth’s surface environment (e.g., pO2, pCO2 and gross primary productivity) throughout the Proterozoic Eon. This approach presumes the incorporation of atmospheric O2 atoms into riverine sulphate via the oxidative weathering of pyrite. However, this is not borne out in recent geological or modern sulphate records, where an atmospheric signal is imperceptible and where terrestrial pyrite weathering occurs predominantly in bedrock fractures that are physically more removed from atmospheric O2. To better define the transition from a Proterozoic to a modern-like weathering regime, here we present new measurements from twelve marine evaporite basins spanning the Phanerozoic. These data display a step-like transition in the triple oxygen isotope composition of evaporite sulphate during the mid-Paleozoic (420 to 387.7 million years ago). We propose that the evolution of early root...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3sz798g0</guid>
      <pubDate>Thu, 3 Apr 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Waldeck, Anna R</name>
      </author>
      <author>
        <name>Olson, Haley C</name>
      </author>
      <author>
        <name>Crockford, Peter W</name>
      </author>
      <author>
        <name>Couture, Abby M</name>
      </author>
      <author>
        <name>Cowie, Benjamin R</name>
      </author>
      <author>
        <name>Hodgin, Eben B</name>
      </author>
      <author>
        <name>Bergmann, Kristin D</name>
      </author>
      <author>
        <name>Dewing, Keith</name>
      </author>
      <author>
        <name>Grasby, Stephen E</name>
      </author>
      <author>
        <name>Clark, Ryan J</name>
      </author>
      <author>
        <name>Macdonald, Francis A</name>
        <uri>https://orcid.org/0000-0001-8416-4894</uri>
      </author>
      <author>
        <name>Johnston, David T</name>
      </author>
    </item>
    <item>
      <title>A new method for diagnosing effective radiative forcing from aerosol–cloud interactions in climate models</title>
      <link>https://escholarship.org/uc/item/54w4j6z2</link>
      <description>Abstract. Aerosol–cloud interactions (ACIs) are a leading source of uncertainty in estimates of the historical effective radiative forcing (ERF). One reason for this uncertainty is the difficulty in estimating the ERF from aerosol–cloud interactions (ERFaci) in climate models, which typically requires multiple calls to the radiation code. Most commonly used methods also cannot disentangle the contributions from different processes to ERFaci. Here, we develop a new, computationally efficient method for estimating the shortwave (SW) ERFaci from liquid clouds using histograms of monthly averaged cloud fraction partitioned by cloud droplet effective radius (re) and liquid water path (LWP). Multiplying the histograms with SW cloud radiative kernels gives the total SW ERFaci from liquid clouds, which can be decomposed into contributions from the Twomey effect, LWP adjustments, and cloud fraction (CF) adjustments. We test the method with data from five CMIP6-era models, using the Moderate...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/54w4j6z2</guid>
      <pubDate>Fri, 14 Mar 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Duran, Brandon M</name>
        <uri>https://orcid.org/0000-0001-5427-8700</uri>
      </author>
      <author>
        <name>Wall, Casey J</name>
      </author>
      <author>
        <name>Lutsko, Nicholas J</name>
      </author>
      <author>
        <name>Michibata, Takuro</name>
      </author>
      <author>
        <name>Ma, Po-Lun</name>
      </author>
      <author>
        <name>Qin, Yi</name>
      </author>
      <author>
        <name>Duffy, Margaret L</name>
      </author>
      <author>
        <name>Medeiros, Brian</name>
      </author>
      <author>
        <name>Debolskiy, Matvey</name>
      </author>
    </item>
    <item>
      <title>Factors influencing underrepresented geoscientists' decisions to accept or decline faculty job offers in the US</title>
      <link>https://escholarship.org/uc/item/4hj0x8g2</link>
      <description>Abstract: 

          Many geoscience departments in the United States (US) are working to recruit faculty from underrepresented groups. However, there is little information about how hiring practices are perceived by candidates. Here we address this gap by interviewing 19 geoscientists who identify as an underrepresented race, ethnicity, or gender who recently declined a tenure-track faculty job offer in the US about their faculty job searches, with an emphasis on their decisions to accept or decline an offer. We find that many participants experienced hiring practices inconsistent with existing recommendations to increase faculty diversity, and some participants were subject to uncivilized, even potentially discriminatory, practices. Therefore, we leverage our results to provide actionable recommendations for improving faculty recruitment efforts. We highlight that departments may doubly benefit from improving their culture: in addition to benefiting current members, it may...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4hj0x8g2</guid>
      <pubDate>Wed, 12 Mar 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Duffy, Margaret L</name>
      </author>
      <author>
        <name>Barnes, Liza Y</name>
      </author>
      <author>
        <name>Wirz, Christopher D</name>
      </author>
      <author>
        <name>Ranganathan, Meghana</name>
      </author>
      <author>
        <name>Freilich, Mara A</name>
      </author>
      <author>
        <name>Freese, Lyssa M</name>
      </author>
      <author>
        <name>Lalk, Ellen</name>
      </author>
      <author>
        <name>Wilcots, Julia</name>
      </author>
    </item>
    <item>
      <title>Atmospheric River Frequency‐Category Characteristics Shape U.S. West Coast Runoff</title>
      <link>https://escholarship.org/uc/item/7dt8d88s</link>
      <description>Abstract This study investigates the factors influencing runoff response to atmospheric rivers (ARs) over the U.S. West Coast. We focused on runoff time series variations impacted by AR characteristics (e.g., category and frequency) and land preconditions during Northern Hemisphere cool seasons in the period of 1940–2023. Results show that high‐category ARs significantly increase local runoff with higher hourly precipitation rates leading to a greater incremental rate and peak runoff. Extreme runoff increases greatly with the AR category with an increase rate up to 12.5 times stronger than non‐extreme runoff. Besides the AR category, land preconditions such as soil moisture and snowpack also play crucial roles in modulating runoff response. We found that runoff induced by weak‐category ARs is more sensitive to land preconditions than high‐category ARs, with high peak runoff occurring when soil is nearly saturated. Additionally, more than 50% of high‐peak‐runoff events in snow‐covered...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7dt8d88s</guid>
      <pubDate>Tue, 11 Mar 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Zhou, Yang</name>
        <uri>https://orcid.org/0000-0003-2835-4081</uri>
      </author>
      <author>
        <name>North, Joshua S</name>
        <uri>https://orcid.org/0000-0001-7631-8021</uri>
      </author>
      <author>
        <name>Rhoades, Alan M</name>
        <uri>https://orcid.org/0000-0003-3723-2422</uri>
      </author>
      <author>
        <name>Tao, Jing</name>
        <uri>https://orcid.org/0000-0002-4009-2910</uri>
      </author>
      <author>
        <name>Rudisill, William</name>
      </author>
      <author>
        <name>Risser, Mark D</name>
        <uri>https://orcid.org/0000-0003-1956-1783</uri>
      </author>
      <author>
        <name>Collins, William D</name>
        <uri>https://orcid.org/0000-0002-4463-9848</uri>
      </author>
    </item>
    <item>
      <title>Efficient hybrid numerical modeling of the seismic wavefield in the presence of solid-fluid boundaries</title>
      <link>https://escholarship.org/uc/item/01r1f2qt</link>
      <description>Applying full-waveform methods to image small-scale structures of geophysical interest buried within the Earth requires the computation of the seismic wavefield over large distances compared to the target wavelengths. This represents a considerable computational cost when using state-of-the-art numerical integration of the equations of motion in three-dimensional earth models. “Box Tomography” is a hybrid method that breaks up the wavefield computation into three parts, only one of which needs to be iterated for each model update, significantly saving computational time. To deploy this method in remote regions containing a fluid-solid boundary, one needs to construct artificial sources that confine the seismic wavefield within a small region that straddles this boundary. The difficulty arises from the need to combine the solid-fluid coupling with a hybrid numerical simulation in this region. Here, we report a reconciliation of different displacement potential expressions used...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/01r1f2qt</guid>
      <pubDate>Mon, 3 Mar 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Lyu, Chao</name>
      </author>
      <author>
        <name>Romanowicz, Barbara</name>
        <uri>https://orcid.org/0000-0002-6208-6044</uri>
      </author>
      <author>
        <name>Zhao, Liang</name>
      </author>
      <author>
        <name>Masson, Yder</name>
      </author>
    </item>
    <item>
      <title>Phase separation of planetary ices explains nondipolar magnetic fields of Uranus and Neptune</title>
      <link>https://escholarship.org/uc/item/1zv9w0bf</link>
      <description>The Voyager spacecraft discovered that the ice giants Uranus and Neptune have nondipolar magnetic fields, defying expectations that a thick interior layer of planetary ices would generate strong dipolar fields. Stanley and Bloxham showed that nondipolar fields emerge if the magnetic field is only generated in a thin outer layer. However, the origin and composition of this dynamo active layer has so far remained elusive. Here, we show with ab initio computer simulations that a mixture of H&lt;sub&gt;2&lt;/sub&gt;O, CH&lt;sub&gt;4&lt;/sub&gt;, and NH&lt;sub&gt;3&lt;/sub&gt; will phase separate under the pressure-temperature condition in the interiors of Uranus and Neptune, forming a H&lt;sub&gt;2&lt;/sub&gt;O-dominated fluid in the upper mantle and a CH&lt;sub&gt;4&lt;/sub&gt;-NH&lt;sub&gt;3&lt;/sub&gt; mixture below. We further demonstrate that with increasing pressure, the CH&lt;sub&gt;4&lt;/sub&gt;-NH&lt;sub&gt;3&lt;/sub&gt; mixture becomes increasingly hydrogen depleted as it assumes the state of a polymeric C-N-H fluid. Since the amount of hydrogen loss increases with...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1zv9w0bf</guid>
      <pubDate>Fri, 28 Feb 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Militzer, Burkhard</name>
        <uri>https://orcid.org/0000-0002-7092-5629</uri>
      </author>
    </item>
    <item>
      <title>A map of the rubisco biochemical landscape</title>
      <link>https://escholarship.org/uc/item/71q1b4jn</link>
      <description>Rubisco is the primary CO2-fixing enzyme of the biosphere1, yet it has slow kinetics2. The roles of evolution and chemical mechanism in constraining its biochemical function remain debated3,4. Engineering efforts aimed at adjusting the biochemical parameters of rubisco have largely failed5, although recent results indicate that the functional potential of rubisco has a wider scope than previously known6. Here we developed a massively parallel assay, using an engineered Escherichia coli7 in which enzyme activity is coupled to growth, to systematically map the sequence–function landscape of rubisco. Composite assay of more than 99% of single-amino acid mutants versus CO2 concentration enabled inference of enzyme velocity and apparent CO2 affinity parameters for thousands of substitutions. This approach identified many highly conserved positions that tolerate mutation and rare mutations that improve CO2 affinity. These data indicate that non-trivial biochemical changes are readily...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/71q1b4jn</guid>
      <pubDate>Thu, 27 Feb 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Prywes, Noam</name>
      </author>
      <author>
        <name>Phillips, Naiya R</name>
      </author>
      <author>
        <name>Oltrogge, Luke M</name>
      </author>
      <author>
        <name>Lindner, Sebastian</name>
      </author>
      <author>
        <name>Taylor-Kearney, Leah J</name>
      </author>
      <author>
        <name>Tsai, Yi-Chin Candace</name>
      </author>
      <author>
        <name>de Pins, Benoit</name>
      </author>
      <author>
        <name>Cowan, Aidan E</name>
      </author>
      <author>
        <name>Chang, Hana A</name>
      </author>
      <author>
        <name>Wang, Renée Z</name>
        <uri>https://orcid.org/0000-0003-3994-3244</uri>
      </author>
      <author>
        <name>Hall, Laina N</name>
      </author>
      <author>
        <name>Bellieny-Rabelo, Daniel</name>
      </author>
      <author>
        <name>Nisonoff, Hunter M</name>
      </author>
      <author>
        <name>Weissman, Rachel F</name>
      </author>
      <author>
        <name>Flamholz, Avi I</name>
      </author>
      <author>
        <name>Ding, David</name>
      </author>
      <author>
        <name>Bhatt, Abhishek Y</name>
      </author>
      <author>
        <name>Mueller-Cajar, Oliver</name>
      </author>
      <author>
        <name>Shih, Patrick M</name>
      </author>
      <author>
        <name>Milo, Ron</name>
      </author>
      <author>
        <name>Savage, David F</name>
      </author>
    </item>
    <item>
      <title>What we can learn about Mars from the magnetism of returned samples</title>
      <link>https://escholarship.org/uc/item/6n43v3wx</link>
      <description>The Red Planet is a magnetic planet. The Martian crust contains strong magnetization from a core dynamo that likely was active during the Noachian period when the surface may have been habitable. The evolution of the dynamo may have played a central role in the evolution of the early atmosphere and the planet's transition to the current cold and dry state. However, the nature and history of the dynamo and crustal magnetization are poorly understood given the lack of well-preserved, oriented, ancient samples with geologic context available for laboratory study. Here, we describe how magnetic measurements of returned samples could transform our understanding of six key unknowns about Mars' planetary evolution and habitability. Such measurements could i) determine the history of the Martian dynamo field's intensity; ii) determine the history of the Martian dynamo field's direction; iii) test the hypothesis that Mars experienced plate tectonics or true polar wander; iv) constrain...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6n43v3wx</guid>
      <pubDate>Fri, 31 Jan 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Weiss, Benjamin P</name>
      </author>
      <author>
        <name>Mansbach, Elias N</name>
      </author>
      <author>
        <name>Maurel, Clara</name>
      </author>
      <author>
        <name>Sprain, Courtney J</name>
      </author>
      <author>
        <name>Swanson-Hysell, Nicholas L</name>
        <uri>https://orcid.org/0000-0003-3215-4648</uri>
      </author>
      <author>
        <name>Williams, Wyn</name>
      </author>
    </item>
    <item>
      <title>PyIRoGlass: An open-source, Bayesian MCMC algorithm for fitting baselines to FTIR spectra of basaltic-andesitic glasses</title>
      <link>https://escholarship.org/uc/item/9151x8zk</link>
      <description>Quantifying volatile concentrations in magmas is critical for understanding magma storage, phase equilibria, and eruption processes. We present PyIRoGlass, an open-source Python package for quantifying concentrations of H2O and CO2 species in the transmission FTIR spectra of basaltic to andesitic glasses. We leverage a dataset of natural melt inclusions and back-arc basin basalts with volatiles below detection to delineate the fundamental shape and variability of the baseline underlying the CO23− and H2Om,1635 peaks, in the mid-infrared region. All Beer-Lambert Law parameters are examined to quantify associated uncertainties. PyIRoGlass employs Bayesian inference and Markov Chain Monte Carlo sampling to fit all probable baselines and peaks, solving for best-fit parameters and capturing covariance to offer robust uncertainty estimates. Results from PyIRoGlass agree with independent analyses of experimental devolatilized glasses (within 6 %) and interlaboratory standards (10 % for...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9151x8zk</guid>
      <pubDate>Wed, 29 Jan 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Shi, Sarah</name>
        <uri>https://orcid.org/0009-0004-8997-7287</uri>
      </author>
      <author>
        <name>Towbin, William Henry</name>
      </author>
      <author>
        <name>Plank, Terry</name>
      </author>
      <author>
        <name>Barth, Anna</name>
      </author>
      <author>
        <name>Rasmussen, Daniel</name>
      </author>
      <author>
        <name>Moussallam, Yves</name>
      </author>
      <author>
        <name>Lee, Hyun Joo</name>
      </author>
      <author>
        <name>Menke, William</name>
      </author>
    </item>
    <item>
      <title>MIBiG 4.0: advancing biosynthetic gene cluster curation through global collaboration</title>
      <link>https://escholarship.org/uc/item/33w736t3</link>
      <description>Specialized or secondary metabolites are small molecules of biological origin, often showing potent biological activities with applications in agriculture, engineering and medicine. Usually, the biosynthesis of these natural products is governed by sets of co-regulated and physically clustered genes known as biosynthetic gene clusters (BGCs). To share information about BGCs in a standardized and machine-readable way, the Minimum Information about a Biosynthetic Gene cluster (MIBiG) data standard and repository was initiated in 2015. Since its conception, MIBiG has been regularly updated to expand data coverage and remain up to date with innovations in natural product research. Here, we describe MIBiG version 4.0, an extensive update to the data repository and the underlying data standard. In a massive community annotation effort, 267 contributors performed 8304 edits, creating 557 new entries and modifying 590 existing entries, resulting in a new total of 3059 curated entries...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/33w736t3</guid>
      <pubDate>Wed, 15 Jan 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Zdouc, Mitja M</name>
      </author>
      <author>
        <name>Blin, Kai</name>
      </author>
      <author>
        <name>Louwen, Nico LL</name>
      </author>
      <author>
        <name>Navarro, Jorge</name>
      </author>
      <author>
        <name>Loureiro, Catarina</name>
      </author>
      <author>
        <name>Bader, Chantal D</name>
      </author>
      <author>
        <name>Bailey, Constance B</name>
      </author>
      <author>
        <name>Barra, Lena</name>
      </author>
      <author>
        <name>Booth, Thomas J</name>
      </author>
      <author>
        <name>Bozhüyük, Kenan AJ</name>
      </author>
      <author>
        <name>Cediel-Becerra, José DD</name>
      </author>
      <author>
        <name>Charlop-Powers, Zachary</name>
      </author>
      <author>
        <name>Chevrette, Marc G</name>
      </author>
      <author>
        <name>Chooi, Yit Heng</name>
      </author>
      <author>
        <name>D’Agostino, Paul M</name>
      </author>
      <author>
        <name>de Rond, Tristan</name>
      </author>
      <author>
        <name>Del Pup, Elena</name>
      </author>
      <author>
        <name>Duncan, Katherine R</name>
      </author>
      <author>
        <name>Gu, Wenjia</name>
      </author>
      <author>
        <name>Hanif, Novriyandi</name>
      </author>
      <author>
        <name>Helfrich, Eric JN</name>
      </author>
      <author>
        <name>Jenner, Matthew</name>
      </author>
      <author>
        <name>Katsuyama, Yohei</name>
      </author>
      <author>
        <name>Korenskaia, Aleksandra</name>
      </author>
      <author>
        <name>Krug, Daniel</name>
      </author>
      <author>
        <name>Libis, Vincent</name>
      </author>
      <author>
        <name>Lund, George A</name>
      </author>
      <author>
        <name>Mantri, Shrikant</name>
      </author>
      <author>
        <name>Morgan, Kalindi D</name>
      </author>
      <author>
        <name>Owen, Charlotte</name>
      </author>
      <author>
        <name>Phan, Chin-Soon</name>
      </author>
      <author>
        <name>Philmus, Benjamin</name>
      </author>
      <author>
        <name>Reitz, Zachary L</name>
      </author>
      <author>
        <name>Robinson, Serina L</name>
      </author>
      <author>
        <name>Singh, Kumar Saurabh</name>
      </author>
      <author>
        <name>Teufel, Robin</name>
      </author>
      <author>
        <name>Tong, Yaojun</name>
      </author>
      <author>
        <name>Tugizimana, Fidele</name>
      </author>
      <author>
        <name>Ulanova, Dana</name>
      </author>
      <author>
        <name>Winter, Jaclyn M</name>
      </author>
      <author>
        <name>Aguilar, César</name>
      </author>
      <author>
        <name>Akiyama, Daniel Y</name>
      </author>
      <author>
        <name>Al-Salihi, Suhad AA</name>
      </author>
      <author>
        <name>Alanjary, Mohammad</name>
      </author>
      <author>
        <name>Alberti, Fabrizio</name>
      </author>
      <author>
        <name>Aleti, Gajender</name>
      </author>
      <author>
        <name>Alharthi, Shumukh A</name>
      </author>
      <author>
        <name>Rojo, Mariela Y Arias</name>
      </author>
      <author>
        <name>Arishi, Amr A</name>
      </author>
      <author>
        <name>Augustijn, Hannah E</name>
      </author>
      <author>
        <name>Avalon, Nicole E</name>
      </author>
      <author>
        <name>Avelar-Rivas, J Abraham</name>
      </author>
      <author>
        <name>Axt, Kyle K</name>
      </author>
      <author>
        <name>Barbieri, Hellen B</name>
      </author>
      <author>
        <name>Barbosa, Julio Cesar J</name>
      </author>
      <author>
        <name>Segato, Lucas Gabriel Barboza</name>
      </author>
      <author>
        <name>Barrett, Susanna E</name>
      </author>
      <author>
        <name>Baunach, Martin</name>
      </author>
      <author>
        <name>Beemelmanns, Christine</name>
      </author>
      <author>
        <name>Beqaj, Dardan</name>
      </author>
      <author>
        <name>Berger, Tim</name>
      </author>
      <author>
        <name>Bernaldo-Agüero, Jordan</name>
      </author>
      <author>
        <name>Bettenbühl, Sandra M</name>
      </author>
      <author>
        <name>Bielinski, Vincent A</name>
      </author>
      <author>
        <name>Biermann, Friederike</name>
      </author>
      <author>
        <name>Borges, Ricardo M</name>
      </author>
      <author>
        <name>Borriss, Rainer</name>
      </author>
      <author>
        <name>Breitenbach, Milena</name>
      </author>
      <author>
        <name>Bretscher, Kevin M</name>
      </author>
      <author>
        <name>Brigham, Michael W</name>
      </author>
      <author>
        <name>Buedenbender, Larissa</name>
      </author>
      <author>
        <name>Bulcock, Brodie W</name>
      </author>
      <author>
        <name>Cano-Prieto, Carolina</name>
      </author>
      <author>
        <name>Capela, João</name>
      </author>
      <author>
        <name>Carrion, Victor J</name>
      </author>
      <author>
        <name>Carter, Riley S</name>
      </author>
      <author>
        <name>Castelo-Branco, Raquel</name>
      </author>
      <author>
        <name>Castro-Falcón, Gabriel</name>
      </author>
      <author>
        <name>Chagas, Fernanda O</name>
      </author>
      <author>
        <name>Charria-Girón, Esteban</name>
      </author>
      <author>
        <name>Chaudhri, Ayesha Ahmed</name>
      </author>
      <author>
        <name>Chaudhry, Vasvi</name>
      </author>
      <author>
        <name>Choi, Hyukjae</name>
      </author>
      <author>
        <name>Choi, Yukyung</name>
      </author>
      <author>
        <name>Choupannejad, Roya</name>
      </author>
      <author>
        <name>Chromy, Jakub</name>
      </author>
      <author>
        <name>Donahey, Melinda S Chue</name>
      </author>
      <author>
        <name>Collemare, Jérôme</name>
      </author>
      <author>
        <name>Connolly, Jack A</name>
      </author>
      <author>
        <name>Creamer, Kaitlin E</name>
        <uri>https://orcid.org/0000-0002-0666-2107</uri>
      </author>
      <author>
        <name>Crüsemann, Max</name>
      </author>
      <author>
        <name>Cruz, Andres Arredondo</name>
      </author>
      <author>
        <name>Cumsille, Andres</name>
      </author>
      <author>
        <name>Dallery, Jean-Felix</name>
      </author>
      <author>
        <name>Damas-Ramos, Luis Caleb</name>
      </author>
      <author>
        <name>Damiani, Tito</name>
      </author>
      <author>
        <name>de Kruijff, Martinus</name>
      </author>
      <author>
        <name>Martín, Belén Delgado</name>
      </author>
      <author>
        <name>Della Sala, Gerardo</name>
      </author>
      <author>
        <name>Dillen, Jelle</name>
      </author>
    </item>
    <item>
      <title>The Role of Southeast Asian Island Topography on Indo‐Pacific Climate and Silicate Weathering</title>
      <link>https://escholarship.org/uc/item/5sc2k0z7</link>
      <description>The geography of the Southeast Asian Islands (SEAI) has changed over the last 15 million years, as a result of tectonic processes contributing to both increased land area and high topography. The presence of the additional land area has been postulated to enhance convective rainfall, facilitating both increased silicate weathering and the development of the modern-day Walker circulation. Using an Earth System Model in conjunction with a climate-silicate weathering model, we argue instead for a significant role of SEAI topography for both effects. SEAI topography increases orographic rainfall over land, through intercepting moist Asian-Australian monsoon winds and enhancing land-sea breezes. Large-scale atmospheric uplift over the SEAI region increases by ∼14% as a consequence of increased rainfall over the SEAI and enhancement through dynamical ocean-atmosphere feedback. The atmospheric zonal overturning circulation over the Indo-Pacific increases modestly arising from dynamical...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5sc2k0z7</guid>
      <pubDate>Thu, 9 Jan 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Chiang, John CH</name>
        <uri>https://orcid.org/0000-0001-7723-9544</uri>
      </author>
      <author>
        <name>Maffre, Pierre</name>
      </author>
      <author>
        <name>Swanson‐Hysell, Nicholas L</name>
      </author>
      <author>
        <name>Macdonald, Francis A</name>
        <uri>https://orcid.org/0000-0001-8416-4894</uri>
      </author>
    </item>
    <item>
      <title>The effect of Pliocene regional climate changes on silicate weathering: a potential amplifier of Pliocene-Pleistocene cooling</title>
      <link>https://escholarship.org/uc/item/4g89m414</link>
      <description>Abstract. The warmer early Pliocene climate featured changes to global sea surface temperature (SST) patterns, namely a reduction to the equator-pole gradient and to the east-west SST gradient in the tropical Pacific, the so-called “permanent El Niño”. Here we investigate the consequences of the SST changes to silicate weathering and thus to atmospheric CO2 on geological timescales. Different SST patterns than today imply regional modifications of the hydrological cycle that directly affects continental silicate weathering in particular over tropical “hotspots” of weathering such as the Maritime continent, thus leading to a “weatherability pattern effect”. We explore the impact of Pliocene SST changes on weathering using climate model and silicate weathering model simulations, and deduce CO2 and temperature at C cycle equilibrium between solid Earth degassing and silicate weathering. In general, we find large regional increases and decreases to weathering fluxes that largely cancel...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4g89m414</guid>
      <pubDate>Thu, 9 Jan 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Maffre, Pierre</name>
      </author>
      <author>
        <name>Chiang, John CH</name>
        <uri>https://orcid.org/0000-0001-7723-9544</uri>
      </author>
      <author>
        <name>Swanson-Hysell, Nicholas L</name>
        <uri>https://orcid.org/0000-0003-3215-4648</uri>
      </author>
    </item>
    <item>
      <title>Regional tropical rainfall shifts under global warming: an energetic perspective</title>
      <link>https://escholarship.org/uc/item/2n38j1bc</link>
      <description>Abstract: 

               Future climate simulations feature pronounced spatial shifts in the structure of tropical rainfall. We apply a novel atmospheric energy flux analysis to diagnose late 21st century tropical rainfall shifts in a large ensemble of simulations of 21st century climate. The method reconstructs 2D spatial changes in rainfall based on horizontal shifts in the lines of zero meridional and zonal divergent energy flux, called the energy flux equator (EFE) and energy flux prime meridian (EFPM), respectively. Two main sources of future atmospheric energy flux changes, and hence rainfall shifts, are identified by the analysis: the high-latitude North Atlantic due to a weakened Atlantic Meridional Overturning Circulation that shifts tropical rainfall southwards over the greater Tropical Atlantic sector and eastern Pacific; and the eastern tropical Pacific due to a permanent El-Niño-like response that produces zonal shifts over the Maritime Continent and South America....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2n38j1bc</guid>
      <pubDate>Thu, 9 Jan 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Nicknish, Paul A</name>
      </author>
      <author>
        <name>Chiang, John CH</name>
        <uri>https://orcid.org/0000-0001-7723-9544</uri>
      </author>
      <author>
        <name>Hu, Aixue</name>
      </author>
      <author>
        <name>Boos, William R</name>
        <uri>https://orcid.org/0000-0001-9076-3551</uri>
      </author>
    </item>
    <item>
      <title>Diverse microbiome functions, limited temporal variation and substantial genomic conservation within sedimentary and granite rock deep underground research laboratories.</title>
      <link>https://escholarship.org/uc/item/5pp6v0nf</link>
      <description>BACKGROUND: Underground research laboratories (URLs) provide a window on the deep biosphere and enable investigation of potential microbial impacts on nuclear waste, CO2 and H2 stored in the subsurface. We carried out the first multi-year study of groundwater microbiomes sampled from defined intervals between 140 and 400&amp;nbsp;m below the surface of the Horonobe and Mizunami URLs, Japan. RESULTS: We reconstructed draft genomes for &amp;gt; 90% of all organisms detected over a four year period. The Horonobe and Mizunami microbiomes are dissimilar, likely because the Mizunami URL is hosted in granitic rock and the Horonobe URL in sedimentary rock. Despite this, hydrogen metabolism, rubisco-based CO2 fixation, reduction of nitrogen compounds and sulfate reduction are well represented functions in microbiomes from both URLs, although methane metabolism is more prevalent at the organic- and CO2-rich Horonobe URL. High fluid flow zones and proximity to subsurface tunnels select for candidate...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5pp6v0nf</guid>
      <pubDate>Fri, 3 Jan 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Amano, Yuki</name>
      </author>
      <author>
        <name>Sachdeva, Rohan</name>
      </author>
      <author>
        <name>Gittins, Daniel</name>
      </author>
      <author>
        <name>Anantharaman, Karthik</name>
      </author>
      <author>
        <name>Lei, Shufei</name>
      </author>
      <author>
        <name>Valentin-Alvarado, Luis</name>
      </author>
      <author>
        <name>Diamond, Spencer</name>
      </author>
      <author>
        <name>Beppu, Hikari</name>
      </author>
      <author>
        <name>Iwatsuki, Teruki</name>
      </author>
      <author>
        <name>Mochizuki, Akihito</name>
      </author>
      <author>
        <name>Miyakawa, Kazuya</name>
      </author>
      <author>
        <name>Ishii, Eiichi</name>
      </author>
      <author>
        <name>Murakami, Hiroaki</name>
      </author>
      <author>
        <name>Jaffe, Alexander</name>
      </author>
      <author>
        <name>Castelle, Cindy</name>
      </author>
      <author>
        <name>Lavy, Adi</name>
      </author>
      <author>
        <name>Suzuki, Yohey</name>
      </author>
      <author>
        <name>Banfield, Jillian</name>
      </author>
    </item>
    <item>
      <title>Cyanobacteria from marine oxygen-deficient zones encode both form I and form II Rubiscos</title>
      <link>https://escholarship.org/uc/item/4pd809vt</link>
      <description>Cyanobacteria are highly abundant in the marine photic zone and primary drivers of the conversion of inorganic carbon into biomass. To date, all studied cyanobacterial lineages encode carbon fixation machinery relying upon form I Rubiscos within a CO&lt;sub&gt;2&lt;/sub&gt;-concentrating carboxysome. Here, we report that the uncultivated anoxic marine zone (AMZ) IB lineage of &lt;i&gt;Prochlorococcus&lt;/i&gt; from pelagic oxygen-deficient zones (ODZs) harbors both form I and form II Rubiscos, the latter of which are typically noncarboxysomal and possess biochemical properties tuned toward low-oxygen environments. We demonstrate that these cyanobacterial form II enzymes are functional in vitro and were likely acquired from proteobacteria. Metagenomic analysis reveals that AMZ IB are essentially restricted to ODZs in the Eastern Pacific, suggesting that form II acquisition may confer an advantage under low-O&lt;sub&gt;2&lt;/sub&gt; conditions. AMZ IB populations express both forms of Rubisco in situ, with the highest...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4pd809vt</guid>
      <pubDate>Tue, 24 Dec 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Jaffe, Alexander L</name>
      </author>
      <author>
        <name>Harrison, Kaitlin</name>
      </author>
      <author>
        <name>Wang, Renée Z</name>
        <uri>https://orcid.org/0000-0003-3994-3244</uri>
      </author>
      <author>
        <name>Taylor-Kearney, Leah J</name>
      </author>
      <author>
        <name>Jain, Navami</name>
      </author>
      <author>
        <name>Prywes, Noam</name>
      </author>
      <author>
        <name>Shih, Patrick M</name>
      </author>
      <author>
        <name>Young, Jodi</name>
      </author>
      <author>
        <name>Rocap, Gabrielle</name>
      </author>
      <author>
        <name>Dekas, Anne E</name>
      </author>
    </item>
    <item>
      <title>Widespread detoxifying NO reductases impart a distinct isotopic fingerprint on N2O under anoxia</title>
      <link>https://escholarship.org/uc/item/5rs275ww</link>
      <description>Nitrous oxide (N&lt;sub&gt;2&lt;/sub&gt;O), a potent greenhouse gas, can be generated by multiple biological and abiotic processes in diverse contexts. Accurately tracking the dominant sources of N&lt;sub&gt;2&lt;/sub&gt;O has the potential to improve our understanding of N&lt;sub&gt;2&lt;/sub&gt;O fluxes from soils as well as inform the diagnosis of human infections. Isotopic "Site Preference" (SP) values have been used toward this end, as bacterial and fungal nitric oxide reductases (NORs) produce N&lt;sub&gt;2&lt;/sub&gt;O with different isotopic fingerprints, spanning a large range. Here, we show that flavohemoglobin (Fhp), a hitherto biogeochemically neglected yet widely distributed detoxifying bacterial NO reductase, imparts a distinct SP value onto N&lt;sub&gt;2&lt;/sub&gt;O under anoxic conditions (~+10‰) that correlates with typical environmental N&lt;sub&gt;2&lt;/sub&gt;O SP measurements. Using &lt;i&gt;Pseudomonas aeruginosa&lt;/i&gt; as a model organism, we generated strains that only contained Fhp or the dissimilatory NOR, finding that in vivo N&lt;sub&gt;2&lt;/sub&gt;O...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5rs275ww</guid>
      <pubDate>Fri, 20 Dec 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Wang, Renée Z</name>
        <uri>https://orcid.org/0000-0003-3994-3244</uri>
      </author>
      <author>
        <name>Lonergan, Zachery R</name>
      </author>
      <author>
        <name>Wilbert, Steven A</name>
      </author>
      <author>
        <name>Eiler, John M</name>
      </author>
      <author>
        <name>Newman, Dianne K</name>
      </author>
    </item>
    <item>
      <title>High-precision chemical quantum sensing in flowing monodisperse microdroplets</title>
      <link>https://escholarship.org/uc/item/1964g090</link>
      <description>A method is presented for high-precision chemical detection that integrates quantum sensing with droplet microfluidics. Using nanodiamonds (ND) with fluorescent nitrogen-vacancy (NV) centers as quantum sensors, rapidly flowing microdroplets containing analyte molecules are analyzed. A noise-suppressed mode of optically detected magnetic resonance is enabled by pairing controllable flow with microwave control of NV electronic spins, to detect analyte-induced signals of a few hundredths of a percent of the ND fluorescence. Using this method, paramagnetic ions in droplets are detected with low limit-of-detection using small analyte volumes, with exceptional measurement stability over &amp;gt;10&lt;sup&gt;3&lt;/sup&gt; s. In addition, these droplets are used as microconfinement chambers by co-encapsulating ND quantum sensors with various analytes such as single cells, suggesting wide-ranging applications including single-cell metabolomics and real-time intracellular measurements from bioreactors....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1964g090</guid>
      <pubDate>Fri, 20 Dec 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Sarkar, Adrisha</name>
        <uri>https://orcid.org/0000-0002-7893-9566</uri>
      </author>
      <author>
        <name>Jones, Zachary R</name>
      </author>
      <author>
        <name>Parashar, Madhur</name>
        <uri>https://orcid.org/0000-0002-0763-4351</uri>
      </author>
      <author>
        <name>Druga, Emanuel</name>
      </author>
      <author>
        <name>Akkiraju, Amala</name>
      </author>
      <author>
        <name>Conti, Sophie</name>
      </author>
      <author>
        <name>Krishnamoorthi, Pranav</name>
      </author>
      <author>
        <name>Nachuri, Srisai</name>
      </author>
      <author>
        <name>Aman, Parker</name>
      </author>
      <author>
        <name>Hashemi, Mohammad</name>
      </author>
      <author>
        <name>Nunn, Nicholas</name>
      </author>
      <author>
        <name>Torelli, Marco D</name>
      </author>
      <author>
        <name>Gilbert, Benjamin</name>
      </author>
      <author>
        <name>Wilson, Kevin R</name>
        <uri>https://orcid.org/0000-0003-0264-0872</uri>
      </author>
      <author>
        <name>Shenderova, Olga A</name>
      </author>
      <author>
        <name>Tanjore, Deepti</name>
        <uri>https://orcid.org/0000-0001-6507-4359</uri>
      </author>
      <author>
        <name>Ajoy, Ashok</name>
      </author>
    </item>
    <item>
      <title>Concurrent measurement of strain and chemical reaction rates in a calcite grain pack undergoing pressure solution: Evidence for surface-reaction controlled dissolution</title>
      <link>https://escholarship.org/uc/item/0ng9q1xs</link>
      <description>Pressure solution is inferred to be a significant contributor to sediment compaction and lithification, especially in carbonate sediments. For a sediment deforming primarily by pressure solution, the compaction rate should be directly related to the rate of calcite dissolution, transport along grain contacts, and calcite reprecipitation. Previous experimental work has shown that there is evidence that deformation in wet calcite grain packs is consistent with control by pressure solution, but considerable ambiguity remains regarding the rate limiting mechanism. We present the results of laboratory compaction experiments designed to directly measure calcite dissolution and precipitation rates (recrystallization rates) concurrently with strain rate to test whether measured rates are consistent with predicted rates both in absolute magnitude and time evolution. Recrystallization rates are measured using trace element chemistry (Sr/Ca, Mg/Ca) and isotopes (87Sr/86Sr) of fluids flowing...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0ng9q1xs</guid>
      <pubDate>Fri, 20 Dec 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Lisabeth, Harrison</name>
      </author>
      <author>
        <name>DePaolo, Donald J</name>
      </author>
      <author>
        <name>Pester, Nicholas J</name>
      </author>
      <author>
        <name>Christensen, John N</name>
      </author>
    </item>
    <item>
      <title>Ensemble Monte Carlo calculations with five novel moves</title>
      <link>https://escholarship.org/uc/item/6bb6x0b5</link>
      <description>We introduce five novel types of Monte Carlo (MC) moves that brings the number of moves of ensemble MC calculations from three to eight. So far such calculations have relied on affine invariant stretch moves that were originally introduced by Christen (2007) [8], walk moves by Goodman and Weare (2010) [16] and quadratic moves by Militzer (2023) [31,32]. Ensemble MC methods have been very popular because they harness information about the fitness landscape from a population of walkers rather than relying on expert knowledge. Here we modified the affine method and employed a simplex of points to set the stretch direction. We adopt the simplex concept to quadratic moves. We also generalize quadratic moves to arbitrary order. Finally, we introduce directed moves that employ the values of the probability density while all other types of moves rely solely on the location of the walkers. We apply all algorithms to the Rosenbrock density in 2 and 20 dimensions and to the ring potential...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6bb6x0b5</guid>
      <pubDate>Wed, 4 Dec 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Militzer, Burkhard</name>
        <uri>https://orcid.org/0000-0002-7092-5629</uri>
      </author>
    </item>
    <item>
      <title>Deep mantle plumes feeding periodic alignments of asthenospheric fingers beneath the central and southern Atlantic Ocean</title>
      <link>https://escholarship.org/uc/item/5s51q9mz</link>
      <description>High-resolution full waveform seismic tomography of the Earth's mantle beneath the south and central Atlantic Ocean brings into focus a series of asthenospheric low shear velocity channels, or "fingers" on both sides of the southern and central mid-Atlantic ridge (MAR), elongated in the direction of absolute plate motion with a spacing of [Formula: see text]1,800 to 2,000 km, and associated with bands of shallower residual seafloor depth anomalies that suggest channeled flow over thousands of kilometers. Each of the three most clearly resolved fingers on the African side of the MAR corresponds to a separate group of whole mantle plumes rooted in distinct patches at the core-mantle boundary, feeding hotspots, and volcanic lines with distinct isotopic signatures. Plumes of a given group appear to merge at the top of the lower mantle before separating again, suggesting interaction of deep mantle flow with a more vigorous mesoscale circulation in the upper mantle. The corresponding...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5s51q9mz</guid>
      <pubDate>Wed, 27 Nov 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Munch, Federico D</name>
      </author>
      <author>
        <name>Romanowicz, Barbara</name>
        <uri>https://orcid.org/0000-0002-6208-6044</uri>
      </author>
      <author>
        <name>Mukhopadhyay, Sujoy</name>
      </author>
      <author>
        <name>Rudolph, Maxwell L</name>
        <uri>https://orcid.org/0000-0001-7721-4224</uri>
      </author>
    </item>
    <item>
      <title>Paleomagnetic Records From Pulsed Magmatism in the Southwestern Laurentia Large Igneous Province and Cardenas Basalt Support Rapid Late Mesoproterozoic Plate Motion</title>
      <link>https://escholarship.org/uc/item/61d4c2hw</link>
      <description>Mafic intrusions, lava flows, and felsic plutons in southwestern Laurentia have been hypothesized to be associated with the emplacement of a late Mesoproterozoic (Stenian Period) large igneous province. Improved geochronologic data resolve distinct episodes of mafic magmatism in the region. The ca. 1,098&amp;nbsp;Ma main pulse of southwestern Laurentia large igneous province (SWLLIP) magmatism is recorded by mafic intrusions across southeastern California to central Arizona. A younger episode of volcanism resulted in eruptions that formed the ca. 1,082&amp;nbsp;Ma Cardenas Basalt, which is the uppermost unit of the Unkar Group in the Grand Canyon. With the updated geochronological constraints, we develop new paleomagnetic data from mafic sills in the SWLLIP. Overlapping poles between the Death Valley sills and rocks of similar age in the Midcontinent Rift are inconsistent with large-scale Cenozoic vertical axis rotations in Death Valley. We also develop a new paleomagnetic pole from the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/61d4c2hw</guid>
      <pubDate>Wed, 6 Nov 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Zhang, Yiming</name>
      </author>
      <author>
        <name>Anderson, Nicolas S</name>
      </author>
      <author>
        <name>Mohr, Michael T</name>
      </author>
      <author>
        <name>Nelson, Lyle L</name>
      </author>
      <author>
        <name>Macdonald, Francis A</name>
        <uri>https://orcid.org/0000-0001-8416-4894</uri>
      </author>
      <author>
        <name>Schmitz, Mark D</name>
      </author>
      <author>
        <name>Thurston, Olivia G</name>
      </author>
      <author>
        <name>Guenthner, William R</name>
      </author>
      <author>
        <name>Karlstrom, Karl E</name>
      </author>
      <author>
        <name>Swanson‐Hysell, Nicholas L</name>
      </author>
    </item>
    <item>
      <title>Reconstructing the paleoenvironment of an oxygenated Mesoproterozoic shoreline and its record of life</title>
      <link>https://escholarship.org/uc/item/2f04b12z</link>
      <description>The Nonesuch Formation microbiota provide a window into ca. 1075 Ma life within the interior of ancient North America. The Nonesuch water body formed following the cessation of widespread volcanism within the Midcontinent Rift as the basin continued to subside. In northern Michigan and Wisconsin, USA, the Copper Harbor Conglomerate records terrestrial alluvial fan and fluvial plain environments that transitioned into subaqueous lacustrine deposition of the Nonesuch Formation. These units thin toward a paleotopographic high associated with the Brownstone Falls angular unconformity. Due to these “Brownstone Highlands,” we were able to explore the paleoenvironment laterally at different depths in contemporaneous deposits. Rock magnetic data constrain that when the lake was shallow, it was oxygenated as evidenced by an oxidized mineral assemblage. Oxygen levels were lower at greater depth—in the deepest portions of the water body, anoxic conditions are recorded. An intermediate facies...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2f04b12z</guid>
      <pubDate>Wed, 6 Nov 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Slotznick, Sarah P</name>
      </author>
      <author>
        <name>Swanson-Hysell, Nicholas L</name>
        <uri>https://orcid.org/0000-0003-3215-4648</uri>
      </author>
      <author>
        <name>Zhang, Yiming</name>
      </author>
      <author>
        <name>Clayton, Katherine E</name>
      </author>
      <author>
        <name>Wellman, Charles H</name>
      </author>
      <author>
        <name>Tosca, Nicholas J</name>
      </author>
      <author>
        <name>Strother, Paul K</name>
      </author>
    </item>
    <item>
      <title>A large colonial choanoflagellate from Mono Lake harbors live bacteria</title>
      <link>https://escholarship.org/uc/item/0w9998xw</link>
      <description>As the closest living relatives of animals, choanoflagellates offer insights into the ancestry of animal cell physiology. Here, we report the isolation and characterization of a colonial choanoflagellate from Mono Lake, California. The choanoflagellate forms large spherical colonies that are an order of magnitude larger than those formed by the closely related choanoflagellate &lt;i&gt;Salpingoeca rosetta&lt;/i&gt;. In cultures maintained in the laboratory, the lumen of the spherical colony is filled with a branched network of extracellular matrix and colonized by bacteria, including diverse Gammaproteobacteria and Alphaproteobacteria. We propose to erect &lt;i&gt;Barroeca monosierra&lt;/i&gt; gen. nov., sp. nov. Hake, Burkhardt, Richter, and King to accommodate this extremophile choanoflagellate. The physical association between bacteria and &lt;i&gt;B. monosierra&lt;/i&gt; in culture presents a new experimental model for investigating interactions among bacteria and eukaryotes. Future work will investigate the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0w9998xw</guid>
      <pubDate>Wed, 30 Oct 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Hake, KH</name>
      </author>
      <author>
        <name>West, PT</name>
      </author>
      <author>
        <name>McDonald, K</name>
      </author>
      <author>
        <name>Laundon, D</name>
      </author>
      <author>
        <name>Reyes-Rivera, J</name>
      </author>
      <author>
        <name>De Las Bayonas, A Garcia</name>
      </author>
      <author>
        <name>Feng, C</name>
      </author>
      <author>
        <name>Burkhardt, P</name>
      </author>
      <author>
        <name>Richter, DJ</name>
      </author>
      <author>
        <name>Banfield, JF</name>
      </author>
      <author>
        <name>King, N</name>
        <uri>https://orcid.org/0000-0002-6409-1111</uri>
      </author>
    </item>
    <item>
      <title>Understanding the Spatiotemporal Variability of Tropical Orographic Rainfall Using Convective Plume Buoyancy</title>
      <link>https://escholarship.org/uc/item/5kn2f6zv</link>
      <description>Abstract Mechanical forcing by orography affects precipitating convection across many tropical regions, but controls on the intensity and horizontal extent of the orographic precipitation peak and rain shadow remain poorly understood. A recent theory explains this control of precipitation as arising from modulation of lower-tropospheric temperature and moisture by orographic mechanical forcing, setting the distribution of convective rainfall by controlling parcel buoyancy. Using satellite and reanalysis data, we evaluate this theory by investigating spatiotemporal precipitation variations in six mountainous tropical regions spanning South and Southeast Asia, and the Maritime Continent. We show that a strong relationship holds in these regions between daily precipitation and a measure of convective plume buoyancy. This measure depends on boundary layer thermodynamic properties and lower-free-tropospheric moisture and temperature. Consistent with the theory, temporal variations...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5kn2f6zv</guid>
      <pubDate>Mon, 7 Oct 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Nicolas, Quentin</name>
      </author>
      <author>
        <name>Boos, William R</name>
        <uri>https://orcid.org/0000-0001-9076-3551</uri>
      </author>
    </item>
    <item>
      <title>Liquid water in the Martian mid-crust</title>
      <link>https://escholarship.org/uc/item/9fk102qf</link>
      <description>Large volumes of liquid water transiently existed on the surface of Mars more than 3 billion years ago. Much of this water is hypothesized to have been sequestered in the subsurface or lost to space. We use rock physics models and Bayesian inversion to identify combinations of lithology, liquid water saturation, porosity, and pore shape consistent with the constrained mid-crust (∼11.5 to 20 km depths) seismic velocities and gravity near the InSight lander. A mid-crust composed of fractured igneous rocks saturated with liquid water best explains the existing data. Our results have implications for understanding Mars' water cycle, determining the fates of past surface water, searching for past or extant life, and assessing in situ resource utilization for future missions.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9fk102qf</guid>
      <pubDate>Thu, 29 Aug 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Wright, Vashan</name>
      </author>
      <author>
        <name>Morzfeld, Matthias</name>
        <uri>https://orcid.org/0000-0003-2257-8930</uri>
      </author>
      <author>
        <name>Manga, Michael</name>
        <uri>https://orcid.org/0000-0003-3286-4682</uri>
      </author>
    </item>
    <item>
      <title>Serpentinization as a Tape Recorder of (Dis)Continuous Mantle Exhumation along the Alpine Tethys Ocean-Continent-Transition</title>
      <link>https://escholarship.org/uc/item/2w616573</link>
      <description>Abstract: 

               Serpentinization has been widely documented and investigated at mid-ocean ridges (MOR) and subduction zones. In contrast, at magma-poor rifted margins serpentinization has received much less attention, despite its importance in controlling rheology and mass fluxes during breakup and establishing of a steady-state MOR. In this study, we present new petrological and geochemical data on subcontinental exhumed serpentinized peridotites from the spectacularly exposed Platta, Tasna and Totalp nappes in the Eastern Central Alps in SE Switzerland, belonging to the Alpine Tethys Ocean Continent Transition (OCT). The results testify of a complex history of fluid–rock interactions recorded by several serpentinization events starting with lizardite mesh and bastite textures (S1), subsequently followed by a succession of serpentine-filling veins with distinct textures and serpentine polysomes that include spherical polyhedral serpentine (S2); chrysotile ± polygonal...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2w616573</guid>
      <pubDate>Thu, 29 Aug 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Hochscheid, Flora</name>
      </author>
      <author>
        <name>Ulrich, Marc</name>
      </author>
      <author>
        <name>Muñoz, Manuel</name>
      </author>
      <author>
        <name>Boulvais, Philippe</name>
      </author>
      <author>
        <name>Manatschal, Gianreto</name>
      </author>
    </item>
    <item>
      <title>pH and thiosulfate dependent microbial sulfur oxidation strategies across diverse environments</title>
      <link>https://escholarship.org/uc/item/8kw270cf</link>
      <description>Sulfur oxidizing bacteria (SOB) play a key role in sulfur cycling in mine tailings impoundment (TI) waters, where sulfur concentrations are typically high. However, our understanding of SOB sulfur cycling via potential S oxidation pathways (&lt;i&gt;sox&lt;/i&gt;, r&lt;i&gt;dsr&lt;/i&gt;, and S&lt;sub&gt;4&lt;/sub&gt;I) in these globally ubiquitous contexts, remains limited. Here, we identified TI water column SOB community composition, metagenomics derived metabolic repertoires, physicochemistry, and aqueous sulfur concentration and speciation in four Canadian base metal mine, circumneutral-alkaline TIs over four years (2016 - 2019). Identification and examination of genomes from nine SOB genera occurring in these TI waters revealed two pH partitioned, metabolically distinct groups, which differentially influenced acid generation and sulfur speciation. Complete &lt;i&gt;sox&lt;/i&gt; (c&lt;i&gt;sox&lt;/i&gt;) dominant SOB (e.g., &lt;i&gt;Halothiobacillus&lt;/i&gt; spp., &lt;i&gt;Thiomonas&lt;/i&gt; spp.) drove acidity generation and S&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;3&lt;/sub&gt;...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8kw270cf</guid>
      <pubDate>Mon, 19 Aug 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Twible, Lauren E</name>
      </author>
      <author>
        <name>Whaley-Martin, Kelly</name>
      </author>
      <author>
        <name>Chen, Lin-Xing</name>
      </author>
      <author>
        <name>Nelson, Tara Colenbrander</name>
      </author>
      <author>
        <name>Arrey, James LS</name>
      </author>
      <author>
        <name>Jarolimek, Chad V</name>
      </author>
      <author>
        <name>King, Josh J</name>
      </author>
      <author>
        <name>Ramilo, Lisa</name>
      </author>
      <author>
        <name>Sonnenberg, Helga</name>
      </author>
      <author>
        <name>Banfield, Jillian F</name>
      </author>
      <author>
        <name>Apte, Simon C</name>
      </author>
      <author>
        <name>Warren, Lesley A</name>
      </author>
    </item>
    <item>
      <title>Asgard archaea modulate potential methanogenesis substrates in wetland soil</title>
      <link>https://escholarship.org/uc/item/2vj1b28x</link>
      <description>The roles of Asgard archaea in eukaryogenesis and marine biogeochemical cycles are well studied, yet their contributions in soil ecosystems remain unknown. Of particular interest are Asgard archaeal contributions to methane cycling in wetland soils. To investigate this, we reconstructed two complete genomes for soil-associated Atabeyarchaeia, a new Asgard lineage, and a complete genome of Freyarchaeia, and predicted their metabolism in situ. Metatranscriptomics reveals expression of genes for [NiFe]-hydrogenases, pyruvate oxidation and carbon fixation via the Wood-Ljungdahl pathway. Also expressed are genes encoding enzymes for amino acid metabolism, anaerobic aldehyde oxidation, hydrogen peroxide detoxification and carbohydrate breakdown to acetate and formate. Overall, soil-associated Asgard archaea are predicted to include&amp;nbsp;non-methanogenic acetogens, highlighting their potential role in carbon cycling in terrestrial environments.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2vj1b28x</guid>
      <pubDate>Mon, 19 Aug 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Valentin-Alvarado, Luis E</name>
      </author>
      <author>
        <name>Appler, Kathryn E</name>
      </author>
      <author>
        <name>De Anda, Valerie</name>
      </author>
      <author>
        <name>Schoelmerich, Marie C</name>
      </author>
      <author>
        <name>West-Roberts, Jacob</name>
      </author>
      <author>
        <name>Kivenson, Veronika</name>
      </author>
      <author>
        <name>Crits-Christoph, Alexander</name>
      </author>
      <author>
        <name>Ly, Lynn</name>
      </author>
      <author>
        <name>Sachdeva, Rohan</name>
      </author>
      <author>
        <name>Greening, Chris</name>
      </author>
      <author>
        <name>Savage, David F</name>
      </author>
      <author>
        <name>Baker, Brett J</name>
      </author>
      <author>
        <name>Banfield, Jillian F</name>
      </author>
    </item>
    <item>
      <title>Clades of huge phages from across Earth’s ecosystems</title>
      <link>https://escholarship.org/uc/item/5br7d58g</link>
      <description>Bacteriophages typically have small genomes1 and depend on their bacterial hosts for replication2. Here we sequenced DNA from diverse ecosystems and found hundreds of phage genomes with lengths of more than 200&amp;nbsp;kilobases (kb), including a genome of 735&amp;nbsp;kb, which is—to our knowledge—the largest phage genome to be described to date. Thirty-five genomes were manually curated to completion (circular and no gaps). Expanded genetic repertoires include diverse and previously undescribed CRISPR–Cas systems, transfer RNAs (tRNAs), tRNA synthetases, tRNA-modification enzymes, translation-initiation and elongation factors, and ribosomal proteins. The CRISPR–Cas systems of phages have the capacity to silence host transcription factors and translational genes, potentially as part of a larger interaction network that intercepts translation to redirect biosynthesis to phage-encoded functions. In addition, some phages may repurpose bacterial CRISPR–Cas systems to eliminate competing...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5br7d58g</guid>
      <pubDate>Sun, 18 Aug 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Al-Shayeb, Basem</name>
      </author>
      <author>
        <name>Sachdeva, Rohan</name>
      </author>
      <author>
        <name>Chen, Lin-Xing</name>
      </author>
      <author>
        <name>Ward, Fred</name>
      </author>
      <author>
        <name>Munk, Patrick</name>
      </author>
      <author>
        <name>Devoto, Audra</name>
      </author>
      <author>
        <name>Castelle, Cindy J</name>
      </author>
      <author>
        <name>Olm, Matthew R</name>
      </author>
      <author>
        <name>Bouma-Gregson, Keith</name>
      </author>
      <author>
        <name>Amano, Yuki</name>
      </author>
      <author>
        <name>He, Christine</name>
      </author>
      <author>
        <name>Méheust, Raphaël</name>
      </author>
      <author>
        <name>Brooks, Brandon</name>
      </author>
      <author>
        <name>Thomas, Alex</name>
      </author>
      <author>
        <name>Lavy, Adi</name>
      </author>
      <author>
        <name>Matheus-Carnevali, Paula</name>
      </author>
      <author>
        <name>Sun, Christine</name>
      </author>
      <author>
        <name>Goltsman, Daniela SA</name>
      </author>
      <author>
        <name>Borton, Mikayla A</name>
      </author>
      <author>
        <name>Sharrar, Allison</name>
      </author>
      <author>
        <name>Jaffe, Alexander L</name>
      </author>
      <author>
        <name>Nelson, Tara C</name>
      </author>
      <author>
        <name>Kantor, Rose</name>
      </author>
      <author>
        <name>Keren, Ray</name>
      </author>
      <author>
        <name>Lane, Katherine R</name>
      </author>
      <author>
        <name>Farag, Ibrahim F</name>
      </author>
      <author>
        <name>Lei, Shufei</name>
      </author>
      <author>
        <name>Finstad, Kari</name>
      </author>
      <author>
        <name>Amundson, Ronald</name>
        <uri>https://orcid.org/0000-0003-1510-7313</uri>
      </author>
      <author>
        <name>Anantharaman, Karthik</name>
      </author>
      <author>
        <name>Zhou, Jinglie</name>
      </author>
      <author>
        <name>Probst, Alexander J</name>
      </author>
      <author>
        <name>Power, Mary E</name>
      </author>
      <author>
        <name>Tringe, Susannah G</name>
        <uri>https://orcid.org/0000-0001-6479-8427</uri>
      </author>
      <author>
        <name>Li, Wen-Jun</name>
      </author>
      <author>
        <name>Wrighton, Kelly</name>
      </author>
      <author>
        <name>Harrison, Sue</name>
      </author>
      <author>
        <name>Morowitz, Michael</name>
      </author>
      <author>
        <name>Relman, David A</name>
      </author>
      <author>
        <name>Doudna, Jennifer A</name>
      </author>
      <author>
        <name>Lehours, Anne-Catherine</name>
      </author>
      <author>
        <name>Warren, Lesley</name>
      </author>
      <author>
        <name>Cate, Jamie HD</name>
      </author>
      <author>
        <name>Santini, Joanne M</name>
      </author>
      <author>
        <name>Banfield, Jillian F</name>
      </author>
    </item>
    <item>
      <title>Fault valving and pore pressure evolution in simulations of earthquake sequences and aseismic slip</title>
      <link>https://escholarship.org/uc/item/9239w933</link>
      <description>Fault-zone fluids control effective normal stress and fault strength. While most earthquake models assume a fixed pore fluid pressure distribution, geologists have documented fault valving behavior, that is, cyclic changes in pressure and unsteady fluid migration along faults. Here we quantify fault valving through 2-D antiplane shear simulations of earthquake sequences on a strike-slip fault with rate-and-state friction, upward Darcy flow along a permeable fault zone, and permeability evolution. Fluid overpressure develops during the interseismic period, when healing/sealing reduces fault permeability, and is released after earthquakes enhance permeability. Coupling between fluid flow, permeability and pressure evolution, and slip produces fluid-driven aseismic slip near the base of the seismogenic zone and earthquake swarms within the seismogenic zone, as ascending fluids pressurize and weaken the fault. This model might explain observations of late interseismic fault unlocking,...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9239w933</guid>
      <pubDate>Thu, 15 Aug 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Zhu, Weiqiang</name>
        <uri>https://orcid.org/0000-0003-2889-1493</uri>
      </author>
      <author>
        <name>Allison, Kali L</name>
      </author>
      <author>
        <name>Dunham, Eric M</name>
      </author>
      <author>
        <name>Yang, Yuyun</name>
      </author>
    </item>
    <item>
      <title>An upper-crust lid over the Long Valley magma chamber</title>
      <link>https://escholarship.org/uc/item/6wm428qf</link>
      <description>Geophysical characterization of calderas is fundamental in assessing their potential for future catastrophic volcanic eruptions. The mechanism behind the unrest of Long Valley Caldera in California remains highly debated, with recent periods of uplift and seismicity driven either by the release of aqueous fluids from the magma chamber or by the intrusion of magma into the upper crust. We use distributed acoustic sensing data recorded along a 100-kilometer fiber-optic cable traversing the caldera to image its subsurface structure. Our images highlight a definite separation between the shallow hydrothermal system and the large magma chamber located at ~12-kilometer depth. The combination of the geological evidence with our results shows how fluids exsolved through second boiling provide the source of the observed uplift and seismicity.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6wm428qf</guid>
      <pubDate>Thu, 15 Aug 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Biondi, Ettore</name>
      </author>
      <author>
        <name>Zhu, Weiqiang</name>
        <uri>https://orcid.org/0000-0003-2889-1493</uri>
      </author>
      <author>
        <name>Li, Jiaxuan</name>
      </author>
      <author>
        <name>Williams, Ethan F</name>
      </author>
      <author>
        <name>Zhan, Zhongwen</name>
      </author>
    </item>
    <item>
      <title>Earthquake transformer—an attentive deep-learning model for simultaneous earthquake detection and phase picking</title>
      <link>https://escholarship.org/uc/item/5146j96s</link>
      <description>Earthquake signal detection and seismic phase picking are challenging tasks in the processing of noisy data and the monitoring of microearthquakes. Here we present a global deep-learning model for simultaneous earthquake detection and phase picking. Performing these two related tasks in tandem improves model performance in each individual task by combining information in phases and in the full waveform of earthquake signals by using a hierarchical attention mechanism. We show that our model outperforms previous deep-learning and traditional phase-picking and detection algorithms. Applying our model to 5 weeks of continuous data recorded during 2000 Tottori earthquakes in Japan, we were able to detect and locate two times more earthquakes using only a portion (less than 1/3) of seismic stations. Our model picks P and S phases with precision close to manual picks by human analysts; however, its high efficiency and higher sensitivity can result in detecting and characterizing more...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5146j96s</guid>
      <pubDate>Thu, 15 Aug 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Mousavi, S Mostafa</name>
      </author>
      <author>
        <name>Ellsworth, William L</name>
      </author>
      <author>
        <name>Zhu, Weiqiang</name>
        <uri>https://orcid.org/0000-0003-2889-1493</uri>
      </author>
      <author>
        <name>Chuang, Lindsay Y</name>
      </author>
      <author>
        <name>Beroza, Gregory C</name>
      </author>
    </item>
    <item>
      <title>Bubble ascent and rupture in mud volcanoes</title>
      <link>https://escholarship.org/uc/item/3bm5v4s7</link>
      <description>Large gas bubbles can reach the surface of pools of mud and lava where they burst, often through the formation and expansion of circular holes. Bursting bubbles release volatiles and generate spatter, and hence play a key role in volcanic degassing and volcanic edifice construction. Here, we study the ascent and rupture of bubbles using a combination of field observations at Pâclele Mici (Romania), laboratory experiments with mud from the Imperial Valley (California, USA), numerical simulations and theoretical models. Numerical simulations predict that bubbles ascend through the mud as elliptical caps that develop a dimple at the apex as they impinge on the free surface. We documented the rupture of bubbles in nature and under laboratory conditions using high-speed video. The bursting of mud bubbles starts with the nucleation of multiple holes, which form at a near-constant rate and in quick succession. The quasi-circular holes rapidly grow and coalesce, and the sheet evolves...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3bm5v4s7</guid>
      <pubDate>Sat, 10 Aug 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Rudolph, Maxwell L</name>
        <uri>https://orcid.org/0000-0001-7721-4224</uri>
      </author>
      <author>
        <name>Sahu, Kirti Chandra</name>
      </author>
      <author>
        <name>Savva, Nikos</name>
      </author>
      <author>
        <name>Szilágyi, András</name>
      </author>
      <author>
        <name>Hórvölgyi, Zoltán</name>
      </author>
      <author>
        <name>Márton, Péter</name>
      </author>
      <author>
        <name>Tajti, Ádám</name>
      </author>
      <author>
        <name>Szép, Károly</name>
      </author>
      <author>
        <name>Balog, Boglárka</name>
      </author>
      <author>
        <name>Tripathi, Manoj Kumar</name>
      </author>
      <author>
        <name>Manikantan, Harishankar</name>
        <uri>https://orcid.org/0000-0002-4270-3527</uri>
      </author>
      <author>
        <name>Forray, Ferenc L</name>
      </author>
      <author>
        <name>Manga, Michael</name>
      </author>
      <author>
        <name>Hantz, Peter</name>
      </author>
    </item>
    <item>
      <title>Imaging the Meissner effect in hydride superconductors using quantum sensors</title>
      <link>https://escholarship.org/uc/item/4ww343m7</link>
      <description>By directly altering microscopic interactions, pressure provides a powerful tuning knob for the exploration of condensed phases and geophysical phenomena1. The megabar regime represents an interesting frontier, in which recent discoveries include high-temperature superconductors, as well as structural and valence phase transitions2–6. However, at such high pressures, many conventional measurement techniques fail. Here we demonstrate the ability to perform local magnetometry inside a diamond anvil cell with sub-micron spatial resolution at megabar pressures. Our approach uses a shallow layer of nitrogen-vacancy colour centres implanted directly within the anvil7–9; crucially, we choose a crystal cut compatible with the intrinsic symmetries of the nitrogen-vacancy centre to enable functionality at megabar pressures. We apply our technique to characterize a recently discovered hydride superconductor, CeH9 (ref. 10). By performing simultaneous magnetometry and electrical transport...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4ww343m7</guid>
      <pubDate>Tue, 6 Aug 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Bhattacharyya, P</name>
      </author>
      <author>
        <name>Chen, W</name>
      </author>
      <author>
        <name>Huang, X</name>
      </author>
      <author>
        <name>Chatterjee, S</name>
      </author>
      <author>
        <name>Huang, B</name>
      </author>
      <author>
        <name>Kobrin, B</name>
      </author>
      <author>
        <name>Lyu, Y</name>
      </author>
      <author>
        <name>Smart, TJ</name>
      </author>
      <author>
        <name>Block, M</name>
      </author>
      <author>
        <name>Wang, E</name>
      </author>
      <author>
        <name>Wang, Z</name>
      </author>
      <author>
        <name>Wu, W</name>
      </author>
      <author>
        <name>Hsieh, S</name>
      </author>
      <author>
        <name>Ma, H</name>
      </author>
      <author>
        <name>Mandyam, S</name>
      </author>
      <author>
        <name>Chen, B</name>
      </author>
      <author>
        <name>Davis, E</name>
      </author>
      <author>
        <name>Geballe, ZM</name>
      </author>
      <author>
        <name>Zu, C</name>
      </author>
      <author>
        <name>Struzhkin, V</name>
      </author>
      <author>
        <name>Jeanloz, R</name>
        <uri>https://orcid.org/0000-0002-3519-7929</uri>
      </author>
      <author>
        <name>Moore, JE</name>
      </author>
      <author>
        <name>Cui, T</name>
      </author>
      <author>
        <name>Galli, G</name>
      </author>
      <author>
        <name>Halperin, BI</name>
      </author>
      <author>
        <name>Laumann, CR</name>
      </author>
      <author>
        <name>Yao, NY</name>
      </author>
    </item>
    <item>
      <title>Back-to-back high category atmospheric river landfalls occur more often on the west coast of the United States</title>
      <link>https://escholarship.org/uc/item/3vn3n0c1</link>
      <description>The catastrophic December 2022-January 2023 nine atmospheric rivers in California underscore the urgent need to better understand such high-risk weather extremes. Here we applied a machine learning clustering tool to understand the activity of atmospheric river clusters. Reanalysis results show that clusters with high density, that is the time fraction under atmospheric river conditions within a cluster, exhibit more frequent high-category atmospheric rivers, alongside an increased likelihood for extreme precipitation and severe land surface responses. The key circulation patterns of atmospheric river clusters are primarily attributed to subseasonal variability. Furthermore, the occurrence and density of atmospheric river clusters are modulated by the daily variability of the geopotential height field. Climate model projections suggest that atmospheric river clusters with higher density and higher categories will be more frequent as warming level increases. Our findings emphasize...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3vn3n0c1</guid>
      <pubDate>Fri, 2 Aug 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Zhou, Yang</name>
        <uri>https://orcid.org/0000-0003-2835-4081</uri>
      </author>
      <author>
        <name>Wehner, Michael</name>
        <uri>https://orcid.org/0000-0001-8423-7870</uri>
      </author>
      <author>
        <name>Collins, William</name>
        <uri>https://orcid.org/0000-0002-4463-9848</uri>
      </author>
    </item>
    <item>
      <title>Forecasting Tropical Annual Maximum Wet‐Bulb Temperatures Months in Advance From the Current State of ENSO</title>
      <link>https://escholarship.org/uc/item/3tp9t0w4</link>
      <description>Abstract  Humid heatwaves, characterized by high temperature and humidity combinations, challenge tropical societies. Extreme wet‐bulb temperatures (TW) over tropical land are coupled to the warmest sea surface temperatures by atmospheric convection and wave dynamics. Here, we harness this coupling for seasonal forecasts of the annual maximum of daily maximum TW (TW max ). We develop a multiple linear regression model that explains 80% of variance in tropical mean TW max and significant regional TW max variances. The model considers warming trends and El Niño and Southern Oscillation indices. Looking ahead, the strong‐to‐very‐strong El Niño at the end of 2023, with an Oceanic Niño Index of ∼2.0, suggests a 2024 tropical land mean TW max of 26.2°C (25.9–26.4°C), and a 68% chance (24%–94%) of breaking existing records. This method also predicts regional TW max in specific areas. 
Plain Language Summary The heat and humidity in the tropics can be particularly challenging for people...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3tp9t0w4</guid>
      <pubDate>Tue, 30 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Zhang, Yi</name>
      </author>
      <author>
        <name>Boos, William R</name>
        <uri>https://orcid.org/0000-0001-9076-3551</uri>
      </author>
      <author>
        <name>Held, Isaac</name>
      </author>
      <author>
        <name>Paciorek, Christopher J</name>
      </author>
      <author>
        <name>Fueglistaler, Stephan</name>
      </author>
    </item>
    <item>
      <title>Using stable isotopes to inform water resource management in forested and agricultural ecosystems</title>
      <link>https://escholarship.org/uc/item/20w4s35z</link>
      <description>Present and future climatic trends are expected to markedly alter water fluxes and stores in the hydrologic cycle. In addition, water demand continues to grow due to increased human use and a growing population. Sustainably managing water resources requires a thorough understanding of water storage and flow in natural, agricultural, and urban ecosystems. Measurements of stable isotopes of water (hydrogen and oxygen) in the water cycle (atmosphere, soils, plants, surface water, and groundwater) can provide information on the transport pathways, sourcing, dynamics, ages, and storage pools of water that is difficult to obtain with other techniques. However, the potential of these techniques for practical questions has not been fully exploited yet. Here, we outline the benefits and limitations of potential applications of stable isotope methods useful to water managers, farmers, and other stakeholders. We also describe several case studies demonstrating how stable isotopes of water...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/20w4s35z</guid>
      <pubDate>Tue, 30 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Scandellari, Francesca</name>
      </author>
      <author>
        <name>Attou, Taha</name>
      </author>
      <author>
        <name>Barbeta, Adrià</name>
      </author>
      <author>
        <name>Bernhard, Fabian</name>
      </author>
      <author>
        <name>D'Amato, Concetta</name>
      </author>
      <author>
        <name>Dimitrova-Petrova, Katya</name>
      </author>
      <author>
        <name>Donaldson, Amanda</name>
      </author>
      <author>
        <name>Durodola, Oludare</name>
      </author>
      <author>
        <name>Ferraris, Stefano</name>
      </author>
      <author>
        <name>Floriancic, Marius G</name>
      </author>
      <author>
        <name>Fontenla-Razzetto, Gabriela</name>
      </author>
      <author>
        <name>Gerchow, Malkin</name>
      </author>
      <author>
        <name>Han, Qiong</name>
      </author>
      <author>
        <name>Khalil, Isis</name>
      </author>
      <author>
        <name>Kirchner, James W</name>
        <uri>https://orcid.org/0000-0001-6577-3619</uri>
      </author>
      <author>
        <name>Kühnhammer, Kathrin</name>
      </author>
      <author>
        <name>Liu, Qin</name>
      </author>
      <author>
        <name>Llorens, Pilar</name>
      </author>
      <author>
        <name>Magh, Ruth-Kristina</name>
      </author>
      <author>
        <name>Marshall, John</name>
      </author>
      <author>
        <name>Meusburger, Katrin</name>
      </author>
      <author>
        <name>Oliveira, Aline Meyer</name>
      </author>
      <author>
        <name>Muñoz-Villers, Lyssette</name>
      </author>
      <author>
        <name>Pires, Sabrina Santos</name>
      </author>
      <author>
        <name>Todini-Zicavo, Diego</name>
      </author>
      <author>
        <name>van Meerveld, Ilja</name>
      </author>
      <author>
        <name>Voigt, Claudia</name>
      </author>
      <author>
        <name>Wirsig, Luise</name>
      </author>
      <author>
        <name>Beyer, Matthias</name>
      </author>
      <author>
        <name>Geris, Josie</name>
      </author>
      <author>
        <name>Hopp, Luisa</name>
      </author>
      <author>
        <name>Penna, Daniele</name>
      </author>
      <author>
        <name>Sprenger, Matthias</name>
        <uri>https://orcid.org/0000-0003-1221-2767</uri>
      </author>
    </item>
    <item>
      <title>Identifying atmospheric rivers and their poleward latent heat transport with generalizable neural networks: ARCNNv1</title>
      <link>https://escholarship.org/uc/item/1hm1q8v0</link>
      <description>Abstract. Atmospheric rivers (ARs) are extreme weather events that can alleviate drought or cause billions of US dollars in flood damage. By transporting significant amounts of latent energy towards the poles, they are crucial to maintaining the climate system's energy balance. Since there is no first-principle definition of an AR grounded in geophysical fluid mechanics, AR identification is currently performed by a multitude of expert-defined, threshold-based algorithms. The variety of AR detection algorithms has introduced uncertainty into the study of ARs, and the thresholds of the algorithms may not generalize to new climate datasets and resolutions. We train convolutional neural networks (CNNs) to detect ARs while representing this uncertainty; we name these models ARCNNs. To detect ARs without requiring new labeled data and labor-intensive AR detection campaigns, we present a semi-supervised learning framework based on image style transfer. This framework generalizes ARCNNs...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1hm1q8v0</guid>
      <pubDate>Mon, 29 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Mahesh, Ankur</name>
      </author>
      <author>
        <name>O'Brien, Travis A</name>
        <uri>https://orcid.org/0000-0002-6643-1175</uri>
      </author>
      <author>
        <name>Loring, Burlen</name>
      </author>
      <author>
        <name>Elbashandy, Abdelrahman</name>
      </author>
      <author>
        <name>Boos, William</name>
        <uri>https://orcid.org/0000-0001-9076-3551</uri>
      </author>
      <author>
        <name>Collins, William D</name>
        <uri>https://orcid.org/0000-0002-4463-9848</uri>
      </author>
    </item>
    <item>
      <title>Analysis of Neptune’s 2017 bright equatorial storm</title>
      <link>https://escholarship.org/uc/item/9j94n9g9</link>
      <description>We report the discovery of a large (∼ 8500 km diameter) infrared-bright storm at Neptune's equator in June 2017. We tracked the storm over a period of 7 months with high-cadence infrared snapshot imaging, carried out on 14 nights at the 10 m Keck II telescope and 17 nights at the Shane 120 inch reflector at Lick Observatory. The cloud feature was larger and more persistent than any equatorial clouds seen before on Neptune, remaining intermittently active from at least 10 June to 31 December 2017. Our Keck and Lick observations were augmented by very high-cadence images from the amateur community, which permitted the determination of accurate drift rates for the cloud feature. Its zonal drift speed was variable from 10 June to at least 25 July, but remained a constant 237.4 ± 0.2 m s−1 from 30 September until at least 15 November. The pressure of the cloud top was determined from radiative transfer calculations to be 0.3-0.6 bar; this value remained constant over the course of...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9j94n9g9</guid>
      <pubDate>Tue, 23 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Molter, Edward</name>
        <uri>https://orcid.org/0000-0003-3799-9033</uri>
      </author>
      <author>
        <name>de Pater, Imke</name>
      </author>
      <author>
        <name>Luszcz-Cook, Statia</name>
      </author>
      <author>
        <name>Hueso, Ricardo</name>
      </author>
      <author>
        <name>Tollefson, Joshua</name>
      </author>
      <author>
        <name>Alvarez, Carlos</name>
      </author>
      <author>
        <name>Sánchez-Lavega, Agustín</name>
      </author>
      <author>
        <name>Wong, Michael H</name>
      </author>
      <author>
        <name>Hsu, Andrew I</name>
      </author>
      <author>
        <name>Sromovsky, Lawrence A</name>
      </author>
      <author>
        <name>Fry, Patrick M</name>
      </author>
      <author>
        <name>Delcroix, Marc</name>
      </author>
      <author>
        <name>Campbell, Randy</name>
      </author>
      <author>
        <name>de Kleer, Katherine</name>
      </author>
      <author>
        <name>Gates, Elinor</name>
        <uri>https://orcid.org/0000-0002-3739-0423</uri>
      </author>
      <author>
        <name>Lynam, Paul David</name>
      </author>
      <author>
        <name>Ammons, S Mark</name>
      </author>
      <author>
        <name>Coy, Brandon Park</name>
      </author>
      <author>
        <name>Duchene, Gaspard</name>
        <uri>https://orcid.org/0000-0002-5092-6464</uri>
      </author>
      <author>
        <name>Gonzales, Erica J</name>
      </author>
      <author>
        <name>Hirsch, Lea</name>
      </author>
      <author>
        <name>Magnier, Eugene A</name>
      </author>
      <author>
        <name>Ragland, Sam</name>
      </author>
      <author>
        <name>Rich, R Michael</name>
      </author>
      <author>
        <name>Wang, Feige</name>
      </author>
    </item>
    <item>
      <title>Quantitative Analysis of Paleomagnetic Sampling Strategies</title>
      <link>https://escholarship.org/uc/item/4k7824f0</link>
      <description>Sampling strategies used in paleomagnetic studies play a crucial role in dictating the accuracy of our estimates of properties of the ancient geomagnetic field. However, there has been little quantitative analysis of optimal paleomagnetic sampling strategies and the community has instead defaulted to traditional practices that vary between laboratories. In this paper, we quantitatively evaluate the accuracy of alternative paleomagnetic sampling strategies through numerical experiments and an associated analytical framework. Our findings demonstrate a strong correspondence between the accuracy of an estimated paleopole position and the number of sites or independent readings of the time-varying paleomagnetic field, whereas larger numbers of in-site samples have a dwindling effect. This remains true even when a large proportion of the sample directions are spurious. This approach can be readily achieved in sedimentary sequences by distributing samples stratigraphically, considering...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4k7824f0</guid>
      <pubDate>Thu, 11 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Sapienza, F</name>
      </author>
      <author>
        <name>Gallo, LC</name>
      </author>
      <author>
        <name>Zhang, Y</name>
      </author>
      <author>
        <name>Vaes, B</name>
      </author>
      <author>
        <name>Domeier, M</name>
      </author>
      <author>
        <name>Swanson‐Hysell, NL</name>
      </author>
    </item>
    <item>
      <title>Embracing Uncertainty to Resolve Polar Wander: A Case Study of Cenozoic North America</title>
      <link>https://escholarship.org/uc/item/3mw2t0h8</link>
      <description>Our understanding of Earth's paleogeography relies heavily on paleomagnetic apparent polar wander paths (APWPs), which represent the time-dependent position of Earth's spin axis relative to a given block of lithosphere. However, conventional approaches to APWP construction have significant limitations. First, the paleomagnetic record contains substantial noise that is not integrated into APWPs. Second, parametric assumptions are adopted to represent spatial and temporal uncertainties even where the underlying data do not conform to the assumed distributions. The consequences of these limitations remain largely unknown. Here, we address these challenges with a bottom-up Monte Carlo uncertainty propagation scheme that operates on site-level paleomagnetic data. To demonstrate our methodology, we present an extensive compilation of site-level Cenozoic paleomagnetic data from North America, which we use to generate a high-resolution APWP. Our results demonstrate that even in the presence...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3mw2t0h8</guid>
      <pubDate>Thu, 11 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Gallo, LC</name>
      </author>
      <author>
        <name>Domeier, M</name>
      </author>
      <author>
        <name>Sapienza, F</name>
      </author>
      <author>
        <name>Swanson‐Hysell, NL</name>
      </author>
      <author>
        <name>Vaes, B</name>
      </author>
      <author>
        <name>Zhang, Y</name>
      </author>
      <author>
        <name>Arnould, M</name>
      </author>
      <author>
        <name>Eyster, A</name>
      </author>
      <author>
        <name>Gürer, D</name>
      </author>
      <author>
        <name>Király, Á</name>
      </author>
      <author>
        <name>Robert, B</name>
      </author>
      <author>
        <name>Rolf, T</name>
      </author>
      <author>
        <name>Shephard, G</name>
      </author>
      <author>
        <name>van der Boon, A</name>
      </author>
    </item>
    <item>
      <title>Tracking Rodinia Into the Neoproterozoic: New Paleomagnetic Constraints From the Jacobsville Formation</title>
      <link>https://escholarship.org/uc/item/1gb4g3rv</link>
      <description>The paleogeography of Laurentia throughout the Neoproterozoic is critical for reconstructing global paleogeography due to its central position in the supercontinent Rodinia. We develop a new paleomagnetic pole from red siltstones and fine-grained sandstones of the early Neoproterozoic Jacobsville Formation which is now constrained to be ca. 990&amp;nbsp;Ma in age. High-resolution thermal demagnetization experiments resolve detrital remanent magnetizations held by hematite. These directions were reoriented within siltstone intraclasts and pass intraformational conglomerate tests—giving confidence that the magnetization is detrital and primary. An inclination-corrected mean paleomagnetic pole position for the Jacobsville Formation indicates that Laurentia's motion slowed down significantly following the onset of the Grenvillian orogeny. Prior rapid plate motion associated with closure of the Unimos Ocean between 1,110 and 1,090&amp;nbsp;Ma transitioned to slow drift of Laurentia across...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1gb4g3rv</guid>
      <pubDate>Thu, 11 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Zhang, Yiming</name>
      </author>
      <author>
        <name>Hodgin, Eben B</name>
      </author>
      <author>
        <name>Alemu, Tadesse</name>
      </author>
      <author>
        <name>Pierce, James</name>
      </author>
      <author>
        <name>Fuentes, Anthony</name>
      </author>
      <author>
        <name>Swanson‐Hysell, Nicholas L</name>
      </author>
    </item>
    <item>
      <title>3D architecture and complex behavior along the simple central San Andreas fault</title>
      <link>https://escholarship.org/uc/item/0qg7h792</link>
      <description>The central San Andreas Fault (CSAF) exhibits a simple linear large-scale fault geometry, yet seismic and aseismic deformation features vary in a complex way along the fault. Here we investigate fault zone behaviors using geodetic observation, seismicity and microearthquake focal mechanisms. We employ an improved focal-mechanism characterization method using relative earthquake radiation patterns on 75,164 Ml ≥ 1 earthquakes along a 2-km-wide, 190-km-long segment of the CSAF, from 1984 to 2015. The data reveal the 3D fine-scale structure and interseismic kinematics of the CSAF. Our findings indicate that the first-order spatial variations in interseismic fault creep rate, creep direction, and the fault zone stress field can be explained by a simple fault coupling model. The inferred 3D mechanical properties of a mechanically weak and poorly coupled fault zone provide a unified understanding of the complex fine-scale kinematics, indicating distributed slip deficits facilitating...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0qg7h792</guid>
      <pubDate>Sat, 6 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Cheng, Yifang</name>
      </author>
      <author>
        <name>Bürgmann, Roland</name>
      </author>
      <author>
        <name>Allen, Richard M</name>
        <uri>https://orcid.org/0000-0003-4293-9772</uri>
      </author>
    </item>
    <item>
      <title>Elastic properties of Fe-bearing Akimotoite at mantle conditions: Implications for composition and temperature in lower mantle transition zone</title>
      <link>https://escholarship.org/uc/item/56g4w0wn</link>
      <description>The pyrolite model, which can reproduce the upper-mantle seismic velocity and density profiles, was suggested to have significantly lower velocities and density than seismic models in the lower mantle transition zone (MTZ). This argument has been taken as mineral-physics evidence for a compositionally distinct lower MTZ. However, previous studies only estimated the pyrolite velocities and density along a one-dimension (1D) geotherm and never considered the effect of lateral temperature heterogeneity. Because the majorite-perovskite-akimotoite triple point is close to the normal mantle geotherm in the lower MTZ, the lateral low-temperature anomaly can result in the presence of a significant fraction of akimotoite in pyrolitic lower MTZ. In this study, we reported the elastic properties of Fe-bearing akimotoite based on first-principles calculations. Combining with literature data, we found that the seismic velocities and density of the pyrolite model can match well those in the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/56g4w0wn</guid>
      <pubDate>Mon, 1 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Zhao, Yajie</name>
      </author>
      <author>
        <name>Wu, Zhongqing</name>
      </author>
      <author>
        <name>Hao, Shangqin</name>
        <uri>https://orcid.org/0000-0002-3724-9657</uri>
      </author>
      <author>
        <name>Wang, Wenzhong</name>
      </author>
      <author>
        <name>Deng, Xin</name>
      </author>
      <author>
        <name>Song, Jian</name>
      </author>
    </item>
    <item>
      <title>Chronostratigraphy of Miocene strata in the Berkeley Hills (California Coast Ranges, USA) and the arrival of the San Andreas transform boundary</title>
      <link>https://escholarship.org/uc/item/52d8z27v</link>
      <description>Miocene strata of the Claremont, Orinda, and Moraga formations of the Berkeley Hills (California Coast Ranges, USA) record sedimentation and volcanism during the passage of the Mendocino triple junction and early evolution of the San Andreas fault system. Detrital zircon laser ablation–inductively coupled plasma–mass spectrometry (LA-ICP-MS) age spectra indicate a change in sedimentary prove nance between the marine Claremont formation (Monterey Group) and the terrestrial Orinda and Moraga Formations associated with uplift of Franciscan Complex lithologies. A sandstone from the Claremont formation produced a detrital zircon chemical abrasion–isotope dilution–thermal ionization mass spec trometry (CA-ID-TIMS) maximum depositional age of 13.298 ± 0.046 Ma, indicating younger Claremont deposition than previously interpreted. A trachydacite tuff clast within the uppermost Orinda Formation yielded a CA-ID-TIMS U-Pb zircon date of 10.094 ± 0.018 Ma, and a dacitic tuff within the Moraga...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/52d8z27v</guid>
      <pubDate>Tue, 25 Jun 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Gerasimov, Stacey H</name>
      </author>
      <author>
        <name>Hodgin, Eben B</name>
      </author>
      <author>
        <name>Crowley, James L</name>
      </author>
      <author>
        <name>Swanson-Hysell, Nicholas L</name>
        <uri>https://orcid.org/0000-0003-3215-4648</uri>
      </author>
    </item>
    <item>
      <title>Airfall volume of the 15 January 2022 eruption of Hunga volcano estimated from ocean color changes</title>
      <link>https://escholarship.org/uc/item/423976jc</link>
      <description>On 15 January 2022, Hunga volcano erupted, creating an extensive and high-reaching umbrella cloud over the open ocean, hindering traditional isopach mapping and fallout volume estimation. In MODIS satellite imagery, ocean surface water was discolored around Hunga following the eruption, which we attribute to ash fallout from the umbrella cloud. By relating intensity of ocean discoloration to fall deposit thicknesses in the Kingdom of Tonga, we develop a methodology for estimating airfall volume over the open ocean. Ash thickness measurements from 41 locations are used to fit a linear relationship between ash thickness and ocean reflectance. This produces a minimum airfall volume estimate of 1.8-0.4+0.3$${1.8}_{-0.4}^{+0.3}$$ km3. The whole eruption produced &amp;gt; 6.3 km3 of uncompacted pyroclastic material on the seafloor and a caldera volume change of 6 km3 DRE. Our fall estimates are consistent with the interpretation that most of the seafloor deposits were emplaced by gravity...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/423976jc</guid>
      <pubDate>Mon, 24 Jun 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Kelly, Liam J</name>
      </author>
      <author>
        <name>Fauria, Kristen E</name>
      </author>
      <author>
        <name>Manga, Michael</name>
      </author>
      <author>
        <name>Cronin, Shane J</name>
      </author>
      <author>
        <name>Latu’ila, Folauhola Helina</name>
      </author>
      <author>
        <name>Paredes-Mariño, Joali</name>
      </author>
      <author>
        <name>Mittal, Tushar</name>
      </author>
      <author>
        <name>Bennartz, Ralf</name>
      </author>
    </item>
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