Department of Earth, Planetary, and Space Sciences
Parent: UCLA
eScholarship stats: Breakdown by Item for December, 2024 through March, 2025
Item | Title | Total requests | Download | View-only | %Dnld |
---|---|---|---|---|---|
5ck322xw | Electron Crescent Distributions as a Manifestation of Diamagnetic Drift in an Electron‐Scale Current Sheet: Magnetospheric Multiscale Observations Using New 7.5 ms Fast Plasma Investigation Moments | 122 | 5 | 117 | 4.1% |
403071pz | Thickness of the crust of Mercury from geoid‐to‐topography ratios | 110 | 8 | 102 | 7.3% |
5jx2s2sm | Heat transfer by rapidly rotating Rayleigh–Bénard convection | 98 | 15 | 83 | 15.3% |
1v0549nf | Rotating thermal convection in liquid gallium: multi-modal flow, absent steady columns | 90 | 15 | 75 | 16.7% |
8rr3m49z | Insufficient Evidence of Purported Lunar Effect on Pollination in Ephedra | 90 | 5 | 85 | 5.6% |
62k0726h | Mechanics of inner core super‐rotation | 88 | 4 | 84 | 4.5% |
3m11w73f | Boundary layer control of rotating convection systems | 87 | 18 | 69 | 20.7% |
8hz43445 | High Arctic wetting reduces permafrost carbon feedbacks to climate warming | 87 | 12 | 75 | 13.8% |
6qz5k7jn | Axisymmetric simulations of libration-driven fluid dynamics in a spherical shell geometry | 84 | 9 | 75 | 10.7% |
1qp6d98w | Microbial Community Response to Simulated Petroleum Seepage in Caspian Sea Sediments | 83 | 7 | 76 | 8.4% |
83j959mc | Δ 13 CH 3 D and Δ 12 CH 2 D 2 signatures of methane aerobically oxidized by Methylosinus trichosporium with implications for deciphering the provenance of methane gases | 83 | 9 | 74 | 10.8% |
2m86n9zw | Local heating of radiation belt electrons to ultra-relativistic energies | 82 | 1 | 81 | 1.2% |
5ch2w82q | Influence of methane seepage on isotopic signatures in living deep-sea benthic foraminifera, 79° N | 81 | 1 | 80 | 1.2% |
2td732sd | Benthic Dinitrogen Fixation Traversing the Oxygen Minimum Zone Off Mauritania (NW Africa) | 80 | 1 | 79 | 1.3% |
47j2c0qj | Thermal evidence for Taylor columns in turbulent rotating Rayleigh-Bénard convection | 79 | 3 | 76 | 3.8% |
8fx1f8cz | Predominance of ECH wave contribution to diffuse aurora in Earth's outer magnetosphere | 79 | 10 | 69 | 12.7% |
31r7q1j8 | Tornado-like vortices in the quasi-cyclostrophic regime of Coriolis-centrifugal convection | 78 | 5 | 73 | 6.4% |
40f8c0s7 | Chorus intensity modulation driven by time‐varying field‐aligned low‐energy plasma | 78 | 2 | 76 | 2.6% |
3m22m0rx | Polar and mid-latitude vortices and zonal flows on Jupiter and Saturn | 76 | 8 | 68 | 10.5% |
0f86k0q7 | The influence of temperature and seawater carbonate saturation state on <sup>13</sup>C–<sup>18</sup>O bond ordering in bivalve mollusks | 75 | 3 | 72 | 4.0% |
1b7778b5 | Ideas and perspectives: A strategic assessment of methane and nitrous oxide measurements in the marine environment | 75 | 1 | 74 | 1.3% |
37d352q9 | Unravelling the large-scale circulation modes in turbulent Rayleigh-Bénard convection (a) Contribution to the Focus Issue Turbulent Thermal Convection edited by Mahendra Verma and Jörg Schumacher. | 75 | 3 | 72 | 4.0% |
5bm6n165 | On the theory of core-mantle coupling | 75 | 15 | 60 | 20.0% |
73m7x0zq | Nitrogen fixation in sediments along a depth transect through the Peruvian oxygen minimum zone | 74 | 1 | 73 | 1.4% |
14x4s6kp | Sulfur's impact on core evolution and magnetic field generation on Ganymede | 73 | 2 | 71 | 2.7% |
1mj2r8jn | Experimental pub crawl from Rayleigh–Bénard to magnetostrophic convection | 73 | 6 | 67 | 8.2% |
9jt5d84b | Convection-driven kinematic dynamos at low Rossby and magnetic Prandtl numbers: Single mode solutions | 73 | 1 | 72 | 1.4% |
02w1x7nc | Thermal evidence for Taylor columns in turbulent rotating Rayleigh-Benard convection | 72 | 2 | 70 | 2.8% |
7xq1k8rq | Libration‐driven flows in ellipsoidal shells | 72 | 1 | 71 | 1.4% |
7sr6v0fw | Regimes of Coriolis-Centrifugal Convection | 71 | 0 | 71 | 0.0% |
7361k8c5 | Anomalous rotation of the inner core and the toroidal magnetic field | 70 | 2 | 68 | 2.9% |
7w78r8q4 | Strong zonal winds from thermal convection in a rotating spherical shell | 70 | 2 | 68 | 2.9% |
8xq8z0g8 | Superfast precipitation of energetic electrons in the radiation belts of the Earth | 70 | 4 | 66 | 5.7% |
0gk963r3 | New Perspectives on Ancient Mars | 68 | 48 | 20 | 70.6% |
94r5r998 | OSS (Outer Solar System): a fundamental and planetary physics mission to Neptune, Triton and the Kuiper Belt | 68 | 1 | 67 | 1.5% |
5b65v425 | Temperature limits to deep subseafloor life in the Nankai Trough subduction zone | 66 | 30 | 36 | 45.5% |
0t18v5vf | Accelerating functional materials discovery Insights from geological sciences, data-driven approaches, and computational advances | 65 | 56 | 9 | 86.2% |
6mh8b2t5 | Shape model and surface properties of the OSIRIS-REx target Asteroid (101955) Bennu from radar and lightcurve observations | 62 | 16 | 46 | 25.8% |
97s3x12h | Rotating convective turbulence in Earth and planetary cores | 62 | 39 | 23 | 62.9% |
26p4c1cd | Convective heat transfer and the pattern of thermal emission on the gas giants | 61 | 2 | 59 | 3.3% |
6g8384vk | Evaporation induced <sup>18</sup>O and <sup>13</sup>C enrichment in lake systems: A global perspective on hydrologic balance effects | 51 | 37 | 14 | 72.5% |
18j8b3nz | First observations of core-transiting seismic phases on Mars | 50 | 5 | 45 | 10.0% |
6gg8t63n | Methanogenic Hydrocarbon Degradation: Evidence from Field and Laboratory Studies | 50 | 18 | 32 | 36.0% |
9hz5p0hv | Planck 2015 results | 47 | 28 | 19 | 59.6% |
3z11n3n5 | Ryugus nucleosynthetic heritage from the outskirts of the Solar System. | 45 | 5 | 40 | 11.1% |
27p899qf | Experiments on Rayleigh–Bénard convection, magnetoconvection and rotating magnetoconvection in liquid gallium | 44 | 18 | 26 | 40.9% |
9r11s5p6 | Brines at high pressure and temperature: Thermodynamic, petrologic and geochemical effects | 44 | 17 | 27 | 38.6% |
3x07r0k2 | Water Reservoirs in Small Planetary Bodies: Meteorites, Asteroids, and Comets | 41 | 6 | 35 | 14.6% |
11b387sn | Dehydration melting and the relationship between granites and granulites | 40 | 20 | 20 | 50.0% |
0rd2j5m0 | The Space Physics Environment Data Analysis System (SPEDAS). | 39 | 5 | 34 | 12.8% |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.