Results 141 to 150 of about 39,453 (210)

Orthogonal Electrodynamics in Multipole Magnetic Fields

open access: yesJournal of Geophysical Research: Space Physics, Volume 130, Issue 7, July 2025.
Abstract Electrodynamics investigations of plasma‐neutral interactions require basis vectors that bridge geographic and geomagnetic coordinates. We present the first orthogonal basis vectors and coordinates for multipole magnetic fields that facilitates mapping geophysical parameters along magnetic field‐lines.
R. A. Stoneback   +3 more
wiley   +1 more source

Global Structure of the Cislunar Magnetotail and Its Evolution During Substorms

open access: yesJournal of Geophysical Research: Space Physics, Volume 130, Issue 7, July 2025.
Abstract So far, the structure and dynamics of the terrestrial magnetotail have largely been investigated within 31RE $31{R}_{E}$ (RE ${R}_{E}$ is the Earth's radius) because of the lack of in‐situ observations beyond that distance, as well as limitations of earlier empirical models.
M. I. Sitnov   +4 more
wiley   +1 more source

Solar wind erosion of lunar regolith is suppressed by surface morphology and regolith properties. [PDF]

open access: yesCommun Earth Environ
Brötzner J   +14 more
europepmc   +1 more source

Atmospheric CO2 Ice in the Martian Polar Regions: Physical and Spectral Properties From Mars Climate Sounder Observations

open access: yesJournal of Geophysical Research: Planets, Volume 130, Issue 7, July 2025.
Abstract CO2 ${\text{CO}}_{2}$ ice clouds are important for polar energy balance and the carbon dioxide cycle on Mars. However, uncertainties remain regarding their physical and radiative properties, which control how polar CO2 ${\text{CO}}_{2}$ clouds interact with the global Martian climate.
R. W. Stevens   +3 more
wiley   +1 more source

Global Lunar Boulder Map From LRO NAC Optical Images Using Deep Learning: Implications for Regolith and Protolith

open access: yesJournal of Geophysical Research: Planets, Volume 130, Issue 7, July 2025.
Abstract Boulders on the lunar surface indicate relatively recent surface activity, related to mass wasting or bedrock excavation by impact cratering, and degrade over time, producing regolith. Previously, the distribution of boulders was indirectly assessed using the anisothermality effects observed by the Lunar Reconnaissance Orbiter (LRO) Diviner ...
B. Aussel   +5 more
wiley   +1 more source

The Seismogenic Thickness of Venus

open access: yesJournal of Geophysical Research: Planets, Volume 130, Issue 7, July 2025.
Abstract Growing evidence that volcanism is currently ongoing on Venus suggests that the sister planet of the Earth may also be seismically active. Given the success of seismic measurements on Mars and the Moon to reveal the interior structure of these bodies, seismic investigations on Venus are a natural next step.
Julia S. Maia   +12 more
wiley   +1 more source

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