Results 101 to 110 of about 16,773 (267)

Do Statistical Models Capture the Dynamics of the Magnetopause During Sudden Magnetospheric Compressions? [PDF]

open access: hybrid, 2020
Frances Staples   +11 more
openalex   +1 more source

Magnetosphere of Mars at Almost Radial Interplanetary Magnetic Field

open access: yesJournal of Geophysical Research: Space Physics, Volume 131, Issue 4, April 2026.
Abstract We have studied the structure of the Martian magnetosphere under conditions of an almost radial interplanetary magnetic field (IMF). Under such conditions, the currents driven by the motional electric field −1cVsw×BIMF ${-}\frac{1}{c}{\mathbf{V}}_{sw}\times {\mathbf{B}}_{\mathit{IMF}}$ are expected to be strongly reduced, and the induced ...
E. Dubinin   +9 more
wiley   +1 more source

Superposed Epoch Analysis of Extreme Geomagnetic Disturbances at Auroral Zone Latitudes Over a Solar Cycle

open access: yesJournal of Geophysical Research: Space Physics, Volume 131, Issue 4, April 2026.
Abstract Intense and rapidly changing electrical currents in near‐Earth space produce geomagnetic disturbances (GMDs) with large magnetic field rates of change (dB/dt) and in turn large geomagnetically induced currents (GICs) in nearby power lines and pipelines. This study builds on the work of Engebretson, Yang, et al.
Mark J. Engebretson   +7 more
wiley   +1 more source

Relationship Between Foreshock Structures and Magnetosheath Jets

open access: yesJournal of Geophysical Research: Space Physics, Volume 131, Issue 4, April 2026.
Abstract Plasma structures with enhanced dynamic pressure know as jets are frequently observed in the magnetosheath. We examine a possible connection of these jets with structures reported in the foreshock like SLAMS or plasmoids. A statistical study of the relation of the upstream conditions and the occurrence rates of magnetosheath (MSH) jets and ...
N. Xirogiannopoulou   +3 more
wiley   +1 more source

How Well Can Solar Wind Parameters Predict Outer Radiation Belt Electron Flux?

open access: yesSpace Weather, Volume 24, Issue 4, April 2026.
Abstract The electron flux in the outer radiation belt is primarily governed by interactions between the solar wind and magnetosphere. While geomagnetic indices are widely used for modeling and forecasting, their real‐time availability is limited. In contrast, solar wind parameters can be continuously monitored by a single satellite at the L1 ${L}_{1}$
Yutong Li, Mengli Tan, Xin Tao
wiley   +1 more source

Galactic cosmic rays on extrasolar Earth-like planets I. Cosmic ray flux

open access: yes, 2015
(abridged abstract) Theoretical arguments indicate that close-in terrestial exoplanets may have weak magnetic fields, especially in the case of planets more massive than Earth (super-Earths).
Atri, D.   +4 more
core   +6 more sources

MMS Examination of FTEs at the Earth's Subsolar Magnetopause [PDF]

open access: hybrid, 2018
Mojtaba Akhavan‐Tafti   +11 more
openalex   +1 more source

Global MHD simulations of Saturns's magnetosphere at the time of Cassini approach [PDF]

open access: yes, 2005
We present the results of a 3D global magnetohydrodynamic simulation of the magnetosphere of Saturn for the period of Cassini's initial approach and entry into the magnetosphere. We compare calculated bow shock and magnetopause locations with the Cassini
Achilleos, N   +6 more
core  

Magnetic Fluctuations and Turbulence in the Venus Magnetosheath and Wake

open access: yes, 2008
Recent research has shown that distinct physical regions in the Venusian induced magnetosphere are recognizable from the variations of strength and of wave/fluctuation activity of the magnetic field.
Amerstorfer   +21 more
core   +1 more source

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