Results 111 to 120 of about 227,323 (221)

Solar Cycle Dynamic of the Martian Induced Magnetosphere. Planetary Ions Acceleration Zones and Escape.

open access: yes, 2015
International audienceThis work presents a massive statistical analysis of the ion flows in the Martian induced magnetosphere. We performed this analysis usingMars Express ion mass spectrometer data taken during 2008 - 20014 time interval.
Fedorov, Andrei   +3 more
core   +2 more sources

Ion‐Scale Characteristics of the Martian Magnetic Pile‐Up Boundary Layer

open access: yesGeophysical Research Letters
The Martian magnetic pile‐up boundary (MPB) delineates the interface between the magnetosheath and the induced magnetosphere, but its global ion‐scale characteristics remaining unclear.
Shibang Li   +12 more
doaj   +1 more source

Neutral Wind Control of Jupiter's Non‐Auroral Ionosphere

open access: yesGeophysical Research Letters, Volume 53, Issue 18, 28 September 2026.
Abstract We use JAMMIES (JAMMIES is Another Model Making Ionospheric EStimates), a new model of Jupiter's non‐auroral ionosphere, to demonstrate that neutral wind‐driven field‐aligned plasma transport can explain decades of measurements inconsistent with a solar‐dominated ionosphere. Two observations highlight these inconsistencies: a minimum in H3+ ${\
K. Mohamed   +7 more
wiley   +1 more source

Signatures of Open Magnetic Flux in Jupiter's Dawnside Magnetotail

open access: yesAGU Advances
Jupiter's magnetosphere exhibits notable distinctions from the terrestrial magnetosphere. The structure and dynamics of Jupiter's dawnside magnetosphere can be characterized as a competition between internally driven sunward flow and solar wind‐driven ...
P. A. Delamere   +17 more
doaj   +1 more source

Observational Analysis on the Relationship Between Chorus Waves and MeV Microburst Electron Precipitation

open access: yesGeophysical Research Letters, Volume 53, Issue 18, 28 September 2026.
Abstract Microbursts are thought to be a key contributor to radiation belt electron loss, with chorus waves considered a primary driver of this precipitation. However, the conditions under which chorus waves produce MeV electron loss remain poorly constrained.
Jorge Romero‐Minaya   +3 more
wiley   +1 more source

IMF By‐Controlled Dawn–Dusk and Hemispheric Asymmetries of Kelvin–Helmholtz Waves and Reconnection Geometry Under Negative Dipole Tilt

open access: yesGeophysical Research Letters, Volume 53, Issue 18, 28 September 2026.
Abstract Along with magnetic reconnection, Kelvin‐Helmholtz (KH) waves are the main mechanisms controlling the solar wind‐magnetosphere interaction, enabling plasma transport into the magnetosphere due to secondary reconnection, diffusion and wave‐particle interactions.
L. Holappa   +3 more
wiley   +1 more source

Chorus Element Repetition: Roles of Energetic Electron Injection and Nonlinear Wave Growth

open access: yesGeophysical Research Letters, Volume 53, Issue 18, 28 September 2026.
Abstract Chorus waves are coherent whistler‐mode emissions in Earth’s magnetosphere and play a key role in the acceleration and loss of radiation belt electrons. Their spectra commonly consist of discrete and repetitive elements, yet the mechanism governing this repetition is not fully understood.
Huayue Chen   +5 more
wiley   +1 more source

A Survey of Magnetic Field Line Curvature in Jovian Dawn Magnetodisc

open access: yesGeophysical Research Letters
The Jovian magnetosphere is highly dynamic, influenced by both solar wind and internal processes associated with the rapid planetary rotation and Io's volcanic activities.
W. D. Gu   +8 more
doaj   +1 more source

Impacts of Tidal Locking on Magnetospheric Energy Input to Exoplanet Atmospheres

open access: yesThe Astrophysical Journal
We investigate the effect of planetary corotation on energy dissipation within the magnetosphere–ionosphere system of exoplanets. Using magnetohydrodynamic simulations, we find that tidally locked exoplanets have a higher cross polar cap potential (CPCP)
Fatemeh Bagheri   +2 more
doaj   +1 more source

Induced magnetosphere of Mars responds fast to interplanetary magnetic field rotation. [PDF]

open access: yesNat Commun
Lin R   +13 more
europepmc   +1 more source

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