Results 121 to 130 of about 48,383 (235)

Particle Acceleration by Magnetic Reconnection in Geospace. [PDF]

open access: yesSpace Sci Rev, 2023
Oka M   +9 more
europepmc   +1 more source

Plasma Acceleration by Magnetic Tension Forces in the Martian Magnetotail: MAVEN Observations

open access: yesGeophysical Research Letters, Volume 52, Issue 24, 28 December 2025.
Abstract The Martian magnetotail is a dynamic region where several processes contribute to plasma acceleration. Here, we analyze ∼5 ${\sim} 5$ years of Mars Atmosphere and Volatile EvolutioN (MAVEN) data to evaluate the role of magnetic tension forces in driving plasma acceleration within current sheets in the tail. Based on magnetic field measurements,
Norberto Romanelli   +15 more
wiley   +1 more source

The Effect of Current on Magnetic Null Topology during Turbulent Reconnection

open access: gold, 2022
Z. Wang   +7 more
openalex   +1 more source

Global Survey of Whistler Mode Waves in the Earth's Magnetosheath Using THEMIS Observations

open access: yesGeophysical Research Letters, Volume 52, Issue 24, 28 December 2025.
Abstract While it is known that whistler mode emissions are frequently detected in Earth's magnetosheath, their properties and dependence on solar wind conditions are not fully understood yet. In this study, we present the global distribution of whistler mode waves in the magnetosheath and their dependence on solar wind parameters, based on 7 years of ...
Jingxuan Li   +3 more
wiley   +1 more source

Fast magnetic reconnection in highly-extended current sheets at the National Ignition Facility [PDF]

open access: green, 2020
W. Fox   +14 more
openalex   +1 more source

Exploring the Solar Wind-Planetary Interaction at Mars: Implication for Magnetic Reconnection. [PDF]

open access: yesJ Geophys Res Space Phys, 2023
Bowers CF   +7 more
europepmc   +1 more source

Direct observations of pure electron outflow in magnetic reconnection. [PDF]

open access: yesSci Rep, 2022
Sakai K   +23 more
europepmc   +1 more source

Natural Generation of Alfvén Waves from Three-dimensional Bursty Interchange Magnetic Reconnection in the Solar Corona

open access: yesThe Astrophysical Journal Letters
Alfvén waves play a significant role in solar coronal heating, solar wind acceleration, and Alfvénic turbulence formation. As a fundamental process, magnetic reconnection has long been credited as a crucial source of Alfvén waves.
Liping Yang   +12 more
doaj   +1 more source

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