Results 111 to 120 of about 48,383 (235)

Modulation of Electron Rolling‐Pin Distribution Behind Anti‐Dipolarization Front

open access: yesGeophysical Research Letters, Volume 52, Issue 24, 28 December 2025.
Abstract The electron rolling pin distribution, showing electron pitch angles primarily at 0°, 90°, and 180°, has been recently observed behind dipolarization fronts (DFs) in the magnetosphere of Earth. However, the relation between such distribution and the leading edge of tailward magnetic reconnection jets, also known as anti‐dipolarization fronts ...
W. Z. Zhang   +4 more
wiley   +1 more source

MMS Observations of a Compressed, Strongly Driven Magnetopause During the 2024 Mother's Day Storm

open access: yesGeophysical Research Letters, Volume 52, Issue 24, 28 December 2025.
Abstract From 10 to 12 May 2024, a series of coronal mass ejections led to one of the strongest geomagnetic storms of the century, referred to as the Mother's Day or Gannon Storm. MMS's position on the dayside magnetosphere on 11 May provided observations of a strongly driven and compressed ∼7RE $\left(\sim 7\ {R}_{E}\right)$ reconnecting magnetopause.
Jason M. H. Beedle   +19 more
wiley   +1 more source

Detection of High‐Latitude Magnetic Reconnection Between the Northward Interplanetary Magnetic Field and a Closed Magnetic Field Wedge Linked to a Transpolar Arc

open access: yesGeophysical Research Letters, Volume 52, Issue 24, 28 December 2025.
Abstract Transpolar arcs (TPAs) describe a subset of auroral emissions observed poleward of the Earth's main auroral ovals when the interplanetary magnetic field (IMF) is northward. These emissions are thought to align with a “wedge” of closed magnetic field lines extending to the high‐latitude boundary of the Earth's magnetosphere, where they are ...
Nawapat Kaweeyanun   +8 more
wiley   +1 more source

Flux-rope-mediated Turbulent Magnetic Reconnection

open access: yesThe Astrophysical Journal
We present a new model of magnetic reconnection in the presence of turbulence. The new model differs from the Lazarian–Vishniac turbulent reconnection theory by emphasizing the role of locally coherent magnetic structures, whose existence is shown to be ...
Alexander J. B. Russell
doaj   +1 more source

Being on time in magnetic reconnection [PDF]

open access: gold, 2009
M. Faganello   +2 more
openalex   +1 more source

Energetic Electron Spectra at Low Altitudes: Transition From the Plasma Sheet to the Outer Radiation Belt

open access: yesGeophysical Research Letters, Volume 52, Issue 24, 28 December 2025.
Abstract Low‐altitude measurements of energetic electron fluxes offer insight into the dynamics of the radiation belts and plasma sheet. However, distinguishing between key magnetospheric regions–such as inner belt, slot region, outer belt, and plasma sheet–based on low‐altitude data remains challenging, particularly for missions lacking pitch‐angle ...
Weiqin Sun   +7 more
wiley   +1 more source

Magnetic reconnection as the driving factor behind high-mass protostellar luminosity flares

open access: yesCommunications Physics
Magnetic reconnection, a critical process in astrophysical luminosity outbursts like solar flares, may also underpin such events in high-mass young stellar objects (HMYSOs).
Xi Chen   +14 more
doaj   +1 more source

Laboratory Study of Collisionless Magnetic Reconnection. [PDF]

open access: yesSpace Sci Rev, 2023
Ji H   +15 more
europepmc   +1 more source

Solar Energetic Particle Events During May 2024 Geomagnetic Superstorm

open access: yesGeophysical Research Letters, Volume 52, Issue 24, 28 December 2025.
Abstract Three solar energetic particle (SEP) events originating from solar active region 13664 occurred on 10–16 May 2024, coinciding with a geomagnetic superstorm. Using data from the Geostationary Operational Environmental Satellites and Meteorological Operational satellite‐C, we investigate the energetic proton fluxes and east‐west flux ratios in ...
Zhenghao She   +7 more
wiley   +1 more source

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