Results 21 to 30 of about 987 (189)
Testing adiabatic models of energetic electron acceleration at dipolarization fronts
Betatron acceleration is commonly cited as a primary accelerator of energetic electrons at dipolarization fronts, and many case studies compare observed energetic electrons measurements to a betatron model.
S. N. F. Chepuri +9 more
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An important question that is being increasingly studied across subdisciplines of Heliophysics is “how do mesoscale phenomena contribute to the global response of the system?” This review paper focuses on this question within two specific but interlinked
Christine Gabrielse +29 more
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Juno Observations of Ion‐Inertial Scale Flux Ropes in the Jovian Magnetotail
Two ion‐inertial scale magnetic flux ropes are identified in the Juno magnetic field measurements in the dawnside Jovian magnetotail. Previously reported plasmoids in this region had typical diameters of several Jovian radii (RJ).
Yash Sarkango +7 more
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Magnetic reconnection is a fundamental process providing topological changes of the magnetic field, reconfiguration of space plasmas and release of energy in key space weather phenomena, solar flares, coronal mass ejections and magnetospheric substorms ...
Mikhail Sitnov +3 more
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Ion distribution functions in magnetotail reconnection: global hybrid-Vlasov simulation results [PDF]
We present results of noon–midnight meridional plane global hybrid-Vlasov simulations of the magnetotail ion dynamics under a steady southward interplanetary magnetic field using the Vlasiator model.
A. Runov +14 more
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Electron‐Scale Measurements of Antidipolarization Front
Antidipolarization fronts (ADFs), usually formed at the leading edge of the tailward reconnection jets in the Earth's magnetotail, are characterized by sharp enhancements of southward magnetic field (negative Bz). The fine structures at electron scale of
Yin Xu +5 more
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The Disturbance Storm Time (Dst) index serves as a critical indicator for quantifying geomagnetic storm intensity; however, the precise contribution of magnetotail currents to its formation remains inadequately characterized.
Jiawen Yue +6 more
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Magnetic Reconnection in the Martian Magnetotail: Occurrence Rate and Impact on Ion Loss
The current sheet is crucial in releasing magnetic free energy in cosmic plasmas via fast magnetic reconnection or wave excitation. This research investigates the characteristics of the Martian tail current sheet by analyzing data acquired from the Mars ...
Lei Wang +6 more
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The Dynamic Response of Jovian Magnetotail Reconnection to Enhanced Solar Wind Ram Pressure
In this study, we employ the Grid Agnostic Magnetohydrodynamic (MHD) for Extended Research Applications (GAMERA), a high-resolving-power, three-dimensional global MHD model, to simulate magnetotail reconnection in Jupiter's magnetosphere.
Junjie Chen +4 more
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The Martian magnetotail is largely controlled by the solar wind (SW) and is modulated by variations in the upstream drivers. However, due to the limitations of single‐spacecraft observations, the effects of SW variations on the Martian magnetotail have ...
Z. Z. Guo +7 more
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