Results 21 to 30 of about 987 (189)

Testing adiabatic models of energetic electron acceleration at dipolarization fronts

open access: yesFrontiers in Astronomy and Space Sciences, 2023
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
doaj   +1 more source

Mesoscale phenomena and their contribution to the global response: a focus on the magnetotail transition region and magnetosphere-ionosphere coupling

open access: yesFrontiers in Astronomy and Space Sciences, 2023
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
doaj   +1 more source

Juno Observations of Ion‐Inertial Scale Flux Ropes in the Jovian Magnetotail

open access: yesGeophysical Research Letters, 2021
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
doaj   +1 more source

Data Mining Reconstruction of Magnetotail Reconnection and Implications for Its First-Principle Modeling

open access: yesFrontiers in Physics, 2021
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
doaj   +1 more source

Ion distribution functions in magnetotail reconnection: global hybrid-Vlasov simulation results [PDF]

open access: yesAnnales Geophysicae, 2021
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
doaj   +1 more source

Electron‐Scale Measurements of Antidipolarization Front

open access: yesGeophysical Research Letters, 2021
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
doaj   +1 more source

Contribution of magnetotail currents to Dst index during different intensity magnetic storms: a global MHD model study

open access: yesFrontiers in Astronomy and Space Sciences
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
doaj   +1 more source

Magnetic Reconnection in the Martian Magnetotail: Occurrence Rate and Impact on Ion Loss

open access: yesGeophysical Research Letters, 2023
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
doaj   +1 more source

The Dynamic Response of Jovian Magnetotail Reconnection to Enhanced Solar Wind Ram Pressure

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

Rapid Response of Martian Magnetotail to Solar Wind Disturbance: Tianwen‐1 and MAVEN Joint Observations

open access: yesGeophysical Research Letters
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
doaj   +1 more source

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