Results 11 to 20 of about 282,550 (204)

The 600 keV electron injections in the Earth’s outer radiation belt: A statistical study

open access: yesEarth and Planetary Physics, 2022
Relativistic electron injections are one of the mechanisms of relativistic (≥0.5 MeV) electron enhancements in the Earth’s outer radiation belt. In this study, we present a statistical observation of 600 keV electron injections in the outer radiation ...
ChaoLing Tang   +4 more
doaj   +1 more source

Energetic Electron Flux Predictions in the Near‐Earth Plasma Sheet From Solar Wind Driving

open access: yesSpace Weather, 2022
Suprathermal electrons in the near‐Earth plasma sheet are important for inner magnetosphere considerations. They are the source population for outer radiation belt electrons and they pose risks to geosynchronous satellites through their contribution to ...
B. M. Swiger   +3 more
doaj   +1 more source

Cluster electron observations of the separatrix layer during traveling compression regions [PDF]

open access: yes, 2005
[ 1] We present Cluster 4-point observations of electrons during traveling compression regions ( TCRs) on 19 September 2001. The electron and \B\ signatures vary with distance from the plasma sheet, confirming that transient plasma sheet bulges propagate
Balogh, A   +4 more
core   +1 more source

Modeling and Prediction of Near-Earth Plasma Sheet Parameters Using the Rice Convection Model and the Recurrent Neural Network

open access: yesFrontiers in Astronomy and Space Sciences, 2021
Interaction between Earth’s magnetotail and its inner magnetosphere plays an important role in the transport of mass and energy in the ionosphere–magnetosphere coupled system.
Shishir Priyadarshi   +3 more
doaj   +1 more source

Contributions of the low-latitude boundary layer to the finite width magnetotail convection model [PDF]

open access: yes, 1993
Convection of plasma within the terrestrial nightside plasma sheet contributes to the structure and, possibly, the dynamical evolution of the magnetotail.
Kivelson, M. G., Spence, Harlan E.
core   +2 more sources

Magnetic Turbulence Associated with Magnetic Dipolarizations in the Near-Tail of the Earth’s Magnetosphere: Test of Anisotropy [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2011
In this paper, the anisotropic nature of the magnetic turbulence associated with magnetic dipolarizations in the Earth’s plasma sheet is examined. Specifically, we determine the power spectral indices for the perpendicular and parallel components of ...
Ji- Hee Lee   +4 more
doaj   +1 more source

SIMULATION STUDY OF THE ENERGETIC NEUTRAL ATOM (ENA) IMAGING MONITORING OF THE GEOMAGNETOSPHERE ON A LUNAR BASE

open access: yesSolar-Terrestrial Physics, 2021
Since the moon’s revolution cycle is exactly the same as its rotation cycle, we can only see the moon always facing Earth in the same direction. Based on the clean particle radiation environment of the moon, a neutral atomic telemetry base station could ...
Li Lu   +6 more
doaj   +1 more source

Particle-in-cell simulations of collisionless magnetic reconnection with a non-uniform guide field [PDF]

open access: yes, 2015
Results are presented of a first study of collisionless magnetic reconnection starting from a recently found exact nonlinear force-free Vlasov–Maxwell equilibrium.
Harrison, M. G.   +4 more
core   +5 more sources

New Results From Galileo's First Flyby of Ganymede: Reconnection‐Driven Flows at the Low‐Latitude Magnetopause Boundary, Crossing the Cusp, and Icy Ionospheric Escape

open access: yesGeophysical Research Letters, 2018
On 27 June 1996, the NASA Galileo spacecraft made humanity's first flyby of Jupiter's largest moon, Ganymede, discovering that it is the only moon known to possess an internally generated magnetic field. Resurrecting the original Galileo Plasma Subsystem
Glyn Collinson   +6 more
doaj   +1 more source

Improvement of Plasma Sheet Neural Network Accuracy With Inclusion of Physical Information

open access: yesFrontiers in Astronomy and Space Sciences, 2020
The near-Earth plasma sheet is the source for electrons in the inner magnetosphere. The coupling between the solar wind and the near-Earth plasma sheet is dominated by non-linear processes, making any relationship difficult to infer.
Brian M. Swiger   +3 more
doaj   +1 more source

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