Simulation of entry of shock-drift-accelerated solar energetic protons into the magnetosphere

The entry of solar energetic protons in the energy range from 100 keV to 10 MeV into the Earth's magnetosphere is simulated to examine the effect of shock drift acceleration at the quasi‐perpendicular bow shock. The proton trajectories are traced from the upstream side of the solar wind in time...

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Veröffentlicht in:	Journal of Geophysical Research. A. Space Physics 2005-10, Vol.110 (A10), p.A10105.1-n/a
Hauptverfasser:	Shimazu, Hironori, Tanaka, Takashi
Format:	Artikel
Sprache:	eng
Schlagworte:	Earth sciences Earth, ocean, space Exact sciences and technology shock drift acceleration
Online-Zugang:	Volltext
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