Solar-wind–magnetosphere coupling, including relativistic electron energization, during high-speed streams

High geomagnetic activity occurs continuously during high-speed solar wind streams, and fluxes of relativistic electrons observed at geosynchronous orbit enhance significantly. High-speed streams are preceded by solar wind compression regions, during which time there are large losses of relativistic...

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Veröffentlicht in:	Journal of atmospheric and solar-terrestrial physics 2009-07, Vol.71 (10), p.1059-1072
Hauptverfasser:	Lyons, L.R., Lee, D.-Y., Kim, H.-J., Hwang, J.A., Thorne, R.M., Horne, R.B., Smith, A.J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Earth, ocean, space Exact sciences and technology External geophysics High-speed streams Physics of the ionosphere Physics of the magnetosphere Radiation belt electrons Substorms
Online-Zugang:	Volltext
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