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Lower Bound for Electron Core Beta in the Solar Wind
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Lower Bound for Electron Core Beta in the Solar Wind
Gary, S. P.
;
Newbury, J. A.
;
Goldstein, B. E.
URI:
http://hdl.handle.net/2014/19283
Date:
1998-03
Citation:
Journal of Geophysical Research
USA
Abstract:
Solar wind electrons, especially under conditions of relatively low speed flow, often can be represented as two bi-Maxwellian components, a cooler more dense core (denoted by the subscript c) and a hotter more tenuous halo.
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JPL TRS 1992+
JPL TRS 1992+
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