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Lower Bound for Electron Core Beta in the Solar Wind

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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