Proton core temperature effects on the relative drift and anisotropy evolution of the ion beam instability in the fast solar wind

Typical nonthermal features of ion velocity distributions observed in the fast solar wind are the relative streaming between two proton components, an alpha/proton relative flow, and anisotropic proton cores with T⟂p > T∥p, where the subscripts denote directions relative to the background magneti...

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Bibliographic Details

Published in:	Journal of Geophysical Research - Space Physics Vol. 107; no. A12; pp. SSH 8-1 - SSH 8-10
Main Authors:	Araneda, Jaime A., Viñas, Adolfo F., Astudillo, Hernán F.
Format:	Journal Article
Language:	English
Published:	American Geophysical Union 01-12-2002 Blackwell Publishing Ltd
Subjects:	fast solar wind Interplanetary Physics ion-beam instabilities ion-cyclotron modes Numerical simulation studies plasma waves preferential heating Solar wind plasma Space Plasma Physics temperature anisotropy Wave/particle interactions Waves and instabilities
Online Access:	Get full text
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