Electromagnetic Ion/Beam Instabilities In The Fast Solar Wind: Proton Core Temperature Anisotropy Effects On The Relative Drift Speed And Ion Heating

Ion velocity distributions in the fast solar wind are usually characterized by nonthermal features such as multicomponent ions, temperature anisotropies and average relative drifts. These nonthermal features lead to the growth of several electromagnetic instabilities. Here, two-dimensional hybrid si...

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Bibliographische Detailangaben

Hauptverfasser:	Araneda, J A, Vinas, A F, Astudillo, H F
Format:	Tagungsbericht
Sprache:	eng
Online-Zugang:	Volltext
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