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Proton temperature anisotropy instabilities in the solar wind

Gary, S. Peter ; Montgomery, M. D. ; Feldman, W. C. ; Forslund, D. W.

J. Geophys. Res.; (United States), 1976-03, Vol.81 (7), p.1241-1246 [Periódico revisado por pares]

United States: Blackwell Publishing Ltd

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Título:
Proton temperature anisotropy instabilities in the solar wind
Autor: Gary, S. Peter ; Montgomery, M. D. ; Feldman, W. C. ; Forslund, D. W.
Assuntos: 640104 - Astrophysics & Cosmology- Solar Phenomena ; ANISOTROPY ; BARYONS ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; CYCLOTRON INSTABILITY ; ELEMENTARY PARTICLES ; FERMIONS ; HADRONS ; HOSE INSTABILITY ; INSTABILITY ; NUCLEONS ; PLASMA INSTABILITY ; PLASMA MICROINSTABILITIES ; PLASMA SIMULATION ; PROTON DENSITY ; PROTON TEMPERATURE ; PROTONS ; SOLAR ACTIVITY ; SOLAR WIND
É parte de: J. Geophys. Res.; (United States), 1976-03, Vol.81 (7), p.1241-1246
Notas: ark:/67375/WNG-64PHCS6M-G
ArticleID:JGR10413
istex:A8ADEE1854281418E67DA55394B3F00EE1AD67F3
ObjectType-Article-2
SourceType-Scholarly Journals-1
ObjectType-Feature-1
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Descrição: The linear dispersion properties of proton temperature anisotropy instabilities in a homogeneous infinite Vlasov plasma are studied by using a configuration appropriate to the solar wind at 1 AU. The proton distribution is taken to consist of two components, a cooler T⊥ > T∥ ‘core’ and a hotter T∥ > T⊥ ‘halo.’ For the parameters considered the k∥B0 fire hose and ion cyclotron instabilities are the most important modes. Resonant proton effects enhance both instabilities, and the presence of the cooler component can substantially reduce the threshold anisotropy of the halo‐driven fire hose.
Editor: United States: Blackwell Publishing Ltd
Idioma: Inglês

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Proton temperature anisotropy instabilities in the solar wind

Gary, S. Peter ; Montgomery, M. D. ; Feldman, W. C. ; Forslund, D. W.

United States: Blackwell Publishing Ltd

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