Particle-in-cell Simulations of the Whistler Heat-flux Instability in Solar Wind Conditions.

López, R A; Shaaban, S M; Lazar, M; Poedts, S; Yoon, P H; Micera, A; Lapenta, G

López, R A; Shaaban, S M; Lazar, M; Poedts, S; Yoon, P H; Micera, A; Lapenta, G.

Afiliação

López RA; Centre for mathematical Plasma Astrophysics, KU Leuven, Celestijnenlaan 200B, B-3001 Leuven, Belgium.
Shaaban SM; Centre for mathematical Plasma Astrophysics, KU Leuven, Celestijnenlaan 200B, B-3001 Leuven, Belgium.
Lazar M; Theoretical Physics Research Group, Physics Department, Faculty of Science, Mansoura University, 35516, Mansoura, Egypt.
Poedts S; Centre for mathematical Plasma Astrophysics, KU Leuven, Celestijnenlaan 200B, B-3001 Leuven, Belgium.
Yoon PH; Institut für Theoretische Physik, Lehrstuhl IV: Weltraum- und Astrophysik, Ruhr-Universität Bochum, D-44780 Bochum, Germany.
Micera A; Centre for mathematical Plasma Astrophysics, KU Leuven, Celestijnenlaan 200B, B-3001 Leuven, Belgium.
Lapenta G; Institute for Physical Science and Technology, University of Maryland, College Park, MD, USA.

Astrophys J Lett ; 882(1)2019.

Article em En | MEDLINE | ID: mdl-32042401

Palavras-chave

instabilities; interplanetary medium; methods: numerical; plasmas; solar wind; waves

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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Revista: Astrophys J Lett Ano de publicação: 2019 Tipo de documento: Article País de afiliação: Bélgica

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