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

In collision-poor plasmas from space, e.g., solar wind or stellar outflows, the heat flux carried by the strahl or beaming electrons is expected to be regulated by the self-generated instabilities. Recently, simultaneous field and particle observations have indeed revealed enhanced whistler-like flu...

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書誌詳細
出版年:Astrophys J Lett
主要な著者: López, R. A., Shaaban, S. M., Lazar, M., Poedts, S., Yoon, P. H., Micera, A., Lapenta, G.
フォーマット: Artigo
言語:Inglês
出版事項: 2019
主題:
オンライン・アクセス:https://ncbi.nlm.nih.gov/pmc/articles/PMC7008930/
https://ncbi.nlm.nih.gov/pubmed/32042401
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3847/2041-8213/ab398b
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