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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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| Publicado no: | Astrophys J Lett |
|---|---|
| Main Authors: | , , , , , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
2019
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| Assuntos: | |
| Acesso em linha: | 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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