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Kinetic scale turbulence and dissipation in the solar wind: key observational results and future outlook
Turbulence is ubiquitous in the solar wind. Turbulence causes kinetic and magnetic energy to cascade to small scales where they are eventually dissipated, adding heat to the plasma. The details of how this occurs are not well understood. This article reviews the evidence for turbulent dissipation an...
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| Yayımlandı: | Philos Trans A Math Phys Eng Sci |
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| Asıl Yazarlar: | , , , |
| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
The Royal Society Publishing
2015
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| Konular: | |
| Online Erişim: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4394679/ https://ncbi.nlm.nih.gov/pubmed/25848084 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2014.0147 |
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