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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...
में बचाया:
| में प्रकाशित: | Philos Trans A Math Phys Eng Sci |
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| मुख्य लेखकों: | , , , |
| स्वरूप: | Artigo |
| भाषा: | Inglês |
| प्रकाशित: |
The Royal Society Publishing
2015
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| विषय: | |
| ऑनलाइन पहुंच: | 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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