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Dissipation and heating in solar wind turbulence: from the macro to the micro and back again
The past decade has seen a flurry of research activity focused on discerning the physics of kinetic scale turbulence in high-speed astrophysical plasma flows. By ‘kinetic’ we mean spatial scales on the order of or, in particular, smaller than the ion inertial length or the ion gyro-radius—the spatia...
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| 出版年: | Philos Trans A Math Phys Eng Sci |
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| 主要な著者: | , , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
The Royal Society Publishing
2015
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| 主題: | |
| オンライン･アクセス: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4394685/ https://ncbi.nlm.nih.gov/pubmed/25848077 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2014.0155 |
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