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The role of turbulence in coronal heating and solar wind expansion
Plasma in the Sun's hot corona expands into the heliosphere as a supersonic and highly magnetized solar wind. This paper provides an overview of our current understanding of how the corona is heated and how the solar wind is accelerated. Recent models of magnetohydrodynamic turbulence have prog...
Uloženo v:
| Vydáno v: | Philos Trans A Math Phys Eng Sci |
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| Hlavní autoři: | , , , , , , |
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
The Royal Society Publishing
2015
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| Témata: | |
| On-line přístup: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4394680/ https://ncbi.nlm.nih.gov/pubmed/25848083 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2014.0148 |
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