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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...

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Detalhes bibliográficos
Publicado no:Philos Trans A Math Phys Eng Sci
Main Authors: Cranmer, Steven R., Asgari-Targhi, Mahboubeh, Miralles, Mari Paz, Raymond, John C., Strachan, Leonard, Tian, Hui, Woolsey, Lauren N.
Formato: Artigo
Idioma:Inglês
Publicado em: The Royal Society Publishing 2015
Assuntos:
Acesso em linha: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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