Extended MHD modeling of the steady solar corona and the solar wind

Extended MHD modeling of the steady solar corona and the solar wind

Abstract The history and present state of large-scale magnetohydrodynamic modeling of the solar corona and the solar wind with steady or quasi-steady coronal physics is reviewed. We put the evolution of ideas leading to the recognition of the existence of an expanding solar atmosphere into historica...

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Bibliographic Details
Main Authors: Tamas I. Gombosi, Bart van der Holst, Ward B. Manchester, Igor V. Sokolov
Format: Article
Language:English
Published: Springer 2018-07-01
Series:Living Reviews in Solar Physics
Subjects:
Sun
Solar wind
MHD
Global simulations
Space weather
Online Access:http://link.springer.com/article/10.1007/s41116-018-0014-4

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http://link.springer.com/article/10.1007/s41116-018-0014-4

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