Three-dimensional magnetohydrodynamic simulation of a global solar corona using a temperature distribution map obtained from SOHO EIT measurements

Astrophysical Journal

Volumn 636, Issue 2 II, 2006, Pages

  Hayashi, Keiji ^a   Benevolenskaya, Elena ^a   Hoeksema, Todd ^a   Liu, Yang ^a   Zhao, Xue Pu ^a  

^a STANFORD UNIVERSITY   (United States)

Author keywords

Methods: numerical; MHD; Solar wind; Sun: corona

Indexed keywords

EID: 32044459743     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/500127     Document Type: Article

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