Three-dimensional model of the structure and evolution of coronal mass ejections

Astrophysical Journal

Volumn 567, Issue 2 I, 2002, Pages 1202-1210

  Tokman, M ^a,c   Bellan, P M ^b  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b California Institute of Technology   (United States)

^c UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Methods: numerical; MHD; Sun: corona; Sun: coronal mass ejections (CMEs); Sun: magnetic fields

Indexed keywords

EID: 0001533485     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/338699     Document Type: Article

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