Self-consistent magnetohydrodynamic modeling of a coronal mass ejection, coronal dimming, and a giant cusp-shaped arcade formation

Astrophysical Journal

Volumn 634, Issue 1 I, 2005, Pages 663-678

  Shiota, Daikou ^a   Isobe, Hiroaki ^b   Chen, P F ^c   Yamamoto, Tetsuya T ^b   Sakajiri, Takuma ^a   Shibata, Kazunari ^a  

^a KYOTO UNIVERSITY   (Japan)

^b UNIVERSITY OF TOKYO   (Japan)

^c NANJING UNIVERSITY   (China)

Author keywords

Conduction; MHD; Shock waves; Sun: corona; Sun: coronal mass ejections (CMEs)

Indexed keywords

EID: 29144465067     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/496943     Document Type: Article

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