Physical conditions in a coronal mass ejection from hinode, stereo, and soho observations

Astrophysical Journal

Volumn 711, Issue 1, 2010, Pages 75-98

  Landi, E ^a   Raymond, J C ^b   Miralles, M P ^b   Hara, H ^c  

^a NAVAL RESEARCH LABORATORY   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

Sun: activity; Sun: corona; Sun: coronal mass ejections (CMEs); Sun: UV radiation; Techniques: spectroscopic

Indexed keywords

EID: 76949095075     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/711/1/75     Document Type: Article

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