A new technique for deriving prominence mass from SOHO/EIT Fe XII (19.5 nanometers) absorption features

Astrophysical Journal

Volumn 618, Issue 1 I, 2005, Pages 524-536

  Gilbert, Holly R ^a   Holzer, Thomas E ^a   Macqueen, R M ^a  

^a NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

Author keywords

Sun: corona; Sun: coronal mass ejections (CMEs); Sun: prominences

Indexed keywords

EID: 13944266013     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/425975     Document Type: Article

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