Application of a new technique for deriving prominence mass from SOHO BIT Fe XII (19.5 nm) absorption features

Astrophysical Journal

Volumn 641, Issue 1 I, 2006, Pages 606-610

  Gilbert, Holly R ^a   Falco, Lauren E ^b   Holzer, Thomas E ^a   Macqueen, R M ^a  

^a NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^b PENNSYLVANIA STATE UNIVERSITY   (United States)

Author keywords

Sun: corona; Sun: prominences; Sun: UV radiation; Techniques: spectroscopic

Indexed keywords

EID: 33745297586     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/500354     Document Type: Article

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