Forward modeling of the corona of the sun and solar-like stars: From a three-dimensional magnetohydrodynamic model to synthetic extreme-ultraviolet spectra

Astrophysical Journal

Volumn 638, Issue 2 I, 2006, Pages 1086-1100

  Peter, Hardi ^a   Gudiksen, Boris V ^b   Nordlund, Åke ^c  

^a KIEPENHEUER INSTITUT FÜR SONNENPHYSIK   (Germany)

^b UNIVERSITY OF OSLO   (Norway)

^c UNIVERSITY OF COPENHAGEN   (Denmark)

Author keywords

MHD; Stars: coronae; Sun: corona; Sun: UV radiation

Indexed keywords

EID: 33644758291     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/499117     Document Type: Article

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