Nonlinear force-free field modeling of a solar active region around the time of a major flare and coronal mass ejection

Astrophysical Journal

Volumn 675, Issue 2, 2008, Pages 1637-1644

  Schrijver, C J ^a   DeRosa, M L ^a   Metcalf, T ^b   Barnes, G ^b   Lites, B ^c   Tarbell, T ^a   McTiernan, J ^d   Valori, G ^e   Wiegelmann, T ^f   Wheatland, M S ^g   Amari, T ^h   Aulanier, G ⁱ   Demoulin P ⁱ   Fuhrmann, M ^j   Kusano, K ^k   Regnier S ^l   Thalmann, J K ^f  

^a LOCKHEED MARTIN   (United States)

^b Colorado Research Associates ^*  (United States)

^c NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^f MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^g UNIVERSITY OF SYDNEY   (Australia)

^h CENTRE DE PHYSIQUE THÉORIQUE   (France)

ⁱ UNIVERSITÉ PARIS DIDEROT   (France)

^j UNIVERSITY OF POTSDAM   (Germany)

^k JAPAN AGENCY FOR MARINE EARTH SCIENCE AND TECHNOLOGY   (Japan)

^l UNIVERSITY OF ST ANDREWS   (United Kingdom)

more..

Author keywords

Sun: activity; Sun: corona; Sun: flares; Sun: magnetic fields

Indexed keywords

EID: 41049109819     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/527413     Document Type: Article

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