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Volumn 757, Issue 2, 2012, Pages

A method for data-driven simulations of evolving solar active regions

Author keywords

magnetic fields; magnetohydrodynamics (MHD); Sun: corona; Sun: coronal mass ejections (CMEs); Sun: evolution; Sun: photosphere

Indexed keywords


EID: 84866403631     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/757/2/147     Document Type: Article
Times cited : (185)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.