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Volumn 464, Issue 1, 2007, Pages 341-349

How does the shape and thickness of the tachocline affect the distribution of the toroidal magnetic fields in the solar dynamo?

Author keywords

Sun: magnetic fields; Sun: transition region

Indexed keywords

KINEMATICS; MAGNETIC FIELDS; MAGNETIC FLUIDS; MATHEMATICAL MODELS; SOLAR RADIATION;

EID: 33947125122     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065834     Document Type: Article
Times cited : (39)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.