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Volumn 464, Issue 1, 2007, Pages 357-365

An empirical 3D model of the large-scale coronal structure based on the distribution of Hα filaments on the solar disk

Author keywords

Sun: corona; Sun: filaments; Sun: prominences

Indexed keywords

CONVERGENCE OF NUMERICAL METHODS; GALAXIES; MAPS; MATHEMATICAL MODELS; SURFACE STRUCTURE;

EID: 33947114435     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066482     Document Type: Article
Times cited : (21)

References (41)
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    • Noci, G., Kohl, J. L., Antonucci, E., et al. 1997a, in Fifth SOHO Workshop: The Corona and Solar Wind Near Minimum Activity, ed. A. Wilson, ESA SP-404, 75
    • Noci, G., Kohl, J. L., Antonucci, E., et al. 1997a, in Fifth SOHO Workshop: The Corona and Solar Wind Near Minimum Activity, ed. A. Wilson, ESA SP-404, 75


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.