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Volumn 251, Issue 1-2, 2008, Pages 135-147

Can we constrain solar interior physics by studying the gravity-mode asymptotic signature?

Author keywords

Helioseismology: Observations; Interior: Radiative zone, core

Indexed keywords


EID: 50249088782     PISSN: 00380938     EISSN: 1573093X     Source Type: Journal    
DOI: 10.1007/s11207-008-9159-y     Document Type: Article
Times cited : (15)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.