Comparison of two fitting methods for ring diagram analysis of very high / solar oscillations

Astrophysical Journal

Volumn 485, Issue 2 PART I, 1997, Pages 869-874

  Patron J ^a   Hernández, I González ^a   Chou, Dean Y I ^b   Sun, M T ^b   Mu, T M ^b   Loudagh, S ^b   Bala, B ^b   Chou, Y P ^b   Lin, C H ^b   Huang, I J ^b   Jimenez A ^a   Rabello Soares, M C ^a   Ai, G ^c   Wang, G P ^c   Zirin, H ^d   Marquette, W ^d   Nenow, J ^d   Ehgamberdiev, S ^e   Khalikov, S ^e  

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b NATIONAL TSING HUA UNIVERSITY   (Taiwan)

^c CHINESE ACADEMY OF SCIENCES   (China)

^d NEW JERSEY INSTITUTE OF TECHNOLOGY   (United States)

^e S YU YUNUSOV INSTITUTE OF THE CHEMISTRY OF PLANT SUBSTANCES   (Uzbekistan)

Author keywords

Convection; Methods: numerical; Sun: oscillations

Indexed keywords

EID: 21744432071     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/304469     Document Type: Article

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