A comparison of solar p-mode parameters from the Michelson doppler imager and the global oscillation network group: Splitting coefficients and rotation inversions

Astrophysical Journal

Volumn 567, Issue 2 I, 2002, Pages 1234-1249

  Schou, J ^a   Howe, R ^b   Basu, S ^c   Christensen Dalsgaard, J ^d   Corbard, T ^e   Hill, F ^b   Komm, R ^b   Larsen, R M ^a   Rabello Soares, M C ^a   Thompson, M J ^e  

^a STANFORD UNIVERSITY   (United States)

^b NATIONAL SOLAR OBSERVATORY   (United States)

^c YALE UNIVERSITY   (United States)

^d AARHUS UNIVERSITY   (Denmark)

^e IMPERIAL COLLEGE LONDON   (United Kingdom)

Author keywords

Methods: data analysis; Sun: interior Sun : oscillations; Sun: rotation

Indexed keywords

EID: 0043150162     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/338665     Document Type: Article

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