First View of the Solar Core from GOLF Acoustic Modes

Bibcode
1997SoPh..175..247T
DOI
10.1023/A:1004992727541
Turck-Chièze, S.; Basu, S.; Brun, A. S.; Christensen-Dalsgaard, J.; Eff-Darwich, A.; Lopes, I.; Pérez Hernández, F.; Berthomieu, G.; Provost, J.; Ulrich, R. K.; Baudin, F.; Boumier, P.; Charra, J.; Gabriel, A. H.; Garcia, R. A.; Grec, G.; Renaud, C.; Robillot, J. M.; Roca-Cortés, T.
Referencia bibliográfica

Solar Physics, Volume 175, Issue 2, pp.247-265

Fecha de publicación:
10
1997
Revista
Solar Physics
Número de autores
19
Número de autores del IAC
3
Número de citas
74
Número de citas referidas
52
Descripción
After 8 months of nearly continuous measurements the GOLF instrument, aboard SOHO, has detected acoustic mode frequencies of more than 100 modes, extending from 1.4 mHz to 4.9 mHz. In this paper, we compare these results with the best available predictions coming from solar models. To verify the quality of the data, we examine the asymptotic seismic parameters; this confirms the improvements achieved in solar models during the last decade.
Tipo
Con árbitro

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