The Solar Acoustic Spectrum as Seen by GOLF. III. Asymmetries, Resonant Frequencies and Splittings

Bibcode
1998ESASP.418..329R
Roca-Cortés, T.; Lazrek, M.; Bertello, L.; Thiery, S.; Baudin, F.; Garcia, R. A.; GOLF Team
Bibliographical reference

Structure and Dynamics of the Interior of the Sun and Sun-like Stars SOHO 6/GONG 98 Workshop Abstract, June 1-4, 1998, Boston, Massachusetts, p. 329

Advertised on:
0
1998
Number of authors
7
IAC number of authors
1
Citations
6
Refereed citations
5
Description
The definition of the model to fit to the observed spectra depends on the physics we are assuming is present in the phenomena we are observing. Here we present the results obtained following the fit of several models (described in poster II). Therefore the effects of asymmetrical line shapes, a common background for all modes, fixed relative power in the components of a multiplet and a constant splitting between the components of each multiplet on the resonant frequencies (and their errors) of the modes will be evaluated. Finally, a table of frequencies and splittings will be given.
Type
Non-refereed

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