Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-11-02
Astrophys. J. 531 (2000) 1088
Astronomy and Astrophysics
Astrophysics
To appear in ApJ
Scientific paper
10.1086/308514
Most helioseismic analyses are based on solar oscillations frequencies obtained by fitting symmetric peak profiles to the power spectra. However, it has now been demonstrated that the peaks are not symmetric. In this work we study the effects of asymmetry of the peak profiles on the solar oscillations frequencies of p-modes for low and intermediate degrees. We also investigate how the resulting shift in frequencies affects helioseismic inferences.
Antia H. M.
Basu Sarbani
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