On the Velocity and Intensity Asymmetries of Solar P-Mode Lines |
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Authors: | M. Gabriel |
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Affiliation: | (1) Institut d'Astrophysique, 5 Av. de Cointe, B-4000 Liège, Belgium |
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Abstract: | We show that to explain the opposite line asymmetries shown by the velocity and intensity spectra, it is necessary to solve the full non-adiabatic problem which is at least of the fourth order. This revised version was published online in June 2006 with corrections to the Cover Date. |
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Keywords: | solar oscillations |
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