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On the Velocity and Intensity Asymmetries of Solar P-Mode Lines
Authors:M. Gabriel
Affiliation:(1) Institut d'Astrophysique, 5 Av. de Cointe, B-4000 Liège, Belgium
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.
Keywords:solar oscillations
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