Non-adiabatic effects in the solar p-mode oscillations |
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Authors: | Shao-lan Bi Ru-feng Li |
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Institution: | Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China |
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Abstract: | Non-adiabatic effects associated with radiative loss and convective transfer add small imaginary parts to solar p-mode eigenfrequencies. An asymptotic approximation is developed to study the non-adiabatic effects. For the outermost layer where the approximation is not valid, an exact solution of the equation of non-adiabatic oscillation which results in an cigenfunction equation, is used. The inclusion of the non-adiabatic effects reduces the discrepancy between the theory and observations particularly for frequencies above 3.1 mHz. |
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Keywords: | the sun p-mode oscillation non-adiabatic effects |
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