Non-adiabatic effects in the solar p-mode oscillations

Details Non-adiabatic effects in the solar p-mode oscillations Non-adiabatic effects in the solar p-mode oscillations

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cha%26a..21..474b&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 21, Issue 4, p. 474-480.

Astronomy and Astrophysics

Astrophysics

Scientific paper

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 eigenfunction 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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