Dynamics of the overshoot layers and boundary conditions in helioseismology

Details Dynamics of the overshoot layers and boundary conditions in helioseismology Dynamics of the overshoot layers and boundary conditions in helioseismology

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286...37n&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 37-39 (SEE N89-25819 19-92)

Physics

Boundary Conditions, Helioseismology, Photosphere, Solar Atmosphere, Velocity Distribution, Entropy, Nonequilibrium Thermodynamics, Stellar Models

Scientific paper

The variation of the horizontal and the vertical small scale rms velocity with height in the photosphere which shows a minimum in photospheric layers 150 to 200 km above the continuum is considered. In the context of the nonequilibrium thermodynamics it is supposed that the small scale rms velocity variation reflects the variation of the entropy production in these layers. It is proposed that the upper boundary of theoretical helioseismology models should be placed at that height where the entropy production shows its minimum.

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