On the thermal surface boundary condition for solar pulsations

Details On the thermal surface boundary condition for solar pulsations On the thermal surface boundary condition for solar pulsations

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..621g&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 621-622 (SEE N89-25819 19-92)

Computer Science

Numerical Analysis

Boundary Conditions, Boundary Value Problems, Solar Oscillations, Solar Physics, Solar Spectra, Stellar Oscillations, Eddington Approximation, Numerical Analysis, Pulses, Solar Limb

Scientific paper

The numerical coefficient which appears in the thermal surface boundary
condition of radial and nonradial oscillations is computed for the Sun.
Values for different values of l and R are listed.

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