Implications of observed frequencies of solar P modes

Details Implications of observed frequencies of solar P modes Implications of observed frequencies of solar P modes

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sses.nasa..199c&link_type=abstract

In JPL Solar Seismology from Space. p 199-204 (SEE N85-25060 14-92)

Other

8

Convection, Errors, Modes (Standing Waves), Power Spectra, Solar Oscillations, Excitation, Frequency Ranges, Spline Functions

Scientific paper

The authors present a preliminary comparison of the observed frequencies of 5-min modes reported by Duvall & Harvey in these proceedings with theoretical frequencies for a traditional solar model. The differences between observations and theory can be understood qualitatively in terms of two separate sources of error in the frequency calculation, one near the solar surface and the other at the base of the convection zone. There is no indication of errors in the deep interior of the model.

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