Physics
Scientific paper
May 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980cpsp.book..677k&link_type=abstract
In NASA. Goddard Space Flight Center Current Probl. in Stellar Pulsation Instabilities p 677-694 (SEE N80-25229 15-90)
Physics
Atmospheric Models, Flux Density, Oscillations, Power Spectra, Solar Spectra, Boundary Value Problems, Periodic Variations, Spherical Harmonics, Temperature Distribution
Scientific paper
The observed power spectrum of the solar five minute oscillations is discussed from the viewpoint that the oscillations are excited by turbulent convection. The observations place significant constraints on the theory and suggest constraints on the solar model structure. It is shown that the steep low frequency side of the peak in the power spectrum is more readily explained if the mixing length is greater than one scale height. The high frequency end of the power spectrum is also discussed.
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