Conditions of the small oscillations excitation in the different solar models with the mixed core

Details Conditions of the small oscillations excitation in the different solar models with the mixed core Conditions of the small oscillations excitation in the different solar models with the mixed core

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220..197g&link_type=abstract

In ESA The Hydromagnetics of the Sun p 197-198 (SEE N85-25091 14-92)

Physics

Solar Oscillations, Stellar Cores, Stellar Models, Magnetic Dipoles, Quadrupoles, Stellar Structure

Scientific paper

The growth rates of dipole and quadrupole oscillations were calculated in quasi-adiabatic approximation in solar models with mixed core. Some modes have advantages in the excitation at the expense of nuclear reaction energy. The oscillation is great inside the core when the node of the radial displacement is on the mixed core boundary. Such a property of oscillations can help to explain the peculiarity of 160-min oscillation in solar models with mixed cores.

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