Non-linear helioseismology

Details Non-linear helioseismology Non-linear helioseismology

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.209..905p&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 209, Aug. 15, 1984, p. 905-912.

Astronomy and Astrophysics

Astronomy

1

Coupled Modes, Solar Oscillations, Stellar Models, Adiabatic Conditions, Differential Equations, Nonlinear Systems, Power Spectra

Scientific paper

The differential equations for non-linearly coupled radial adiabatic
oscillation modes are integrated for three detailed solar models. In all
experiments the resulting power spectrum of the surface displacement
shows a peak at a long period PL exceeding 2 hr.

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