Helioseismic tests of a new category of solar models

Details Helioseismic tests of a new category of solar models Helioseismic tests of a new category of solar models

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.508...83l&link_type=abstract

In: Proceedings of the SOHO 11 Symposium on From Solar Min to Max: Half a Solar Cycle with SOHO, 11-15 March 2002, Davos, Switze

Other

2

Sun: Oscillations, Sun: Magnetic Fields, Sun: Interior

Scientific paper

We have constructed a series of solar models that unlike others which treat the effects of magnetic fields as a perturbation, incorporate the effect of magnetic fields into the stellar structure equations. Such models can reproduce the observed irradiance and effective temperature variations of the Sun. We study the helioseismic properties of these models representing different epochs of the solar cycle. In particular we examine whether the frequency differences between the models reproduce the observed solar-cycle related change of solar oscillation frequencies.

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