Helioseismic tests of solar variability models

Details Helioseismic tests of solar variability models Helioseismic tests of solar variability models

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.517..329l&link_type=abstract

In: Proceedings of SOHO 12 / GONG+ 2002. Local and global helioseismology: the present and future, 27 October - 1 November 2002,

Physics

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

Scientific paper

We construct models of the structure and evolution of the Sun which includes variable magnetic fields and turbulence. The magnetic effects included are: (1) magnetic pressure, (2) magnetic energy, and (3) magnetic modulation of turbulence. The effects of turbulence are: (1) turbulent pressure, (2) turbulent kinetic energy, (3) inhibition of radiative losses from a convective eddy, and (4) generation of magnetic fields. Using these ingredients we construct various types of solar models and test them against helioseismic data. We find that only a solar variability model which includes a magnetically-modulated mechanism to generate turbulence can agree with all the current available observational data.

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