Using oscillation data to probe the internal rotation and magnetism of the Sun

Details Using oscillation data to probe the internal rotation and magnetism of the Sun Using oscillation data to probe the internal rotation and magnetism of the Sun

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..259d&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 259-263 (SEE N89-25819 19-92)

Physics

Solar Interior, Solar Magnetic Field, Solar Oscillations, Solar Rotation, Fine Structure, Helioseismology, Solar Cycles

Scientific paper

Integral equations relating the rotation rate and the toroidal field intensity to the parameters describing fine structure in the frequency spectra are discussed. Solutions of the inverse problem for the rotation are presented. Features which may be relevant to the magnetic activity were found in the radial dependence of the rotation rate. Evidence exists for changes with the solar cycle. There is no clear signature of direct effect of magnetism in the observed fine structure.

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