Solar internal rotation from helioseismology

Details Solar internal rotation from helioseismology Solar internal rotation from helioseismology

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286...55h&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 55-66 (SEE N89-25819 19-92)

Physics

21

Helioseismology, Solar Activity, Solar Interior, Solar Rotation, Time Functions, Frequency Ranges, Solar Gravitation, Solar Oscillations

Scientific paper

Observations of solar oscillations were used to determine the properties of internal solar rotation. Measurements of p-mode frequencies made by several groups are in essential agreement that rotation within the convection zone differs in depth and latitude only slightly from the observed rotation of the surface. Deeper layers seem to rotate with less latitudinal differential rotation. The rotation of the energy-generating core is not well determined by p-mode oscillations and it may be rotating faster or at the same rate as the surface. Observations of g-modes support the notion of a rapidly rotating core.

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