Differential rotation in the solar interior

Details Differential rotation in the solar interior Differential rotation in the solar interior

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..149c&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 149-153 (SEE N89-25819 19-92)

Computer Science

Numerical Analysis

47

Angular Velocity, Solar Atmosphere, Solar Interior, Solar Rotation, Depth, Latitude, Numerical Analysis, Solar Observatories

Scientific paper

The angular velocity in the outer half of the Sun was estimated as a function of depth and latitude by applying inversion by means of optimally localized averages to rotational splitting coefficients. The results indicate that the surface differential rotation persists through the convection zone; beneath the convection zone there appears to be a transition, which occurs within the resolution width of 0.1R, to solid-body rotation. It was not possible to perform the inversion in the core, due to the lack of adequate data for modes of low degree.

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