The resolving power of current helioseismic inversions for the sun's internal rotation

Details The resolving power of current helioseismic inversions for the sun's internal rotation The resolving power of current helioseismic inversions for the sun's internal rotation

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...385l..59s&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 385, Feb. 1, 1992, p. L59-L62. Research supported by SNFO, Danish

Physics

22

Helioseismology, Solar Interior, Solar Physics, Solar Rotation, Temporal Resolution, Kernel Functions, Solar Oscillations, Weighting Functions

Scientific paper

An inversion of the currently available rotational splitting data which is representative of other recent inversions for the sun's internal rotation is analyzed. The so-called polar rate is found to be an extrapolation from lower latitudes. The basic conclusion that the average radial gradient of the rotation rate in the solar convection zone is small is corroborated.

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