Physics
Scientific paper
Jul 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984natur.310...22d&link_type=abstract
Nature (ISSN 0028-0836), vol. 310, July 5, 1984, p. 22-25. NSF-USAF-supported research.
Physics
167
Solar Interior, Solar Oscillations, Solar Rotation, Stellar Cores, Convection, Quadrupoles, Relativity, Stellar Spectra
Scientific paper
The frequency difference between prograde and retrograde sectoral solar oscillations is analysed to determine the rotation rate of the solar interior, assuming no latitudinal dependence. Much of the solar interior rotates slightly less rapidly than the surface, while the innermost part apparently rotates more rapidly. The resulting solar gravitational quadrupole moment is J2 = (1.7±0.4)×10-7 and provides a negligible contribution to current planetary tests of Einstein's theory of general relativity.
Duvall Thomas L. Jr.
Dziembowski Wojciech A.
Goode Philip. R.
Gough Douglas O.
Harvey Jack W.
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