Solar Spin-down Problem

Details Solar Spin-down Problem Solar Spin-down Problem

Jun 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967natur.214.1297h&link_type=abstract

Nature, Volume 214, Issue 5095, pp. 1297-1299 (1967).

Physics

48

Scientific paper

It has been suggested that if the solar Interior rotates rapidly, the resultant oblateness may noticeably affect the precession of the perihelion of Mercury. It is now argued that such effects would be reduced by the action of the boundary layer between the convective envelope and the interior of the Sun. The boundary layer suction causes a slow internal motion which stretches vortex lines and spins down the solar interior.

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