Rapid Rotation of the Solar Interior

Details Rapid Rotation of the Solar Interior Rapid Rotation of the Solar Interior

Apr 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967sci...156..236d&link_type=abstract

Science, Volume 156, Issue 3772, pp. 236-237

Physics

8

Scientific paper

A model proposed for the sun apparently can account for the maintenance
of photospheric rotation against deceleration by the solar wind. The
rotational period is about half a day near the top of the radiative
mass, and 1.6 times shorter at the center.

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