Rapid Rotation of the Solar Interior
- 14 April 1967
- journal article
- other
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 156 (3772), 236-237
- https://doi.org/10.1126/science.156.3772.236
Abstract
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.Keywords
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