Published April 14, 1967
| public
Journal Article
Rapid Rotation of the Solar Interior
- Creators
- Deutsch, Armin J.
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.
Additional Information
© 1967 American Association for the Advancement of Science. 14 February 1967. I thank J. Faulkner, P. Goldreich, R. P. Kraft, I. W. Roxburgh, W. L. W. Sargent, and P. A. Strittmatter for assistance and discussions.Additional details
- Eprint ID
- 62863
- DOI
- 10.1126/science.156.3772.236
- Resolver ID
- CaltechAUTHORS:20151214-104451064
- Created
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2015-12-14Created from EPrint's datestamp field
- Updated
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2023-10-25Created from EPrint's last_modified field