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Rapid Rotation of the Solar Interior

Deutsch, Armin J. (1967) Rapid Rotation of the Solar Interior. Science, 156 (3772). pp. 236-237. ISSN 0036-8075.

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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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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.
Issue or Number:3772
Record Number:CaltechAUTHORS:20151214-104451064
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Official Citation:Rapid Rotation of the Solar Interior Armin J. Deutsch Science 14 April 1967: 156 (3772), 236-237. [DOI:10.1126/science.156.3772.236]
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:62863
Deposited By: Ruth Sustaita
Deposited On:14 Dec 2015 18:55
Last Modified:03 Oct 2019 09:23

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