CaltechAUTHORS
  A Caltech Library Service

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. http://resolver.caltech.edu/CaltechAUTHORS:20151214-104451064

Full text is not posted in this repository. Consult Related URLs below.

Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20151214-104451064

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.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.do.org/10.1126/science.156.3772.236 DOIArticel
http://www.sciencemag.org/content/156/3772/236.abstractPublisherArticle
http://www.jstor.org/stable/1720509JSTORArticle
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.
Record Number:CaltechAUTHORS:20151214-104451064
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20151214-104451064
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
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:14 Dec 2015 18:55
Last Modified:14 Dec 2015 18:55

Repository Staff Only: item control page