Stevenson, D. J. (1980) Saturn's Luminosity and Magnetism. Science, 208 (4445). pp. 746-748. ISSN 0036-8075. doi:10.1126/science.208.4445.746. https://resolver.caltech.edu/CaltechAUTHORS:20131114-143222111
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Abstract
The Pioneer 11 results for Saturn's large heat output, small magnetic field, and near-axisymmetry of the field may all be explained by an interior model in which the helium is undergoing phase separation and is nonuniformly distributed. Substantial depletion of helium from the atmosphere is predicted.
| Item Type: | Article | ||||||||||||
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| Additional Information: | © 1980 American Association for the Advancement of Science. Published May 16, 1980. | ||||||||||||
| Issue or Number: | 4445 | ||||||||||||
| DOI: | 10.1126/science.208.4445.746 | ||||||||||||
| Record Number: | CaltechAUTHORS:20131114-143222111 | ||||||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20131114-143222111 | ||||||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||||||||
| ID Code: | 42467 | ||||||||||||
| Collection: | CaltechAUTHORS | ||||||||||||
| Deposited By: | INVALID USER | ||||||||||||
| Deposited On: | 14 Nov 2013 23:31 | ||||||||||||
| Last Modified: | 10 Nov 2021 16:23 |
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