Murray, Bruce C. and Wildey, Robert L. and Westphal, James A. (1963) Venus: A Map of Its Brightness Temperature. Science, 140 (3565). pp. 391-392. ISSN 0036-8075. doi:10.1126/science.140.3565.391. https://resolver.caltech.edu/CaltechAUTHORS:20151211-083052794
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Abstract
The 200-inch Hale telescope has been used to make high-resolution maps of the brightness temperature of Venus at wavelengths 8 to 14 microns. Resolution of about 1/30 of the disk reveals a general symmetry about the plane of the orbit, no daynight temperature effects, and a transient temperature anomaly in the southern hemisphere.
Item Type: | Article | ||||||||||||
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Additional Information: | © 1963 American Association for the Advancement of Science. 10 April 1963. Supported by grant NsG 56-60 from the National Aeronautics and Space Administration and grant G-25210 from the National Science Foundation. | ||||||||||||
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Issue or Number: | 3565 | ||||||||||||
DOI: | 10.1126/science.140.3565.391 | ||||||||||||
Record Number: | CaltechAUTHORS:20151211-083052794 | ||||||||||||
Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20151211-083052794 | ||||||||||||
Official Citation: | Venus: A Map of Its Brightness Temperature Bruce C. Murray, Robert L. Wildey, and James A. Westphal Science 26 April 1963: 140 (3565), 391-392. [DOI:10.1126/science.140.3565.391] | ||||||||||||
Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||||||||
ID Code: | 62787 | ||||||||||||
Collection: | CaltechAUTHORS | ||||||||||||
Deposited By: | Ruth Sustaita | ||||||||||||
Deposited On: | 11 Dec 2015 20:28 | ||||||||||||
Last Modified: | 10 Nov 2021 23:06 |
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