Westphal, J. A. and Wildey, R. L. and Murray, B. C. (1965) The 8-14-μ Appearance of Venus Before the 1964 Conjunction. Astrophysical Journal, 142 . pp. 799-801. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20151120-090218795
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Abstract
In an earlier paper (Murray, Wildey, and Westphal 1963) we have described the detailed mapping of the 8-14-μ radiation from Venus using the 200-inch Hale telescope. This paper extends that work over a period of about 7 months from December 15, 1963, to June 6, 1964. Detailed maps for 6 days are presented that show the morphology of the upper-atmosphere brightness temperature and illustrate a number of anomalous features near the cusps. The problem of atmospheric extinction and the derived brightness temperature is discussed.
| Item Type: | Article | |||||||||
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| Additional Information: | © 1965 American Astronomical Society. Provided by the NASA Astrophysics Data System. | |||||||||
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| Record Number: | CaltechAUTHORS:20151120-090218795 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20151120-090218795 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 62275 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Tony Diaz | |||||||||
| Deposited On: | 20 Nov 2015 17:17 | |||||||||
| Last Modified: | 03 Oct 2019 09:17 |
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