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The 8-14-μ Appearance of Venus Before the 1964 Conjunction

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
Related URLs:
URLURL TypeDescription
http://adsabs.harvard.edu/abs/1965ApJ...142..799WADSArticle
http://dx.doi.org/10.1086/148347DOIArticle
Additional Information:© 1965 American Astronomical Society. Provided by the NASA Astrophysics Data System.
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Caltech Division of Geological Sciences1318
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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