Planetary brightness temperature measurements at 1.4-mm wavelength

Rather, J. D. G., Ulich, B. L. and Ade, Peter A. R. ORCID: https://orcid.org/0000-0002-5127-0401 1974. Planetary brightness temperature measurements at 1.4-mm wavelength. Icarus 22 (4) , pp. 448-453. 10.1016/0019-1035(74)90077-3

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Abstract

Precise relative measurements of the disk brightness temperatures of Venus, Mars, Jupiter, and Saturn have been made at a mean wavelength of 1.4 mm. The rings of Saturn contribute significantly to the observed total emission. Other results include a better understanding of the properties of the NRAO 11-m antenna near its high frequency limit and of atmospheric degradation of observations in this wavelength range.

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Schools > Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Publisher:	Elsevier Science
ISSN:	0019-1035
Last Modified:	27 Oct 2022 08:43
URI:	https://orca.cardiff.ac.uk/id/eprint/63181

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