Rather, J. D. G., Ulich, B. L. and Ade, Peter A. R. 1974. Planetary brightness temperature measurements at 1.4-mm wavelength. Icarus 22 (4) , pp. 448-453. 10.1016/0019-1035(74)90077-3 |
Official URL: http://dx.doi.org/10.1016/0019-1035(74)90077-3
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 |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Publisher: | Elsevier Science |
ISSN: | 0019-1035 |
Last Modified: | 04 Jun 2017 06:38 |
URI: | http://orca.cf.ac.uk/id/eprint/63181 |
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