1949
DOI: 10.1071/ch9490063
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Microwave Thermal Radiation from the Moon

Abstract: Measurements have been made of the thermal radiation from the moon in a 15 Mc/s. band, centred a t 24,000 Mc/s. The radiation from the whole lunar disk has been measured during several phase cycles. Temperatures corresponding to this radiation have been deduced and curves of temperature against phase angle drawn. One of these corresponds to average temperature over the disk and the other to the temperature of a point on the lunar equator. They are found to be approximately sinusoidal, with amplitude k 4 0 . 3 … Show more

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Cited by 54 publications
(31 citation statements)
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“…In 1961 Carl Sagan argued that at a depth of less than 50cm some locations on the Moon could have stable temperatures between 0 and 70 ℃, citing microwave radiation data (Piddington and Minnett, 1949) [3] that was consistent with this result. (https://science.nasa.gov/science-news/science-at-nasa/ 2010/12jul_rabbithole/)…”
supporting
confidence: 55%
“…In 1961 Carl Sagan argued that at a depth of less than 50cm some locations on the Moon could have stable temperatures between 0 and 70 ℃, citing microwave radiation data (Piddington and Minnett, 1949) [3] that was consistent with this result. (https://science.nasa.gov/science-news/science-at-nasa/ 2010/12jul_rabbithole/)…”
supporting
confidence: 55%
“…Even though the Moon's mean disk temperature observed in 1948 by Piddington and Minnett [31] is about 26 K higher than that of Monstein [30], it is still 31 K lower than 270 K e T ≅ . Despite the Moon is nearly a perfect example of a planet without atmosphere, some authors argued that Equations (1.3) and (1.4) are only valid for fast-rotating planets so that the Moon must be excluded.…”
Section: 30mentioning
confidence: 84%
“…1500 oK. This disk temperature is made less negative by two terms: firstly, that due to the reflection of galactic radiation by the Moon; and, secondly, the temperature of the lunar surface, which, according to the 1·25 cm observations of Piddington and Minnett (1949), is 270 oK at the Moon's last quarter. Tbis lunar radiation is thermal, and so the effective brightness temperature at 3·5 m is likely to be similar.…”
Section: (C) the Effect On The Occultation Of The Apparent Brightnessmentioning
confidence: 99%