During the Italian Antarctic Expedition 2004/2005 we observed Mercury at 150 and 240 GHz. The observations have been carried out by means of the 2.6m OASI telescope. By using the responsivity of our detectors, obtained from Venus, the brightness temperature of the planet was derived.
Sabbatini, L., Dall'Oglio, G., Pizzo, G. (2011). The brightness temperature of Mercury at 150 and 240 GHz. THE EUROPEAN PHYSICAL JOURNAL. C, PARTICLES AND FIELDS, 126 [10.1140/epjp/i2011-11099-3].
The brightness temperature of Mercury at 150 and 240 GHz
DALL'OGLIO, Giorgio;PIZZO, Gabriella
2011-01-01
Abstract
During the Italian Antarctic Expedition 2004/2005 we observed Mercury at 150 and 240 GHz. The observations have been carried out by means of the 2.6m OASI telescope. By using the responsivity of our detectors, obtained from Venus, the brightness temperature of the planet was derived.File in questo prodotto:
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