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., Pizzo, G., Dalloglio, G. (2011). The brightness temperature of Mercury at 150 and 240 GHz. THE EUROPEAN PHYSICAL JOURNAL PLUS, 126, 99-101 [10.1140/epjp/i2011-11099-3].
The brightness temperature of Mercury at 150 and 240 GHz
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:
Non ci sono file associati a questo prodotto.
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
