The solar brightness temperature at mill
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Richard A. Kuseski; Paul N. Swanson
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Article
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1976
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Springer
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English
โ 283 KB
The authors have previously discussed an improved method for obtaining the absolute solar brightness temperature using the new Moon as a calibration source. New measurements of the Sun-to-new Moon ratio at three frequencies near 36 GHz ()t = 8 mm) and also at two frequencies near 93 GHz ()t = 3 mm)