The solar spectrum at 8 MM

Details The solar spectrum at 8 MM The solar spectrum at 8 MM

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.253..513s&link_type=abstract

Nature, vol. 253, Feb. 13, 1975, p. 513, 514.

Astronomy and Astrophysics

Astronomy

2

Brightness Temperature, Millimeter Waves, Solar Spectra, Solar Temperature, Astronomical Models, Lunar Temperature, Solar Radio Emission

Scientific paper

Measurements have been conducted of the slope of the brightness-frequency curve near 36 GHz. The observational method used was similar to that of Reber's (1971) in which the new moon is used as a calibration source. The calculated slope is presented in a table along with the slope from the van de Hulst model (1953) and the slope from the Zheleznyakov model (1965). It is suggested that the future measurements of the solar brightness temperature at millimeter wavelengths should include a measurement of the new moon.

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