Planetary radio emission in the H2O line at 1.35 CM

Details Planetary radio emission in the H2O line at 1.35 CM Planetary radio emission in the H2O line at 1.35 CM

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977avest..11...25e&link_type=abstract

Astronomicheskii Vestnik, vol. 11, Jan.-Mar. 1977, p. 25-29. In Russian.

Astronomy and Astrophysics

Astronomy

2

Brightness Temperature, Centimeter Waves, Planetary Atmospheres, Radio Emission, Water Masers, Antenna Radiation Patterns, Optical Thickness, Radio Telescopes, Solar System

Scientific paper

Results are presented for measurements of the brightness temperatures of several planets. The observations were carried out with the RT-22 radiotelescope and a maser centered at 1.35 cm. The brightness temperatures are 457 plus or minus 26 K for Venus, 207 plus or minus 20 K for Mars, 406 plus or minus 28 K for Mercury, 138 plus or minus 8 K for Saturn, and 147 plus or minus 13 K for Uranus. The brightness temperature of Jupiter was assumed to be 140 plus or minus 6 K. The concentration of H2O in the atmosphere of Venus below the cloud layer is estimated.

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