Disk brightness temperature of the planets at 43 GHz (and 43 GHz flux densities of some continuum sources)

Details Disk brightness temperature of the planets at 43 GHz (and 43 GHz flux densities of some continuum sources) Disk brightness temperature of the planets at 43 GHz (and 43 GHz flux densities of some continuum sources)

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...286..654g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 286, no. 2, p. 654-658

Astronomy and Astrophysics

Astronomy

10

Brightness Temperature, Flux Density, Jupiter (Planet), Mars (Planet), Neptune (Planet), Radio Astronomy, Saturn (Planet), Uranus (Planet), Venus (Planet), Extremely High Frequencies, H Ii Regions, Millimeter Waves, Planetary Nebulae, Very Long Base Interferometry

Scientific paper

We have used the MPIfR 43 GHz (7 mm) Schottky receiver, installed in 1991 on the Institut de Radio Astronomie Millimetrique (IRAM) 30-m telescope for VLBI observations, for flux density measurements of several planets in comparison with several Galactic and extra-galactic continuum sources, using as calibration standards the sources W3OH and NGC 7027. The disk brightness temperatures of the planets are derived from these flux densities.

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