The X-band low noise antenna measurement cone

Details The X-band low noise antenna measurement cone The X-band low noise antenna measurement cone

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975dsn..nasa..105r&link_type=abstract

In its The Deep Space Network p 105-112 (SEE N76-15190 06-12)

Astronomy and Astrophysics

Astronomy

Antennas, Cones, Electromagnetic Noise, Superhigh Frequencies, Amplification, Calibrating, Radio Sources (Astronomy)

Scientific paper

An X-band low-noise receiving cone with 17-MHz instantaneous bandwidth was built to evaluate the 26-m antenna at the Venus Station (DSS 13), Goldstone, California, at X-band frequencies, and also to provide a means for precise radio source calibrations in this frequency range. These measurments are necessary to provide more accurate antenna gain performance calibrations for the 64-m antenna subnet. The zenith system temperatures with the cone on the ground and on the antenna are 17.5 and 20.8 K, respectively.

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