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Radio Frequency Interference Survey over the 1.0 - 10.4 GHz Frequency Range at the Goldstone - Venus Tracking Station

Published online by Cambridge University Press:  12 April 2016

S. Gulkis ,
E. T. Olsen ,
M. J. Klein  and
E. B. Jackson
S. Gulkis
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109
E. T. Olsen
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109
M. J. Klein
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109
E. B. Jackson
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109

Extract

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Plans are currently being made to carry out a comprehensive, all-sky search for radio signals of extraterrestrial origin. The survey will employ the Goldstone tracking station near Barstow, California, and other sites in the northern and southern hemispheres. The principal parameters of this survey are given in Table 1. In preparation for this search, we have constructed a radio spectrum surveillance system (RSSS), and made a series of measurements of the RFI environment at the Goldstone-Venus tracking station. We describe in this paper the receiving system used (Crow et al. 1985), and the results of a low-sensitivity survey performed during February 16-24,1987.

Type
Radio Frequency Interference
Information
International Astronomical Union Colloquium , Volume 112: Light Pollution, Radio Interference, and Space Debris , 1991 , pp. 228 - 239
Copyright
Copyright © Astronomical Society of the Pacific 1991

References

Crow, B., Lokshin, A., Marina, M. and Ching, L. “SETI Radio Surveillance System, JPL Publication – TDA Progress Report 42-82, April-June 1985, pp. 173–184.Google Scholar