Voyager radio astronomy and the low frequency near-Earth radio environment.

Details Voyager radio astronomy and the low frequency near-Earth radio environment. Voyager radio astronomy and the low frequency near-Earth radio environment.

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989lfsv.conf...35d&link_type=abstract

Workshop on a Lunar Far-Side Very Low Frequency Array, p. 35 - 41

Astronomy and Astrophysics

Astronomy

Scientific paper

The author reviews the major features of the radio astronomy experiment onboard the two Voyager spacecraft. In addition, the major sources of noise in the near-Earth environment are identified. They are: (1) terrestrial atmospherics, (2) terrestrial kilometric radiation, and (3) solar Type III bursts. Interference from all but the last is eliminated by observing from the lunar far-side. Based on experience with numerous classes of spaced-based radio astronomy experiments, the use of relatively simple antennas with a sophisticated observing scheme seems not only expedient but most likely to operate effectively on the Moon.

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