Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989lfsv.conf...13e&link_type=abstract
Workshop on a Lunar Far-Side Very Low Frequency Array, p. 13 - 17
Astronomy and Astrophysics
Astronomy
Radio Telescopes: Telescope Arrays, Radio Telescopes: Data Processing
Scientific paper
Most radio astronomical observations below 100 MHz have been the result of considerable effort on the part of a relatively small number of astronomers and engineers. The size required for the instruments has precluded the construction of more than a few in the world and, until recently, technology has not allowed the design of a large decametric array which would operate over more than a limited frequency range and be steerable in two coordinates with reasonable speed. Advances in the technology of decade bandwidth antennas and low cost, reliable, wideband, solid state devices have made large fully-steerable decametric systems practical. Around these developments, the design of the Clark Lake telescope evolved during the 1970s. It was operable anywhere between 10 and 125 MHz with nearly instantaneous frequency and beam positioning capability.
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