Lunar far-side very low frequency array.

Details Lunar far-side very low frequency array. Lunar far-side very low frequency array.

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989lfsv.conf...53b&link_type=abstract

Workshop on a Lunar Far-Side Very Low Frequency Array, p. 53 - 60

Physics

Radio Telescopes: Moon Surface

Scientific paper

The authors suggest an initial general design for a low-frequency array for the lunar surface. Deployment would occur over several phases. In the first phase, incremental dipoles would be placed in a semiregular pattern over a region 17 km in diameter. This would provide a resolution of 1° at the lowest operating frequency of 1 MHz. Operating frequencies for the array would range from 1 to 30 MHz. The array would operate in an interferometric mode rather than as a phased array.

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