Science at very low radio frequencies.

Details Science at very low radio frequencies. Science at very low radio frequencies.

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989lfsv.conf...29d&link_type=abstract

Workshop on a Lunar Far-Side Very Low Frequency Array, p. 29 - 33

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Scientific paper

The broad scientific goals of a lunar based Very Low Frequency Array are presented. The frequency range of 1 - 30 MHz is defined to be the operative VLF window. The low frequency end of this window is useful for studies of the interstellar medium since the large scale distributions of thermal and relativistic gas are traceable at these frequencies. Studies of discrete objects, both galactic and ectragalactic, are possible at the higher frequency end of the window. The VLF window is ideally suited for studies of phenomena not manifested in any other spectral band.

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