Very low frequency array on the lunar far side. Report by the Very Low Frequency Astronomy Study Team.

Details Very low frequency array on the lunar far side. Report by the Very Low Frequency Astronomy Study Team. Very low frequency array on the lunar far side. Report by the Very Low Frequency Astronomy Study Team.

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997vlfa.book......&link_type=abstract

Very low frequency array on the lunar far side. Report by the Very Low Frequency Astronomy Study Team., by . European Space Age

Astronomy and Astrophysics

Astronomy

Scientific paper

The far side of the Moon offers unique advantages for performing radio astronomy at very low frequencies. The instrument that is proposed is an array of 300 independent receiving elements arranged in a spiralled-'Y' within an enclosing circle 40 km in diameter. This array is designed to perform all-sky surveys within the frequency range of 0.5 to 16 MHz with an angular resolution of at least 0.5 degrees. The mission can be completed within 5 years.

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