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Lunar low-frequency radio arrayA simple, inexpensive experiment is proposed for the early lunar mission to make high angular resolution observations in one of the last unexplored parts of the electromagnetic spectrum. An array of nineteen simple crossed-dipole antennas will make images at frequencies below the earth's ionospheric cut-off - from about 100 kHz to 10 MHz. It would serve as a precursor to a major low-frequency telescope which would eventually be built on the back of the moon, away from terrestrial interference.
Document ID
19910071993
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Kuiper, T. B. H.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Jones, D. L.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Mahoney, M. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Preston, R. A.
(JPL Pasadena, CA, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1990
Subject Category
Astronomy
Meeting Information
Meeting: Astrophysics from the Moon
Location: Annapolis, MD
Country: United States
Start Date: February 5, 1990
End Date: February 7, 1990
Sponsors: NASA
Accession Number
91A56616
Distribution Limits
Public
Copyright
Other

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