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Lunar Radar Cross Section at Low FrequencyRecent bistatic measurements of the lunar radar cross-section have extended the spectrum to long radio wavelength. We have utilized the HF Active Auroral Research Program (HAARP) radar facility near Gakona, Alaska to transmit high power pulses at 8.075 MHz to the Moon; the echo pulses were received onboard the NASA/WIND spacecraft by the WAVES HF receiver. This lunar radar experiment follows our previous use of earth-based HF radar with satellites to conduct space experiments. The spacecraft was approaching the Moon for a scheduled orbit perturbation when our experiment of 13 September 2001 was conducted. During the two-hour experiment, the radial distance of the satellite from the Moon varied from 28 to 24 Rm, where Rm is in lunar radii.
Document ID
20020074705
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Rodriguez, P.
(Naval Research Lab. Washington, DC United States)
Kennedy, E. J.
(Naval Research Lab. Washington, DC United States)
Kossey, P.
(Air Force Research Lab. Hanscom AFB, MA United States)
McCarrick, M.
(Advanced Power Technologies, Inc. Washington, DC United States)
Kaiser, M. L.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Bougeret, J.-L.
(Observatoire de Paris-Meudon France)
Tokarev, Y. V.
(Radiophysical Research Inst. Nizhny Novgorod Russia)
Date Acquired
August 20, 2013
Publication Date
January 1, 2002
Publication Information
Publication: The Moon Beyond 2002: Next Steps in Lunar Science and Exploration
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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