Comparison of Measured and Computed Values of the Rapid Fading-Rate of Ultra High-Frequency Signals reflected from the Moon

Details Comparison of Measured and Computed Values of the Rapid Fading-Rate of Ultra High-Frequency Signals reflected from the Moon Comparison of Measured and Computed Values of the Rapid Fading-Rate of Ultra High-Frequency Signals reflected from the Moon

Nov 1958

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1958natur.182.1438f&link_type=abstract

Nature, Volume 182, Issue 4647, pp. 1438-1439 (1958).

Physics

Scientific paper

DURING August 1957, a bistatic moon reflexion experiment was carried out between South Dartmouth, Massachusetts (41.5395° N., 76.9512° W.), and Alpha, Maryland (39.3224° N., 76.9258° W.). The continuous-wave transmitter fed approximately 40 kW. of power, at a frequency of 412.85 Mc./s., into a horizontally polarized feed mounted in a 60-ft. diameter parabolic antenna. The antenna was movable in azimuth and elevation. The receiving system at Alpha used a dual-polarization feed in a 28-ft. diameter parabolic antenna, which was free to move in azimuth and elevation.

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