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The rapid fading of moon echoes at 100 Mc/s

Published online by Cambridge University Press:  14 August 2015

J. V. Evans ,
S. Evans  and
J. H. Thomson
J. V. Evans
Affiliation:
Jodrell Bank Experimental Station University of Manchester, England
S. Evans
Affiliation:
Jodrell Bank Experimental Station University of Manchester, England
J. H. Thomson
Affiliation:
Jodrell Bank Experimental Station University of Manchester, England

Extract

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In recent years the way in which the moon reflects radio waves has been the subject of much study. Observations by Yaplee [1] at 2860 Mc/s, Trexler [2] at 198 Mc/s, Evans [3] at 120 Mc/s, and others show that radio waves are reflected principally by a small region at the center of the moon's visible disk which has a radius of the order of one-third of the lunar radius.

Type
Part I: Moon and Planets
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 8 - 12
Copyright
Copyright © Stanford University Press 1959 

References

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