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Radar observations of the moon at 10-cm wavelength

Published online by Cambridge University Press:  14 August 2015

J. S. Hey  and
V. A. Hughes
J. S. Hey
Affiliation:
Royal Radar Establishment, Malvern, England
V. A. Hughes
Affiliation:
Royal Radar Establishment, Malvern, England

Extract

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This note describes some of the initial results derived from observations of radar echoes from the moon obtained at 10-cm wavelength at the Royal Radar Establishment, Malvern. The radar, which has been described elsewhere [1], has a transmitter of 2 megawatts peak power with a pulse length of 5 microseconds and a pulse recurrence frequency of 260 per second. The receiver is of conventional design and has a bandwidth of 500 kc/s and a noise factor of 7.5. The aerial used is the 45-foot diameter radio telescope shown in Fig. 1. The telescope is controlled from a mechanical computer that converts the lunar coordinates into azimuth and elevation, which are then fed into a servo drive.

Type
Part I: Moon and Planets
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 13 - 18
Copyright
Copyright © Stanford University Press 1959 

References

1. Staff of the Royal Radar Establishment. Nature , 180, 1225, 1957.Google Scholar
2. Yaplee, B. S., Bruton, R. H., Craig, K. J., and Roman, N. G. Proc. I.R.E. 46, 293, 1958.Google Scholar
3. Hewish, A. Proc. Roy. Soc. 209, 81, 1951; 214, 494, 1952.Google Scholar