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The Use of Meteor Radars in the Detection of Infalling Space Debris

Published online by Cambridge University Press:  12 April 2016

D.I. Olsson-Steel  and
W.G. Elford
D.I. Olsson-Steel
Affiliation:
Department of Physics and Mathematical Physics, University of Adelaide, G.P.O.Box 498, Adelaide, SA 5001, Australia
W.G. Elford
Affiliation:
Spaceguard Orbital Debris Analysts, 51 Warwick Street, Enfield, SA 5085, Australia

Abstract

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Radars of various configurations are used to detect the flux of meteors into the atmosphere, and therefore may be of use in characterizing the artificial meteors produced by small (100 microns - 1 cm) pieces of space debris upon re-entry. Both conventional and over-the-horizon radars are discussed here, and the ways in which they may be deployed in order to detect infalling space debris are outlined.

Type
Space Debris
Information
International Astronomical Union Colloquium , Volume 112: Light Pollution, Radio Interference, and Space Debris , 1991 , pp. 166 - 171
Copyright
Copyright © Astronomical Society of the Pacific 1991

References

Elford, W.G., 1964. “Calculation of the Response Function of the Harvard Radio Meteor Project Radar System”, Harvard Radio Meteor Project Research Report Number 8, Cambridge, Mass.Google Scholar
Elford, W.G. and Olsson-Steel, D., 1987a. “The height distribution of radar meteors: Observations at 6 MHz”, J. Atmos. Terr. Phys. (in press).CrossRefGoogle Scholar
Hughes, D.W., 1978. “Meteors”, pp.123–185 in “Cosmic Dust” (ed. McDonnell, J. AM.), Wiley, Chichester.Google Scholar
Kessler, D.J., 1985. “Orbital Debris Issues”, Adv. Space Res., 5,3–10.CrossRefGoogle Scholar
Laurance, M.R. and Brownlee, D.E., 1986. “The flux of meteoroids and orbital space debris striking satellites in low Earth orbit”, Nature, 323,136–138.Google Scholar
McKinley, D.W.R., 1961. “Meteor Science and Engineering”, McGraw-Hill, New York.Google Scholar
Olsson-Steel, D. and Elford, W.G., 1987a. “The height distribution of radar meteors: Observations at 2 MHz”, J. Atmos. Terr. Phys., 49,243–258.CrossRefGoogle Scholar
Olsson-Steel, D. and Elford, W.G., 1987b. “The true height distribution and flux of radar meteors”, Publ. Astron. Inst. Czechoslov. Acad. Sci., No.67, Vol.2, 193–197.Google Scholar
Olsson-Steel, D., 1988. “The origin and physical characteristics of meteoroids”, Highlights of Astronomy (in press).CrossRefGoogle Scholar
Thomas, R.M., Whitham, P.S. and Elford, W.G., 1986. “Frequency dependence of radio meteor echo rates”, Proc. Astron. Soc. Australia, 6,303–306.CrossRefGoogle Scholar
Thomas, R.M., Whitham, P.S. and Elford, W.G., 1988. “Response of High Frequency radar to meteor backscatter”, J. Atmos. Terr. Phys. (in press).CrossRefGoogle Scholar
Wang, S.T., Tetenbaum, D., Balsley, B.B. Obert, R.L., Avery, S.K. and Avery, J.P., 1988. “A meteor echo detection and collection system for use on VHF radars”, Radio Sci., 23,46–54.CrossRefGoogle Scholar