The nature of radar target glint and the factors upon which it depends when using the Hubble Space Telescope as a radar target is discussed. An analysis of the glint problem using a 35 MHz or 94 MHz radar on the orbital maneuvering vehicle is explored. A strategy for overcoming glint is suggested.
Consideration of radar target glint from ST during OMV rendezvous
1985-09-01
Report
No indication
English
A Statistical Glint/Radar Cross Section Target Model
IEEE | 1983
|Further Comparison Between Two Concepts of Radar Target Angular Glint
Online Contents | 2008
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