Reduced-Rank STAR for high PRF radar
Document Type
Article
Publication Date
12-1-1999
Abstract
Due to the range ambiguity of high pulse-repetition frequency (HPRF) radars, echoes from far-range fold over near-range returns. This effect may cause low Doppler targets to compete with near-range strong clutter. Another consequence of the range ambiguity is that the sample support for estimating the array covariance matrix is reduced, leading to degraded performance. It is shown that space-time adaptive processing (STAP) techniques are required to reject the clutter in HPRF radar. Four STAP methods are studied in the context of the HPRF radar problem: low rank approximation sample matrix inversion (SMI), diagonally loaded SMI, eigencanceler, and element-space post-Doppler. These three methods are evaluated in typical HPRF radar scenarios and for various training conditions, including when the target is present in the training data. © 1999 IEEE.
Identifier
0033155642 (Scopus)
Publication Title
IEEE Transactions on Aerospace and Electronic Systems
External Full Text Location
https://doi.org/10.1109/7.784065
ISSN
00189251
First Page
953
Last Page
962
Issue
3
Volume
35
Grant
F30602-94-1-0012
Recommended Citation
Ayoub, T. F., "Reduced-Rank STAR for high PRF radar" (1999). Faculty Publications. 15878.
https://digitalcommons.njit.edu/fac_pubs/15878
