• DocumentCode
    1005994
  • Title

    Comparison of low angle radar clutter models

  • Author

    Shnidman, D.A.

  • Author_Institution
    RADET Consulting, Lexington, MA, USA
  • Volume
    41
  • Issue
    2
  • fYear
    2005
  • fDate
    4/1/2005 12:00:00 AM
  • Firstpage
    736
  • Lastpage
    746
  • Abstract
    Three low angle clutter models, the compound-K, the noncentral gamma-gamma (NCGG), both of which model speckle, and the Weibull distributions are compared. The derivations of the first two densities are surprisingly similar, differing on only one critical point. The compound-K assumes that the Gaussian random variables that are the input to the square law detector have zero means, while the NCGG assumes that the Gaussian random variables have nonzero means. The compound-K must then assume that it is the output variance that is fluctuating to produce speckle, while the NCGG assumes that it is the noncentrality parameter, resulting from the addition of the nonzero means that is fluctuating. The difference in the resulting models is significant. The Weibull density has long been used to model clutter successfully, and it too will be considered for comparison, but its use is not based upon a physically motivated development. Rather, its use is based on comparisons of clutter output densities being well matched by the Weibull density with appropriate parameters.
  • Keywords
    Gaussian distribution; Weibull distribution; radar clutter; Gaussian random variables; Weibull density; Weibull distributions; compound-K; low angle radar clutter models; noncentral gamma-gamma; noncentrality parameter; nonzero means; square law detector; zero means; Decorrelation; Frequency; Power generation; Radar antennas; Radar clutter; Radar cross section; Spatial resolution; Speckle; Transmitters; Weibull distribution;
  • fLanguage
    English
  • Journal_Title
    Aerospace and Electronic Systems, IEEE Transactions on
  • Publisher
    ieee
  • ISSN
    0018-9251
  • Type

    jour

  • DOI
    10.1109/TAES.2005.1468764
  • Filename
    1468764