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Statistical Analysis of High Resolution Land Clutter

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96 Azimuth Swaths, 500 Range Gates, 128 Frequencies, Repeated 32 times, For 7 ... 100m azimuth resolution. Glen Davidson - Radar 2002. 5. Distribution Analysis ... – PowerPoint PPT presentation

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Title: Statistical Analysis of High Resolution Land Clutter


1
Statistical Analysis of High Resolution Land
Clutter
  • G Davidson
  • Kochi University of Technology
  • H D Griffiths
  • University College London
  • S Ablett
  • Dstl

2
Overview
  • Large amount of Byson C-band (VV) frequency agile
    radar data operated in mixed clutter environment
    of Worcester.
  • Analysis suggests that no single distribution
    fits well.
  • Dominated by varying statistics including
    non-stationarity, clutter edges and
    discontinuities related to environment.
  • Due to instrumental effects and sample
    uncertainty, performance predictions were
    erroneous.
  • Show a 7dB detection gain (Pfa of 10-4) possible
    when the normalised log estimate U is used as a
    measure of uncertainty. Proposed CFAR has a
    variable threshold multiplier as an empirical
    function of U.
  • Uses real data to include all instrumental
    effects.

3
Aim
Intensity
Terrain Height
  • Analyse high resolution data and determine
    possible target detection gain from using
    non-Gaussian statistics.

4
Data Acquisition
  • Frequency Agile 30m
  • Pulse compression into range cells of 1 metre.
  • 96 Azimuth Swaths,500 Range Gates,128
    Frequencies,Repeated 32 times,For 7
    attenuations
  • Total 1?109 samples
  • 100m azimuth resolution
  • The natural local statistics to analyse were the
    100 compressed range cells within each range gate.

5
Distribution Analysis
  • Normalised log estimate U reasonable for both K
    and Weibull

Shape parameter
(Blacknell, Oliver)
6
Dynamic Range Digitisation
Gaussian U -1 U -2 U -3 U -4 U -5 U
-6 Spiky
  • Byson instrumentation has a strong effect upon U

7
Individual Gate Attenuation
  • 0dB to 50dB attenuation required over entire scene

8
U Measured for Entire Scene
  • Wide variation in U but Motorway and Railway
    visible

9
Range Cell Traces
Motorway (dB)
Open Area (linear)
  • Two cases with identical measured U obviously
    have very different statistics and may not be
    Independent Identically Distributed

10
Step Effect upon U
10dB 15dB 20dB
  • Steps in the data seriously alter the estimate of
    U, such that the clutter variance is
    over-estimated

11
Edge Corrupted or K?
Edges
Stable K
Edge Present Stable Gaussian Stable K
12
Scene Likelihood Analysis
Edge-like
log10 likelihood
K-like
  • More edge-corrupted speckle than K, except
    motorway is visibly K-like.

13
Detection Algorithm
  • Postulate Distribution

Environmental, Weibull, K, ??
  • Estimate Shape

Low sample number, edge corruption
  • N-sum Distribution

Mathematically intractable, stability over
time/range
  • Pfa Calculation

Mathematical architecture choice
  • Pd Calculation

Monte Carlo often used
  • Dynamic Range, Digitisation, Pulse Compression

14
Empirical Method
Gaussian
Spiky
  • Empirical distributions are already used
    (Weibull). A large dataset means the mathematics
    can be avoided by directly mapping the shape
    estimate to the required threshold.

15
Fixed Multiplier CFAR
Intensity
Range
  • Threshold multiplier chosen for Pfa of 10-4 over
    scene

16
Variable Multiplier CFAR
U
Intensity
Range
U
  • Threshold multiplier now a function of U for Pfa
    of 10-4

17
Real Data/Simulated Target
  • 16 Pulse CFAR
  • 4 Guard Cells
  • Pfa 10-4
  • Swerling 0 target

7dB
  • At Pd 0.5 7dB target gain

18
Conclusions
  • Land data can be so variable that the concept of
    a stable statistical distribution is not useful
    for small sample numbers.
  • Normalised log estimator U can illustrate this
    variability, but it is susceptible to edges,
    digitisation and small samples.
  • Likelihood analysis suggested that a large
    proportion is affected by edges, but CAGO didnt
    help.
  • Fixed multiplier CFAR false alarms dominated by
    motorway and other spiky areas strongly
    correlated to environment.
  • Instead of empirically fitting distributions such
    as Weibull to single pulse data, weve
    empirically fitted the required threshold for a
    variable multiplier CFAR architecture as f(U).
  • When all instrumentation effects are included,
    still see a 7dB improvement in performance.
    Normalised log U is useful as a general measure
    of uncertainty.
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