problem: ground clutter clutter: there is always clutter in signals and it distorts the purposeful...
Post on 21-Dec-2015
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Problem: Ground Clutter
Clutter: There is always clutter in signals and it distorts the purposeful component of the signal. Getting rid of clutter, or compensating for the loss caused by clutter might be possible by
applying appropriate filtering and enhancing techniques. Ground Clutter: Ground clutter is the return from the ground. The returns from ground scatters are usually very large with respect to other echoes, and so can be easily recognized Ground-based obstacles may be immediately in the line of site of the main radar beam, for instance hills, tall buildings, or towers.
Solution: IIR/Pulse-Pair approach
Uses a fixed notch-width IIR clutter filter followed by time-domain autocorrelation processing (pulse-pair processing)
Drawbacks to using this approach:Perturbations that are encountered will effect the filter output for many pulses, effecting the output for several beamwidths
The filter width has to change accordingly with clutter strength
Have to manually select a filter that is sufficiently wide to remove the clutter without being to wide so it doesn’t affect wanted data
Solution: FFT processing
FFT: is essentially a finite impulse response block processing approach that does not have the transient behavior problems of the IIR filter. It minimizes the effects of filter bias. Drawbacks to this approach:
Spectrum resolution is limited by the number of points in the FFT. If the number points is to low it will obscure weather targetsWhen time-domain windows are applied such as Hamming or Blackman the number of samples that are processed are reduced
Solution: GMAP
GMAP: GMAP is a frequency domain approach that uses a Gaussian clutter model to remove ground clutter over a variable number of spectral components that is dependent on the assumed clutter width, signal power, nyquist interval and number of samples. Then a Gaussian weather model is used to iteratively interpolate over the components that were removed, restoring any of the overlapped weather spectrum with minimal bias
Solution: GMAP
GMAP assumptions: Spectrum width of the weather signal is greater then clutter.
Doppler spectrum consists of ground clutter, a single weather target and noise.
The width of the clutter is approximately known.
The shape of the clutter is a Gaussian.
The shape of the weather is a Gaussian
GMAP Algorithm Description
First a Hamming window weighting function is applied to the In phase and quadrature phase (IQ) values and a discrete Fourier transform (DFT) is then performed.
The Hamming window is used as the first guess after analysis is complete a decision is made to either accept results or use a more aggressive window based on the clutter to signal ratio (CSR).
GMAP Algorithm Description
Remove Clutter points The power in the three central spectrum components is summed and compared to the power that would be in the three central components of a normalized Gaussian spectrum. Normalizes the power of the Gaussian to the observed power the Gaussian is extended down to the noise level and all spectral components that fall within the gaussian curve are removed. The removed components are the “clutter power”
GMAP Algorithm Description
Replace Clutter pointsDynamic noise case
Fit a Gaussian and fill-in the clutter points that were removed earlier keep doing this until the computed power does not change more then .2dB and the velocity does not change by more than .5% of the Nyquist velocity.
Fixed noise caseSimilar to dynamic noise case except the spectrum points that are larger than the noise level are used
GMAP Algorithm Description
Recompute GMAP with optimal windowDetermin if the optimal window was used based on the CSR
IF CSR > 40 dB repeat GMAP using a Blackman window and dynamic noise calculation.IF CSR > 20 dB repeat GMAP using a Blackman window. Then if CSR>25dB use Blackman results.IF CSR < 2.5 dB repeat GMAP using a rectangular window. Then if CSR < 1 dB use rectangular results.ELSE accept the Hamming window result.
Gmap With Data From CASA
Power from PRF1
Gmap With Data From CASA
Power with gmap from PRF1
Gmap With Data From CASA
Velocity from Prf1
Gmap With Data From CASA
Velocity of Prf1
Gmap With Data From CASA
Velocity from PRF1with GMAP
Gmap With Data From CASA
Power from Prf1 using Hamming
Gmap With Data From CASA
Power from Prf1 using Hamming [0 60] dbs
Gmap With Data From CASA
Power from Prf1 using Hamming [-20 20] dbs