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Space/time/frequency methods in adaptive radar - New Jersey ...

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66estimate the covariance matrix. Noise exists at all frequencies and hence, an <strong>in</strong>f<strong>in</strong>itenumber of degrees of freedom is needed to fully estimate the noise subspace. As thesample support size K <strong>in</strong>creases, R approaches the true covariance matrix R andthe noise eigenvalues <strong>in</strong> A all converge towards the noise power a -2 .3.2 Beamform<strong>in</strong>g TechniquesA brief review of previous and related work <strong>in</strong> the field of <strong>adaptive</strong> process<strong>in</strong>g of<strong>radar</strong> will now be presented.3.2.1 Non-Adaptive BeamformerThe non-<strong>adaptive</strong> beamformer uses the weight vectorwhere s is the presumed steer<strong>in</strong>g vector for the target. For a given angle and velocity,s has the form of Equation 3.6 or Equation 3.7. Amplitude taper<strong>in</strong>g w<strong>in</strong>dow<strong>in</strong>gfunctions maybe used on the steer<strong>in</strong>g vector to lower the sidelobes. When this is done,the width of the ma<strong>in</strong>lobe is <strong>in</strong>creased. The non-<strong>adaptive</strong> beamformer maximizesthe beamformer's output signal-to-noise ratio <strong>in</strong> the absence of <strong>in</strong>terferences.3.2.2 Optimum Signal Process<strong>in</strong>gBrennan and Reed[46] with Mallet [151147], developed the theory for optimum<strong>adaptive</strong> arrays which maximizes the probability of detection. It was shown that theoptimal detector for a signal <strong>in</strong> Gaussian noise is achieved by us<strong>in</strong>g a Wiener filterwhen the covariance matrix of the signal is known a priori. The weights of this filterare given by

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