Page 390 - Fundamentals of Radar Signal Processing
P. 390

(5.99)

               The algorithm finds the set of model coefficients {a } that optimally fits Ŷ(ω) to
                                                                            p
               Y(ω) for a given model order P. These coefficients are found by solving a set of
               normal equations (Hayes, 1996) derived from the autocorrelation of the slow-

               time data y[m]; the actual spectrum Y(ω) is not needed. The {ap} are then used
               to  compute  an  estimated  spectrum  according  to Eq.  (5.99),  which  can  be
               analyzed for target detection, pulse pair processing, or other functions.
                     Modeling the spectrum as shown in Eq. (5.99) is equivalent to modeling
               the slow-time signal y[m] as the impulse response of an IIR filter with frequency
               response                       .  The  inverse  filter  is  an  FIR  filter  with  impulse
               response coefficients h[m] = a  and a  = 1. If y[m] is passed through this filter
                                                             0
                                                    m
               the  output  spectrum  will  be  approximately  constant  provided  that  the  actual
               signal spectrum is accurately modeled by Eq. (5.99). It follows that if the {a }
                                                                                                            p
                                               2
               are chosen such that |Ŷ(ω)|  is a good model of the power spectrum of random
               process data such as noise and clutter, then passing that data through the inverse
               filter  will  produce  a  new  random  process  with  an  approximately  flat  power

               spectrum. Thus, the FIR filter designed from the model coefficients whitens the
               signal, removing any correlated signal components such as clutter.
                     Figure 5.24 illustrates the application of AR spectral estimation to design a
               clutter filter to enhance detection of windshear from an airborne radar (Keel,
               1989). Part a shows the Fourier spectrum of the slow-time data from one range
               bin. Two peaks are evident above the noise floor. The one at zero velocity is
               ground clutter. The smaller peak at approximately 8 m/s is due to windblown

               rain. The middle plot shows the frequency response of an optimal clutter filter
               implemented from the {a }. The third plot shows the Fourier spectrum of the
                                              p
               slow-time data after processing with the clutter filter. The ground clutter has
               been significantly suppressed and the weather echo is now the dominant spectral
               feature.
   385   386   387   388   389   390   391   392   393   394   395