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output of a linear detector. The threshold will be set according to







                                                                                                     (6.142)

               A formula can be found relating            and   that must be solved iteratively and is
               numerically  difficult  (Raghavan,  1992).  The  exact  results  show  excellent

               agreement with the approximation (Di Vito and Moretti, 1989)





                                                                                                     (6.143)

               where c  =  4/π.  Notice  the  similarity  to Eq.  (6.135).  The  square  root  is  a
               consequence of using a linear rather than square-law detector. For N > 4 the (c –
               1)  exp(1  – N)  term  is  negligible  and  since c  ≈  1.27,                 .  Furthermore,
               although the square law detector CA CFAR performs marginally better than the
               linear  detector  for  some  parameter  choices,  its  performance  is  virtually

               identical for parameter values of practical interest.
                     In the example of Fig. 6.20 it was noted that for the parameters given the
               ideal  threshold  would  be  8.4  dB  above  the  mean  power  if  the  interference
               power were known exactly, but if the power had to be estimated from the data
               with N = 20 the threshold would be 9.2 dB above the estimated power level.
               This higher threshold compared to the interference power level is necessary to
               compensate  for  the  imperfectly  known  interference  power  and  guarantee  the
               desired  . Because the threshold multiplier is increased in CFAR, the average

               probability of detection for a target of a given SNR will be decreased relative
               to the known-interference case. Alternately, to achieve a specified   for a given
                  , a higher SNR will be required than would be were the interference power
               known exactly. This increase in SNR required to achieve specified detection
               statistics when using CFAR techniques is called the CFAR loss.

                     To  quantify  the  CFAR  loss  in  the  case  of  a  CA  CFAR,  combine  Eqs.
               (6.134) and (6.137) to eliminate the multiplier α and solve for the value of SNR
               required  to  achieve  a  specified  combination  of    and  .  The  result  is  a
               function of the number of samples averaged and is denoted by  :







                                                                                                     (6.144)

               As N → ∞, the estimate of interference power converges to the true value and
               so    and    will  converge  to  the  values  given  by Eqs. (6.139)  and (6.140).
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