Nonlinear Predictor and Interpolator
For narrowband interference added to a spread-spectrum signal
in an AWGN environment, the prediction of the interferer takes place in the
presence of both Gaussian and non-Gaussian noise. The non-Gaussian noise is the
spread-spectrum signal itself. In such a non-Gaussian environment, linear
methods are no longer optimal, and nonlinear techniques offer improved
suppression capability over linear methods, as demonstrated in Section 7.3. Essentially,
the nonlinear filters provide decision feedback that suppresses the
spread-spectrum signal from the observations. When the decision feedback is
accurate, the filter adaptation is done in essentially Gaussian noise (i.e.,
observations from which the spread-spectrum signal has been removed).
Based on the discussion above, we can obtain similar SINR upper
bounds for the nonlinear predictive/interpolative methods. The idea is that we
assume that the decision feedback part of the nonlinear filter accurately
estimates the SS signal, and the SS signal is always subtracted from the
observations, so that the NBI signal is estimated only in the presence of
Gaussian noise. More specifically, consider the signal model (7.5). Assume that for the
purpose of estimating the NBI signal, a genie provides an SS-signal-free
observation
A linear predictor or interpolator is then employed to obtain
and estimate în of the NBI signal,
which is then subtracted from the received signal to form the decision statistic
for the SS data bit b,
Equation 7.124
where
n is the prediction error of the linear predictor
(interpolator) (i.e.,
n = in
- în + un). Modeling {cn,1} as a sequence of i.i.d. random
variables such that
with probability ½, the output SINR
of this ideal system is then
Equation 7.125
Substituting the lower bounds for the mean-square prediction
errors
given by the linear predictor and linear interpolator [310, 311], we obtain the following very
optimistic SINR upper bounds for the nonlinear estimator-subtracter methods:
Equation 7.126
Equation 7.127
Now assume that the NBI is a pth-order AR signal, given by (7.94). Its power spectral
density function is given by
Equation 7.128
Substituting (7.128)
into (7.127) and letting s
0, we get the SINR upper bound for the nonlinear interpolator when the
NBI is an AR signal in the absence of background noise:
Equation 7.129
Notice that this is the same output SINR value for the linear
MMSE detector when the NBI is an AR signal in the absence of noise, given by (7.106).