Concept:
The Wiener filter is a classic linear filter optimized to minimize the mean square error (MSE) between a desired target signal and a noisy received signal. To mathematically solve the foundational Wiener-Hopf equations and determine fixed, optimal filter coefficients, the system must operate under strict statistical constraints.
Step 1: Core operational assumptions of the standard Wiener filter.
The derivation of the standard Wiener filter relies on two primary statistical assumptions:
• Both the useful underlying signal, $s[n]$, and the interfering corrupting noise, $v[n]$, must be wide-sense stationary (WSS) random processes. This means their statistical properties—such as mean, variance, and autocorrelation functions—remain completely constant and invariant over time.
• The noise process must be completely uncorrelated with, and statistically independent of, the target signal.
Step 2: Examining the impact of independence on the filter derivation.
Let the received noisy signal be $x[n] = s[n] + v[n]$. The design of the filter depends on the cross-correlation function between the input and the desired target signal, $R_{xs}[k]$. Because the noise is assumed to be statistically independent and has a zero mean value, the expectation simplifies cleanly:
\[
R_{xs}[k] = E[x[n]s[n-k]] = E[(s[n] + v[n])s[n-k]] = E[s[n]s[n-k]] + E[v[n]s[n-k]]
\]
Due to complete statistical independence, the joint expectation splits into separate products:
\[
E[v[n]s[n-k]] = E[v[n]] \cdot E[s[n-k]] = 0 \cdot E[s[n-k]] = 0
\]
This simplifies the cross-correlation equation to:
\[
R_{xs}[k] = R_{ss}[k]
\]
This simplification allows the optimal transfer function to be derived directly from the power spectral densities:
\[
H_{\text{Wiener}}(\omega) = \frac{P_{ss}(\omega)}{P_{ss}(\omega) + P_{vv}(\omega)}
\]
This mathematical derivation shows that the process requires the noise to be stationary and independent of the stationary signal, which matches Option (A).