On: “The Complex Wiener Filter” by Sven Treitel (GEOPHYSICS, April 1974, p. 169–173)
In this publication Treitel determines the complex normal equations and proposes a solution method (Robinson’s block‐Toeplitz algorithm). With respect to these results, I would like to draw attention to the paper Berkhout (1973). In Appendix B of that paper the complex normal equations were also derived: [Formula: see text]for n = 0, 1, ⋯ , N. In (1a), [Formula: see text] is the autocorrelation function of a complex input signal x(t), [Formula: see text] is the complex least‐squares filter of duration (N + 1)Δt, [Formula: see text] is the complex desired output, and Δt represents the sampling interval. Note that in matrix notation expression (1a) equals expression (3) of Treitel’s paper. In the case of least‐squares inverse filtering, (1a) takes on a different form.