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&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Short description|Variation of the Wigner distribution function}}&lt;br /&gt;
{{No footnotes|date=February 2025}}&lt;br /&gt;
:&amp;#039;&amp;#039;Note: the Wigner distribution function is abbreviated here as WD rather than WDF as used at [[Wigner distribution function]]&amp;#039;&amp;#039;&lt;br /&gt;
A &amp;#039;&amp;#039;&amp;#039;Modified Wigner distribution function&amp;#039;&amp;#039;&amp;#039; is a variation of the [[Wigner distribution function]] (WD) with reduced or removed cross-terms.&lt;br /&gt;
&lt;br /&gt;
The Wigner distribution (WD) was first proposed for corrections to classical statistical mechanics in 1932 by [[Eugene Wigner]]. The [[Wigner distribution function]], or Wigner&amp;amp;ndash;Ville distribution (WVD) for analytic signals, also has applications in time frequency analysis. The Wigner distribution gives better auto term localisation compared to the smeared out [[spectrogram]] (SP). However, when applied to a signal with multi frequency components, cross terms appear due to its quadratic nature. Several methods have been proposed to reduce the cross terms. For example, in 1994 [[Ljubiša Stanković]] proposed a novel technique, now mostly referred to as S-method, resulting in the reduction or removal of cross terms. The concept of the S-method is a combination between the spectrogram and the Pseudo Wigner Distribution (PWD), the windowed version of the WD.&lt;br /&gt;
&lt;br /&gt;
The original WD, the spectrogram, and the modified WDs all belong to the [[Cohen&amp;#039;s class]] of bilinear time-frequency representations :&lt;br /&gt;
:&amp;lt;math&amp;gt;C_x(t, f)=\int_{-\infty}^{\infty}\int_{-\infty}^{\infty}W_x(\theta,\nu) \Pi(t - \theta,f - \nu)\, d\theta\, d\nu \quad = [W_x\,\ast\,\Pi] (t,f)&amp;lt;/math&amp;gt;&lt;br /&gt;
where &amp;lt;math&amp;gt;\Pi \left(t, f\right)&amp;lt;/math&amp;gt; is Cohen&amp;#039;s  &amp;#039;&amp;#039;&amp;#039;kernel function&amp;#039;&amp;#039;&amp;#039;, which is often a low-pass function, and normally serves to mask out the interference in the original Wigner representation.&lt;br /&gt;
&lt;br /&gt;
== Mathematical definition ==&lt;br /&gt;
&lt;br /&gt;
*&amp;#039;&amp;#039;&amp;#039;Wigner distribution&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
:&amp;lt;math&amp;gt; W_x(t,f) = \int_{-\infty}^\infty x(t+\tau/2) x^*(t-\tau/2) e^{-j2\pi\tau f} \, d\tau&amp;lt;/math&amp;gt;&lt;br /&gt;
Cohen&amp;#039;s kernel function : &amp;lt;math&amp;gt;\Pi (t,f) = \delta_{(0,0)} (t,f) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
*&amp;#039;&amp;#039;&amp;#039;Spectrogram&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
:&amp;lt;math&amp;gt;SP_x (t,f) = |ST_x (t,f)|^2 = ST_x (t,f)\,ST_x^* (t,f)&amp;lt;/math&amp;gt;&lt;br /&gt;
where &amp;lt;math&amp;gt;ST_x&amp;lt;/math&amp;gt; is the [[short-time Fourier transform]] of &amp;lt;math&amp;gt;x&amp;lt;/math&amp;gt;. &lt;br /&gt;
:&amp;lt;math&amp;gt; ST_x(t,f) = \int_{-\infty}^\infty x(\tau) w^*(t-\tau) e^{-j2\pi f\tau} \, d\tau&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Cohen&amp;#039;s kernel function : &amp;lt;math&amp;gt;\Pi (t,f) = W_h(t,f) &amp;lt;/math&amp;gt; which is the WD of the window function itself. This can be verified by applying the convolution property of the [[Wigner distribution function]].&lt;br /&gt;
&lt;br /&gt;
The spectrogram cannot produce interference since it is a positive-valued quadratic distribution.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Modified form I&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; W_x(t,f) = \int_{-B}^B w(\tau)x(t+\tau/2) x^*(t-\tau/2) e^{-j2\pi\tau f} \, d\tau&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Can&amp;#039;t solve the cross term problem, however it can solve the problem of 2 components time difference larger than window size B.&lt;br /&gt;
&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Modified form II&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; W_x(t,f) = \int_{-B}^B w(\eta)X(f+\eta/2) X^*(f-\eta/2) e^{j2\pi t \eta} \, d\eta&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Modified form III (Pseudo L-Wigner Distribution)&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; W_x(t,f) = \int_{-\infty}^\infty w(\tau)x^L(t+\tau/(2L)) \overline{x^{*L}(t-\tau/(2L))} e^{-j2\pi \tau f} \, d\tau&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Where L is any integer greater than 0&lt;br /&gt;
&lt;br /&gt;
Increase L can reduce the influence of cross term (however it can&amp;#039;t eliminate completely )&lt;br /&gt;
&lt;br /&gt;
For example, for L=2, the dominant third term is divided by 4 ( which is equivalent to 12dB ).&lt;br /&gt;
&lt;br /&gt;
This gives a significant improvement over the Wigner Distribution.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Properties of L-Wigner Distribution:&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
# The L-Wigner Distribution is always real.&lt;br /&gt;
# If the signal is time shifted &amp;lt;math&amp;gt; x(t-t0)&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&amp;#039;&amp;#039;,&amp;#039;&amp;#039; then its LWD is time shifted as well, &amp;lt;math&amp;gt; LWD: W_x(t-t0,f)&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
# The LWD of a modulated signal &amp;lt;math&amp;gt; x(t)\exp(j\omega_0 t)&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;is shifted in frequency &amp;lt;math&amp;gt; LWD: W_x(t,f-f0)&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
# Is the signal &amp;lt;math&amp;gt; x(t)&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;is time limited, i.e.,&amp;lt;math&amp;gt; x(t)=0 &lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt; &amp;lt;math&amp;gt; for \left\vert t \right\vert &amp;gt;T,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt; then the L-Wigner distribution is time limited, &amp;lt;math&amp;gt; LWD: W_x(t,f)=0&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt; &amp;lt;math&amp;gt; for\left\vert t \right\vert &amp;gt;T&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
# If the signal &amp;lt;math&amp;gt; x(t)&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;is band limited with &amp;lt;math&amp;gt; f_m&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;(&amp;lt;math&amp;gt; F(f)=0&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&amp;lt;math&amp;gt; for \left\vert f \right\vert &amp;gt; f_m&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;), then &amp;lt;math&amp;gt; LWD: W_x(t,f)&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;is limited in the frequency domain by &amp;lt;math&amp;gt; f_m&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;as well.&lt;br /&gt;
# Integral of L-Wigner distribution over frequency is equal to the generalized signal power: &amp;lt;math&amp;gt; \int_{-\infty}^\infty W_x(t, f)df = \left\vert x(t) \right\vert ^{2L}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
# Integral of &amp;lt;math&amp;gt; LWD: W_x(t,f)&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;over time and frequency is equal to the &amp;lt;math&amp;gt; 2L^{th}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;power of the &amp;lt;math&amp;gt; 2L^{th}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;norm of signal &amp;lt;math&amp;gt; x(t)&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;: &lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \int_{-\infty}^\infty \int_{-\infty}^\infty W_x(t,f)dtdf = \int_{-\infty}^\infty \left\vert x(t) \right\vert ^{2L} dt = \lVert x(t) \rVert _{2L} ^{2L}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
# The integral over time is:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \int_{-\infty}^\infty W_x(t,f)dt = \left\vert F_L(f) \right\vert ^2=\left\vert \underbrace{ F(L_f)*F(L_f)*\cdots*F(L_f) }_{L times} \right\vert ^2&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
# For a large value of &amp;lt;math&amp;gt; L(L\rightarrow \infty)&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;We may neglect all values of &amp;lt;math&amp;gt; LWD: W_x(t,f)&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;, Comparing them to the one at the points &amp;lt;math&amp;gt; (t_m, f_m)&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;, where the distribution reaches its essential supremum:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \lim_{L \to \infty} (W_x(t,f)/W_x(t_m,f_m)) = \begin{cases} 0, &amp;amp; \text{if }f \neq f_m\text{  or }t\neq t_m\text{ } \\ 1, &amp;amp; \text{if }f=f_m\text{ and } t=t_m\end{cases}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;  &amp;lt;br /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Modified form IV (Polynomial Wigner Distribution Function)&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; W_x(t,f) = \int_{-B}^B [\textstyle \prod_{l=1}^{q/2} \displaystyle x(t+d_l \tau) x^*(t- d_{-l} \tau)] e^{-j2\pi\tau f} \, d\tau&lt;br /&gt;
         &lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
When &amp;lt;math&amp;gt; q=2&lt;br /&gt;
&lt;br /&gt;
         &lt;br /&gt;
&amp;lt;/math&amp;gt; and &amp;lt;math&amp;gt; d_l=d_{-l}=0.5&lt;br /&gt;
         &lt;br /&gt;
&amp;lt;/math&amp;gt;, it becomes the original Wigner distribution function.&lt;br /&gt;
&lt;br /&gt;
It can avoid the cross term when the order of phase of the exponential function is no larger than &amp;lt;math&amp;gt; q/2+1&lt;br /&gt;
         &lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
However the cross term between two components cannot be removed.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; d_l&lt;br /&gt;
         &lt;br /&gt;
&amp;lt;/math&amp;gt;should be chosen properly such that&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \textstyle \prod_{l=1}^{q/2} \displaystyle x(t+d_l \tau) x^*(t-d_{-l}\tau)=\exp\big(j2\pi\textstyle \sum_{n=1}^{q/2+1} n a_n t^{n-1}\tau \displaystyle\big)&lt;br /&gt;
         &lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; W_x(t,f) = \int_{-\infty}^\infty \exp\Bigl(-j2\pi (f-\sum_{n=1}^{q/2+1}na_nt^{n-1})\tau\Bigr)d\tau&lt;br /&gt;
         &lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \cong \delta\bigl(f-\sum_{n=1}^{q/2+1}na_nt^{n-1}\bigr)&lt;br /&gt;
         &lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt; x(t)=\exp\bigl(j2\pi\sum_{n=1}^{q/2+1}a_nt^n\bigr)&lt;br /&gt;
         &lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
when &amp;lt;math&amp;gt; q=2     &lt;br /&gt;
         &lt;br /&gt;
&amp;lt;/math&amp;gt; ,   &amp;lt;math&amp;gt; x(t+d_l \tau) x^*(t-d_{-l}\tau)=\exp\bigl(j2\pi\sum_{n=1}^{q/2+1}na_nt^{n-1}\tau\bigr)&lt;br /&gt;
         &lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; a_2(t+d_l\tau)^2+a_1(t+d_l\tau)-a_2(t-d_{-l}\tau)^2-a_1(t-d_{-l}\tau)=2a_2t\tau+a_1\tau&lt;br /&gt;
         &lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \Longrightarrow d_l+d_{-l}=1, d_l-d_{-l}=0&lt;br /&gt;
&lt;br /&gt;
         &lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \Longrightarrow d_l=d_{-l}=1/2&lt;br /&gt;
         &lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
*&amp;#039;&amp;#039;&amp;#039;Pseudo Wigner distribution&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
:&amp;lt;math&amp;gt; PW_x(t,f) = \int_{-\infty}^\infty w(\tau/2) w^*(-\tau/2) x(t+\tau/2) x^*(t-\tau/2) e^{-j2\pi\tau\,f} \, d\tau&amp;lt;/math&amp;gt;&lt;br /&gt;
Cohen&amp;#039;s kernel function : &amp;lt;math&amp;gt;\Pi (t,f) = \delta_0 (t)\,W_h(t,f) &amp;lt;/math&amp;gt; which is concentred on the frequency axis.&lt;br /&gt;
&lt;br /&gt;
Note that the pseudo Wigner can also be written as the Fourier transform of the “spectral-correlation” of the STFT&lt;br /&gt;
:&amp;lt;math&amp;gt; PW_x(t,f) = \int_{-\infty}^\infty ST_x(t, f+\nu/2) ST_x^*(t, f-\nu/2) e^{j2\pi\nu\,t} \, d\nu&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
*&amp;#039;&amp;#039;&amp;#039;Smoothed pseudo Wigner distribution&amp;#039;&amp;#039;&amp;#039; : &lt;br /&gt;
In the pseudo Wigner the time windowing acts as a frequency direction smoothing. Therefore, it suppresses the Wigner distribution interference components that oscillate in the frequency direction. Time direction smoothing can be implemented by a time-convolution of the PWD with a lowpass function &amp;lt;math&amp;gt;q&amp;lt;/math&amp;gt; :&lt;br /&gt;
:&amp;lt;math&amp;gt; SPW_x(t,f) = [ q\,\ast\, PW_x (.,f)] (t) =  \int_{-\infty}^\infty q(t-u) \int_{-\infty}^\infty w(\tau/2) w^*(-\tau/2) x(u+\tau/2) x^*(u-\tau/2) e^{-j2\pi\tau\,f} \, d\tau\, du&amp;lt;/math&amp;gt;&lt;br /&gt;
Cohen&amp;#039;s kernel function : &amp;lt;math&amp;gt;\Pi (t,f) = q(t)\, W(f) &amp;lt;/math&amp;gt; where &amp;lt;math&amp;gt;W&amp;lt;/math&amp;gt; is the Fourier transform of the window &amp;lt;math&amp;gt;w&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
Thus the kernel corresponding to the smoothed pseudo Wigner distribution has a separable form. Note that even if the SPWD and the S-Method both smoothes the WD in the time domain, they are not equivalent in general.&lt;br /&gt;
&lt;br /&gt;
*&amp;#039;&amp;#039;&amp;#039;S-method&amp;#039;&amp;#039;&amp;#039; &lt;br /&gt;
:&amp;lt;math&amp;gt; SM(t,f) = \int_{-\infty}^\infty ST_x(t, f+\nu/2) ST_x^*(t, f-\nu/2) G(\nu) e^{j2\pi\nu\,t} \, d\nu&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Cohen&amp;#039;s kernel function : &amp;lt;math&amp;gt;\Pi (t,f) = g(t)\, W_h(t,f) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The S-method limits the range of the integral of the PWD with a low-pass windowing function &amp;lt;math&amp;gt;g(t)&amp;lt;/math&amp;gt; of Fourier transform &amp;lt;math&amp;gt;G(f)&amp;lt;/math&amp;gt;. This results in the cross-term removal, without blurring the auto-terms that are well-concentred along the frequency axis.&lt;br /&gt;
The S-method strikes a balance in smoothing between the pseudo-Wigner distribution &amp;lt;math&amp;gt;PW_x&amp;lt;/math&amp;gt; [&amp;lt;math&amp;gt;g(t) = 1&amp;lt;/math&amp;gt;] and the power spectrogram &amp;lt;math&amp;gt;SP_x&amp;lt;/math&amp;gt; [&amp;lt;math&amp;gt;g(t) = \delta_0 (t)&amp;lt;/math&amp;gt;].&lt;br /&gt;
&lt;br /&gt;
Note that in the original 1994 paper, Stankovic defines the S-methode with a modulated version of the short-time Fourier transform : &lt;br /&gt;
:&amp;lt;math&amp;gt; SM(t,f) = \int_{-\infty}^\infty \tilde{ST}_x(t,f+\nu) \tilde{ST}_x^*(t,f-\nu) P(\nu)\, d\nu &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \tilde{ST}_x(t,f) = \int_{-\infty}^\infty x(t+\tau) w^*(\tau) e^{-j2\pi f\tau} \, d\tau \quad = ST_x(t,f)\,e^{j2\pi f t}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Even in this case we still have&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\Pi (t,f) = p(2t)\, W_h(t,f) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== See also ==&lt;br /&gt;
* [[Time-frequency representation]]&lt;br /&gt;
* [[Wigner distribution function]]&lt;br /&gt;
* [[Bilinear time–frequency distribution]]&lt;br /&gt;
* [[Short-time Fourier transform]]&lt;br /&gt;
* [[Gabor transform]]&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
*P. Gonçalves and R. Baraniuk, “Pseudo Affine Wigner Distributions : Definition and Kernel Formulation”, IEEE Transactions on Signal Processing, vol. 46, no. 6, Jun. 1998&lt;br /&gt;
*L. Stankovic, “A Method for Time-Frequency Analysis”, IEEE Transactions on Signal Processing, vol. 42, no. 1, Jan. 1994&lt;br /&gt;
*L. J. Stankovic, S. Stankovic, and E. Fakultet, “An analysis of instantaneous frequency representation using time frequency distributions-generalized Wigner distribution,” &amp;#039;&amp;#039;IEEE Trans. on Signal Processing,&amp;#039;&amp;#039; pp. 549-552, vol. 43, no. 2, Feb. 1995 &lt;br /&gt;
&lt;br /&gt;
[[Category:Signal processing]]&lt;br /&gt;
[[Category:Transforms]]&lt;/div&gt;</summary>
		<author><name>imported&gt;Yodo9000</name></author>
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