The Rihaczek and Margenau-Hill distributions
Another
possible definition of a time-frequency energy density is given by the
Rihaczek distribution. If we consider the interaction energy between a
signal

restricted to an infinitesimal interval

centered on

, and

passed through an infinitesimal bandpass filter

centered on

, it can be approximated by the following expression:
This leads us to interpret the quantity
called the
Rihaczek distribution, as a complex energy density at
point

. This distribution, which corresponds to the element of
the Cohen's class for which

, verifies many
good properties (1-2, 4-11, see section
4.1.1). However, it
is complex valued, which can be awkward in practice. It is implemented
under the name
tfrri.m. The real part of
the Rihaczek distribution is also a time-frequency distribution of the
Cohen's class (

), known as the
Margenau-Hill distribution (see the M-file
tfrmh.m). It has also numerous interesting properties:
1-5, 8, 10-11. As for the WVD, we can define smoothed versions of the
Rihaczek and Margenau-Hill distributions. The file
tfrpmh.m computes the pseudo Margenau-Hill distribution.
The interference structure of the Rihaczek and Margenau-Hill
distributions is different from the Wigner-Ville one: the interference
terms corresponding to two points located on
and
are positioned at the coordinates
and
. This can be seen on the following example (see
fig. 4.14):
>> sig=atoms(128,[32,0.15,20,1;96,0.32,20,1]);
>> tfrmh(sig);
Figure 4.14:
Margenau-Hill distribution of 2 atoms : the
position of the interferences is quite different from the one obtained with
the WVD
 |
Thus, the use of the Rihaczek (or Margenau-Hill) distribution for signals
composed of multi-components located at the same position in time or in
frequency is not advised, since the interference terms will then be
superposed to the signal terms.
Eric Chassande-Mottin
2005-10-26