Geology Reference
In-Depth Information
In general, this is not a satisfactory definition for energy signals since it would
give zero for all lags. For energy signals, the autocorrelation is given the relaxed
definition
f l f l k .
φ ff ( k )
=
(2.22)
l =−∞
While this definition might appear to be inconsistent with the ensemble definition
of autocorrelation, we shall see later that if we form a stochastic process in which
the deterministic energy signal is taken to begin at random times with random
amplitudes, it becomes a consistent definition for such a process.
The crosscorrelation of the sequence f j with the sequence g j at lag k , time
index l ,isdefinedtobe
E f l g l k .
φ f g ( k , l )
=
(2.23)
Once again, for stationary sequences, the dependence on time index disappears and
E f l g l k
E g m f m + k = φ g f (
φ f g ( k )
=
=
k ).
(2.24)
Accepting the ergodic hypothesis for two stationary power signals yields the equi-
valent definition
N
1
f l g l k .
φ f g ( k )
=
lim
N →∞
(2.25)
2 N
+
1
l
=−
N
For two energy signals, or one energy signal and one power signal, the definition
is relaxed to
f l g l k .
φ f g ( k )
=
(2.26)
l =−∞
Again, we shall see later how this definition can be made consistent with the
ensemble average definition.
We can make a connection between autocorrelation, crosscorrelation and con-
volution by introducing the time reverse of a sequence. The time reverse of the
sequence f j is simply defined as the sequence f j .If f j and g j are two energy
signals, the crosscorrelation of f j with g j is
f l g l k =
φ f g ( k )
=
f l h k l ,
(2.27)
l =−∞
l =−∞
= g j , the time reverse of g j . Hence, the crosscorrelation of f j
with g j is the same as the convolution of f j with the time reverse of g j . Similarly,
the autocorrelation of an energy signal is the same as its convolution with its own
time reverse.
= g l k or h j
with h k l
Search WWH ::




Custom Search