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Concept in probability and statistics
In probability theory and statistics, given a stochastic process, the autocovariance is a function that gives the covariance of the process with itself at pairs of time points. Autocovariance is closely related to the autocorrelation of the process in question.
Auto-covariance of stochastic processes[edit]With the usual notation E {\displaystyle \operatorname {E} } for the expectation operator, if the stochastic process { X t } {\displaystyle \left\{X_{t}\right\}} has the mean function μ t = E [ X t ] {\displaystyle \mu _{t}=\operatorname {E} [X_{t}]} , then the autocovariance is given by[1]: p. 162
K X X ( t 1 , t 2 ) = cov [ X t 1 , X t 2 ] = E [ ( X t 1 − μ t 1 ) ( X t 2 − μ t 2 ) ] = E [ X t 1 X t 2 ] − μ t 1 μ t 2 {\displaystyle \operatorname {K} _{XX}(t_{1},t_{2})=\operatorname {cov} \left[X_{t_{1}},X_{t_{2}}\right]=\operatorname {E} [(X_{t_{1}}-\mu _{t_{1}})(X_{t_{2}}-\mu _{t_{2}})]=\operatorname {E} [X_{t_{1}}X_{t_{2}}]-\mu _{t_{1}}\mu _{t_{2}}} Eq.1where t 1 {\displaystyle t_{1}} and t 2 {\displaystyle t_{2}} are two instances in time.
Definition for weakly stationary process[edit]If { X t } {\displaystyle \left\{X_{t}\right\}} is a weakly stationary (WSS) process, then the following are true:[1]: p. 163
and
and
where τ = t 2 − t 1 {\displaystyle \tau =t_{2}-t_{1}} is the lag time, or the amount of time by which the signal has been shifted.
The autocovariance function of a WSS process is therefore given by:[2]: p. 517
K X X ( τ ) = E [ ( X t − μ t ) ( X t − τ − μ t − τ ) ] = E [ X t X t − τ ] − μ t μ t − τ {\displaystyle \operatorname {K} _{XX}(\tau )=\operatorname {E} [(X_{t}-\mu _{t})(X_{t-\tau }-\mu _{t-\tau })]=\operatorname {E} [X_{t}X_{t-\tau }]-\mu _{t}\mu _{t-\tau }} Eq.2which is equivalent to
It is common practice in some disciplines (e.g. statistics and time series analysis) to normalize the autocovariance function to get a time-dependent Pearson correlation coefficient. However in other disciplines (e.g. engineering) the normalization is usually dropped and the terms "autocorrelation" and "autocovariance" are used interchangeably.
The definition of the normalized auto-correlation of a stochastic process is
If the function ρ X X {\displaystyle \rho _{XX}} is well-defined, its value must lie in the range [ − 1 , 1 ] {\displaystyle [-1,1]} , with 1 indicating perfect correlation and −1 indicating perfect anti-correlation.
For a WSS process, the definition is
where
respectively for a WSS process:
The autocovariance of a linearly filtered process { Y t } {\displaystyle \left\{Y_{t}\right\}}
is
Autocovariance can be used to calculate turbulent diffusivity.[4] Turbulence in a flow can cause the fluctuation of velocity in space and time. Thus, we are able to identify turbulence through the statistics of those fluctuations[citation needed].
Reynolds decomposition is used to define the velocity fluctuations u ′ ( x , t ) {\displaystyle u'(x,t)} (assume we are now working with 1D problem and U ( x , t ) {\displaystyle U(x,t)} is the velocity along x {\displaystyle x} direction):
where U ( x , t ) {\displaystyle U(x,t)} is the true velocity, and ⟨ U ( x , t ) ⟩ {\displaystyle \langle U(x,t)\rangle } is the expected value of velocity. If we choose a correct ⟨ U ( x , t ) ⟩ {\displaystyle \langle U(x,t)\rangle } , all of the stochastic components of the turbulent velocity will be included in u ′ ( x , t ) {\displaystyle u'(x,t)} . To determine ⟨ U ( x , t ) ⟩ {\displaystyle \langle U(x,t)\rangle } , a set of velocity measurements that are assembled from points in space, moments in time or repeated experiments is required.
If we assume the turbulent flux ⟨ u ′ c ′ ⟩ {\displaystyle \langle u'c'\rangle } ( c ′ = c − ⟨ c ⟩ {\displaystyle c'=c-\langle c\rangle } , and c is the concentration term) can be caused by a random walk, we can use Fick's laws of diffusion to express the turbulent flux term:
The velocity autocovariance is defined as
where τ {\displaystyle \tau } is the lag time, and r {\displaystyle r} is the lag distance.
The turbulent diffusivity D T x {\displaystyle D_{T_{x}}} can be calculated using the following 3 methods:
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