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Shumway Stoffer Time_Series_Analysis_and_Its_Applications__With_R_Examples 3rd edition (1)

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28 1 Characteristics of Time Series

assumed to be positive definite, the multivariate normal density function can

be written as

{

f(x) = (2π) −n/2 |Γ | −1/2 exp − 1 }

2 (x − µ)′ Γ −1 (x − µ) , (1.31)

where |·| denotes the determinant. This distribution forms the basis for solving

problems involving statistical inference for time series. If a Gaussian time

series, {x t }, is weakly stationary, then µ t = µ and γ(t i , t j ) = γ(|t i − t j |),

so that the vector µ and the matrix Γ are independent of time. These facts

imply that all the finite distributions, (1.31), of the series {x t } depend only

on time lag and not on the actual times, and hence the series must be strictly

stationary.

1.6 Estimation of Correlation

Although the theoretical autocorrelation and cross-correlation functions are

useful for describing the properties of certain hypothesized models, most of

the analyses must be performed using sampled data. This limitation means

the sampled points x 1 , x 2 , . . . , x n only are available for estimating the mean,

autocovariance, and autocorrelation functions. From the point of view of classical

statistics, this poses a problem because we will typically not have iid

copies of x t that are available for estimating the covariance and correlation

functions. In the usual situation with only one realization, however, the assumption

of stationarity becomes critical. Somehow, we must use averages

over this single realization to estimate the population means and covariance

functions.

Accordingly, if a time series is stationary, the mean function (1.21) µ t = µ

is constant so that we can estimate it by the sample mean,

¯x = 1 n∑

x t . (1.32)

n

The standard error of the estimate is the square root of var(¯x), which can be

computed using first principles (recall footnote 3 on page 20), and is given by

( ) (

1

n∑

var(¯x) = var x t = 1 n

)

n

n 2 cov ∑ n∑

x t , x s

t=1

t=1

t=1

= 1 (nγ

n 2 x (0) + (n − 1)γ x (1) + (n − 2)γ x (2) + · · · + γ x (n − 1)

)

+ (n − 1)γ x (−1) + (n − 2)γ x (−2) + · · · + γ x (1 − n)

= 1 n∑ (

1 − |h| )

γ x (h). (1.33)

n

n

h=−n

s=1

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