For , iterating an AR(1) from a fixed value gives the displayed finite sum. With centered white noise of variance and ,
For , its covariance is , which depends on . Even setting leaves a changing variance. At , , and , the variances at times zero through three are , approaching ; this finite initialized record is not weakly stationary.
To initialize in weak stationarity, give mean , variance , and zero covariance with every future driving noise value. The full stationary construction sets . For discrete Gaussian white noise, equivalently draw from independently of future noise. This gives exact strict stationarity from the first plotted point; it is the initialization used in the figure in time series. Matching these first two moments alone does not guarantee strict stationarity for non-Gaussian inputs. See also stationary initialization of a scalar linear state-space model.
Take the latent autoregression as the scalar state . A state-space model is
The transition and observation matrices are both scalar, , . State-noise variance is , observation-noise variance is , and the cross-noise covariance is zero at every pair of times.
A complete stationary initialization is
It is orthogonal to future state noise and to all observation noise. This is the stationary initialization of a scalar linear state-space model. This specifies the initial state in terms of the actual given two-sided white noise sequence, as well as its second-order law; simply starting from zero would give transient rather than stationary observations.
If a Gaussian state-space specification is intended, the complete specialization is , independent of the future iid Gaussian state and observation noises, themselves independent with variances . Under the printed assumptions alone, Gaussian distributions and independence cannot be deduced from white noise orthogonality; the equations and stationary-series initialization above give the exact second-order representation without adding them.