## 8.7 Forecasting with ETS models

Point forecasts are obtained from the models by iterating the equations for $$t=T+1,\dots,T+h$$ and setting all $$\varepsilon_t=0$$ for $$t>T$$.

For example, for model ETS(M,A,N), $$y_{T+1} = (\ell_T + b_T )(1+ \varepsilon_{T+1}).$$ Therefore $$\hat{y}_{T+1|T}=\ell_{T}+b_{T}.$$ Similarly, \begin{align*} y_{T+2} &= (\ell_{T+1} + b_{T+1})(1 + \varepsilon_{T+1})\\ &= \left[ (\ell_T + b_T) (1+ \alpha\varepsilon_{T+1}) + b_T + \beta (\ell_T + b_T)\varepsilon_{T+1} \right] ( 1 + \varepsilon_{T+1}). \end{align*} Therefore, $$\hat{y}_{T+2|T}= \ell_{T}+2b_{T},$$ and so on. These forecasts are identical to the forecasts from Holt’s linear method, and also to those from model ETS(A,A,N). Thus, the point forecasts obtained from the method and from the two models that underlie the method are identical (assuming that the same parameter values are used).

ETS point forecasts are equal to the medians of the forecast distributions. For models with only additive components, the forecast distributions are normal, so the medians and means are equal. For ETS models with multiplicative errors, or with multiplicative seasonality, the point forecasts will not be equal to the means of the forecast distributions.

To obtain forecasts from an ETS model, we use the forecast() function.

fit %>% forecast(h=8) %>%
autoplot(aus_holidays) +
ylab("Domestic holiday visitors in Australia (thousands)")

### Prediction intervals

A big advantage of the models is that prediction intervals can also be generated — something that cannot be done using the methods. The prediction intervals will differ between models with additive and multiplicative methods.

For most ETS models, a prediction interval can be written as $\hat{y}_{T+h|T} \pm c \sigma_h$ where $$c$$ depends on the coverage probability, and $$\sigma_h^2$$ is the forecast variance. Values for $$c$$ were given in Table 3.1. For ETS models, formulas for $$\sigma_h^2$$ can be complicated; the details are given in Chapter 6 of Hyndman et al. (2008). In Table 8.8 we give the formulas for the additive ETS models, which are the simplest.

Table 8.8: Forecast variance expressions for each additive state space model, where $$\sigma^2$$ is the residual variance, $$m$$ is the seasonal period, and $$k$$ is the integer part of $$(h-1) /m$$ (i.e., the number of complete years in the forecast period prior to time $$T+h$$).
Model Forecast variance: $$\sigma_h^2$$
(A,N,N) $$\sigma_h^2 = \sigma^2\big[1 + \alpha^2(h-1)\big]$$
(A,A,N) $$\sigma_h^2 = \sigma^2\Big[1 + (h-1)\big\{\alpha^2 + \alpha\beta h + \frac16\beta^2h(2h-1)\big\}\Big]$$
(A,A$$_d$$,N) $$\sigma_h^2 = \sigma^2\biggl[1 + \alpha^2(h-1) + \frac{\beta\phi h}{(1-\phi)^2} \left\{2\alpha(1-\phi) +\beta\phi\right\}$$
$$\mbox{} - \frac{\beta\phi(1-\phi^h)}{(1-\phi)^2(1-\phi^2)} \left\{ 2\alpha(1-\phi^2)+ \beta\phi(1+2\phi-\phi^h)\right\}\biggr]$$
(A,N,A) $$\sigma_h^2 = \sigma^2\Big[1 + \alpha^2(h-1) + \gamma k(2\alpha+\gamma)\Big]$$
(A,A,A) $$\sigma_h^2 = \sigma^2\Big[1 + (h-1)\big\{\alpha^2 + \alpha\beta h + \frac16\beta^2h(2h-1)\big\}$$
$$\mbox{} + \gamma k \big\{2\alpha+ \gamma + \beta m (k+1)\big\} \Big]$$
(A,A$$_d$$,A) $$\sigma_h^2 = \sigma^2\biggl[1 + \alpha^2(h-1) + \gamma k(2\alpha+\gamma)$$
$$\mbox{} +\frac{\beta\phi h}{(1-\phi)^2} \left\{2\alpha(1-\phi) + \beta\phi \right\}$$
$$\mbox{} - \frac{\beta\phi(1-\phi^h)}{(1-\phi)^2(1-\phi^2)} \left\{ 2\alpha(1-\phi^2)+ \beta\phi(1+2\phi-\phi^h)\right\}$$
$$\mbox{} + \frac{2\beta\gamma\phi}{(1-\phi)(1-\phi^m)}\left\{k(1-\phi^m) - \phi^m(1-\phi^{mk})\right\}\biggr]$$

For a few ETS models, there are no known formulas for prediction intervals. In these cases, the forecast() function uses simulated future sample paths and computes prediction intervals from the percentiles of these simulated future paths.

### Bibliography

Hyndman, R. J., Koehler, A. B., Ord, J. K., & Snyder, R. D. (2008). Forecasting with exponential smoothing: The state space approach. Berlin: Springer-Verlag. http://www.exponentialsmoothing.net