2 Introduction to Time Series Analysis
The goal of this lecture is to introduce time series and their common components. You should become confident in identifying and characterizing trends, seasonal and other variability based on visual analysis of time series plots and plots of autocorrelation functions.
Objectives
 Define time series, common components (decomposition), and patterns to look out for (outliers, change points, heteroskedasticity).
 Discuss peculiarities of assessing (crossvalidating) regression models built for time series.
 Distinguish simple models for univariate time series (building blocks for more complex models).
 Define autocorrelation and partial autocorrelation and interpret such estimates.
 Explain the assumption of stationarity for calculating autocorrelation.
Reading materials
 Chapters 1.1–1.4 in Brockwell and Davis (2002)
2.1 Time series and its components
A time series is a set of observations \(Y_t\), each one being recorded at a specific time \(t\) (Brockwell and Davis 2002). The index \(t\) will typically refer to some standard unit of time, e.g., seconds, hours, days, weeks, months, or years.
A time series is a collection of observations made sequentially through time (Chatfield 2000).
A stochastic process is a sequence of random variables \(Y_t\), \(t = 1, 2, \dots\) indexed by time \(t\), which can be written as \(Y_t\), \(t \in [1,T]\). A time series is a realization of a stochastic process.
We shall frequently use the term time series to mean both the data and the process.
Let’s try to describe the patterns we see in Figure 2.1, Figure 2.2, and Figure 2.3.
Code
p < forecast::autoplot(TSstudio::Michigan_CS) +
xlab("") +
ylab("Index") +
theme_light()
plotly::ggplotly(p)
Code
ggplot2::autoplot(JohnsonJohnson) +
xlab("") +
ylab("Earnings per share (USD)") +
theme_light()
Code
In this course, we will be interested in constructing time series models to learn more about their properties and to forecast (predict) future values of \(Y_t\), i.e., values of \(Y_t\) for \(t\) beyond the end of the data set. Typically, we will use the historical data (or some appropriate subset of it) to build our forecasting models.
2.2 Decomposition of time series
A time series can generally be expressed as a sum or product of four distinct components: \[ Y_t = M_t + S_t + C_t + \epsilon_t \] or \[ Y_t = M_t \cdot S_t \cdot C_t \cdot \epsilon_t, \] where

\(M_t\) is the trend, representing the average change (change in the mean) in the time series over time. Examples of trends are:
\(M_t = \beta_0\) (constant over time, we usually refer to this case as ‘no trend’);
\(M_t = \beta_0 + \beta_1t\) (linear increase or decrease over time);
\(M_t = \beta_0 + \beta_1t + \beta_2t^2\) (quadratic over time).
 \(S_t\) represents regular periodic fluctuations (a.k.a. seasonality) in the time series. \(S_t\) has the property that it is not constant but there exists an integer \(m \geqslant 2\) and scaling factors \(\lambda_k > 0\) such that \(S_{t+km} = \lambda_kS_t\) for \(1 \leqslant t \leqslant m\) and each \(k \geqslant 1\). The smallest such \(m\) is called the period. Periodic time series are quite common and include seasonal variability (the period is 1 year), diurnal (the period is 24 hours), and other cycles such as tides (the period is 12 hours 25 minutes). This component can be modeled using sinusoidal functions or indicator variables.
 \(C_t\) represents irregular cyclical fluctuations, i.e., sinusoidaltype movements that are of irregular length and are not as predictable as the seasonal component, e.g., El Niño Southern Oscillation (ENSO) and macroeconomic business cycles. We do not explicitly model \(C_t\) in this course.
 \(\epsilon_t\) is the residual or error and represents the remaining unexplained variation in \(Y_t\). In other words, it is a random or stochastic component.
Figure 2.4 illustrates an automatic decomposition, however, because the user has too little control over how the decomposition is done, this function is not recommended. We will talk about the alternatives in the next lecture.
2.3 General approach to time series modeling
 Plot the series and examine the main features of the graph, checking whether there is
 a trend,
 a seasonal or another periodic component,
 any apparent sharp changes in behavior,
 any outlying observations.
 Remove the trend and periodic components to get stationary residuals (this step is called detrending and deseasonalizing). Broadly speaking, a time series is said to be stationary if there is
 no systematic change in the mean (no trend);
 no systematic change in the variance, and
 no strictly periodic variations.
 Choose a model to fit the residuals, making use of various sample statistics, including the sample autocorrelation function (ACF).
 Forecast the residuals and then invert the transformations to arrive at forecasts of the original series.
There are two general classes of forecasting models.
Univariate time series models include different types of exponential smoothing, trend models, autoregressive models, etc. The characteristic feature of these models is that we need only one time series to start with (\(Y_t\)), then we can build a regression of this time series over time (\(Y_t \sim t\)) for estimating the trend or, for example, an autoregressive model (‘auto’ \(=\) self). In the autoregressive approach, the current value \(Y_t\) is modeled as a function of the past values: \[ Y_t = f(Y_{t1}, Y_{t2}, \dots, Y_{tp}) + \epsilon_t, \tag{2.1}\] while a linear autoregressive model has the form (assume that function \(f(\cdot)\) is a linear parametric function, with parameters \(\phi_0, \phi_1, \dots, \phi_p\)): \[ Y_t = \phi_0 + \phi_1 Y_{t1} + \phi_2 Y_{t2} + \dots +\phi_p Y_{tp} + \epsilon_t. \]
Multivariate models involve additional covariates (a.k.a. regressors, predictors, or independent variables) \(X_{1,t}, X_{2,t}, \dots, X_{k,t}\). A multivariate time series model can be as simple as the multiple regression \[ Y_t = f(X_{1,t}, X_{2,t}, \dots, X_{k,t}) + \epsilon_t, \] or involve autoregressive components of the response (and predictors): \[ \begin{split} Y_t = f(&X_{1,t}, X_{2,t}, \dots, X_{k,t}, \\ &X_{1,t1}, X_{1,t2}, \dots, X_{1,tq1}, \\ &\dots\\ &X_{k,t1}, X_{k,t2}, \dots, X_{k,tqk}, \\ &Y_{t1}, Y_{t2}, \dots, Y_{tp}) + \epsilon_t, \end{split} \tag{2.2}\] where \(p\), \(q1, \dots, qk\) are the lags. We can start the analysis with many variables and build a forecasting model as complex as Equation 2.2, but remember that a simpler univariate model may also work well. We should create an appropriate univariate model (like in Equation 2.1) to serve as a baseline, then compare the models’ performance on some outofsample data, as described in Section 2.4.
2.4 Model comparison
How do we compare forecasting models to decide which one is better? We will look at various ways of choosing between models as the course progresses, but the most obvious answer is to see which one is better at predicting.
Suppose we have used the data \(Y_1, \dots, Y_n\) to build \(M\) forecasting models \(\hat{Y}^{(m)}_t\) (\(m = 1,\dots,M\)) and we now obtain future observations \(Y_{n+1}, \dots, Y_{n+k}\) that were not used to fit the models (also called outofsample data, aftersample, or the testing set; \(k\) is the size of this set). The difference \(Y_t  \hat{Y}^{(m)}_t\) is the forecast (or prediction) error at the time \(t\) for the \(m\)th model. For each model, compute the prediction mean square error (PMSE) \[ PMSE_m = k^{1}\sum_{t=n+1}^{n+k}\left(Y_t  \hat{Y}^{(m)}_t\right)^2 \tag{2.3}\] and prediction mean absolute error (PMAE) \[ PMAE_m = k^{1}\sum_{t=n+1}^{n+k}\leftY_t  \hat{Y}^{(m)}_t\right \tag{2.4}\] and, similarly, prediction root mean square error (PRMSE; \(PRMSE = \sqrt{PMSE}\)), prediction mean absolute percentage error (PMAPE, if \(Y_t \neq 0\) in the testing period), etc. We choose the model with the smallest error.
One obvious drawback to the above method is that it requires us to wait for future observations to compare models. A way around this is to take the historical dataset \(Y_1, \dots, Y_n\) and split it into a training set \(Y_1, \dots, Y_k\) and a testing set \(Y_{k+1}, \dots, Y_n\), where \((n  k)\ll k\), i.e., most of the data goes into the training set.
Forecasting models are then built using only the training set and used to ‘forecast’ values from the testing set. Sometimes it is called an outofsample forecast because we predict values for the times we have not used for the model specification and estimation. The testing set is used as a set of future observations to compute the PMSE. The PMSE and other errors are computed for each model over the testing set and then compared to see errors for which models are smaller.
If two models produce approximately the same errors, we choose the model that is simpler (involves fewer variables). This is called the law of parsimony.
The above error measures (PMSE, PRMSE, PMAE, etc.) compare observed and forecasted data points, hence, are measures of the accuracy of the point forecasts. Another way of comparing models could be based on the quality of their interval forecasts, i.e., by assessing how good the prediction intervals are. To assess the quality of interval forecasts, one may start by computing the empirical coverage (proportion of observations in the testing set that are within – covered by – corresponding prediction intervals for given confidence \(C\), e.g., 95%) and average interval width. Prediction intervals are wellcalibrated if empirical coverage is close to \(C\) (more important) while intervals are not too wide (less important).
We may compare a great number of models using the training set, and choose the best one (with the smallest errors), however, it would be unfair to use the outofsample errors from the testing set for demonstrating the model performance because this part of the sample was used to select the model. Thus, it is advisable to have one more chunk of the same time series that was not used for model specification, estimation, or selection. Errors of the selected model on this validation set will be closer to the true (genuine) outofsample errors and can be used to improve coverage of true outofsample forecasts when the model is finally deployed.
2.5 Some simple time series models
Recall that a random process is a sequence of random variables, so its model would be the joint distribution of these random variables \[ f_1(Y_{t_1}), \; f_2(Y_{t_1}, Y_{t_2}), \; f_3(Y_{t_1}, Y_{t_2}, Y_{t_3}), \dots \]
With sample data, usually, we cannot estimate so many parameters. Instead, we use only first and secondorder moments of the joint distributions, i.e., \(\mathrm{E}(Y_t)\) and \(\mathrm{E}(Y_tY_{t+h})\). In the case when all the joint distributions are multivariate normal (MVN), these secondorder properties completely describe the sequence (we do not need any other information beyond the first two moments in this case).
 i.i.d. noise – independent and identically distributed random variables with zero mean. There is no dependence between observations, at any moment. The joint distribution function is \[ \Pr[Y_1\leqslant y_1, \dots, Y_n\leqslant y_n] = \Pr[Y_1\leqslant y_1]\dots \Pr[Y_n\leqslant y_n]. \] and the forecast is 0 (zero).
 binary process is a case of i.i.d. process with \(0 < p < 1\), and \[ \begin{split} \Pr[X_t=1]& = p, \\ \Pr[X_t=1]& = 1p. \end{split} \]
 random walk is a cumulative sum of i.i.d. noise: \[ S_t=X_1+X_2+\dots +X_t = \sum_{i=1}^t X_i, \] where \(t=1,2,\dots\), and \(X_t\) is i.i.d. noise.
 white noise (WN) is a sequence of uncorrelated random variables, each with zero mean and finite variance \(\sigma^2\). An i.i.d.(0,\(\sigma^2\)) series is also WN(0,\(\sigma^2\)), but not conversely.
2.6 Autocorrelation function
It is time to give more formal definitions of stationarity. Loosely speaking, a time series \(X_t\) (\(t=0,\pm 1, \dots\)) is stationary if it has statistical properties similar to those of the timeshifted series \(X_{t+h}\) for each integer \(h\).
Let \(X_t\) be a time series with \(\mathrm{E}(X^2_t)<\infty\), then the mean function of \(X_t\) is \[ \mu_X(t)=\mathrm{E}(X_t). \]
The autocovariance function of \(X_t\) is \[ \gamma_X(r,s) = \mathrm{cov}(X_r,X_s) = \mathrm{E}[(X_r\mu_X(r))(X_s\mu_X(s))] \tag{2.5}\] for all integers \(r\) and \(s\).
Weak stationarity
\(X_t\) is (weakly) stationary if \(\mu_X(t)\) is independent of \(t\), and \(\gamma_X(t+h,t)\) is independent of \(t\) for each \(h\) (consider only the first two moments): \[ \begin{split} \mathrm{E}(X_t) &= \mu, \\ \mathrm{cov}(X_t, X_{t+h}) &= \gamma_X(h) < \infty. \end{split} \tag{2.6}\]
Strong stationarity
\(X_t\) is strictly stationary if (\(X_1, \dots, X_n\)) and (\(X_{1+h}, \dots, X_{n+h}\)) have the same joint distribution (consider all moments).
Strictly stationary \(X_t\) with finite variance \(\mathrm{E}(X_t^2) <\infty\) for all \(t\) is also weakly stationary.
If \(X_t\) is a Gaussian process, then strict and weak stationarity are equivalent (i.e., one form of stationarity implies the other).
Given the second condition of weak stationarity in Equation 2.6, we can write for stationary(!) time series the autocovariance function (ACVF) for the lag \(h\): \[ \gamma_X(h)= \gamma_X(t+h,t) = \mathrm{cov}(X_{t+h},X_t) \] and the autocorrelation function (ACF), which is the normalized autocovariance: \[ \rho_X(h)=\frac{\gamma_X(h)}{\gamma_X(0)}=\mathrm{cor}(X_{t+h},X_t). \]
The sample autocovariance function is defined as: \[
\hat{\gamma}_X(h)= n^{1}\sum_{t=1}^{nk}(x_{t+h} \bar{x})(x_t  \bar{x}),
\] with \(\hat{\gamma}_X(h) = \hat{\gamma}_X(h)\) for \(h = 0,1,\dots, n1\). In R, use acf(X, type = "covariance")
.
The sample autocorrelation function is defined as (in R, use acf(X)
): \[
\hat{\rho}_X(h)=\frac{\hat{\gamma}_X(h)}{\hat{\gamma}_X(0)}.
\]
2.6.1 Properties of autocovariance and autocorrelation functions
 Linearity: if \(\mathrm{E}(X^2) < \infty\), \(\mathrm{E}(Y^2) < \infty\), \(\mathrm{E}(Z^2) < \infty\) and \(a\), \(b\), and \(c\) are any real constants, then \[ \mathrm{cov}(aX + bY + c, Z) = a\mathrm{cov}(X,Z) + b\mathrm{cov}(Y,Z). \]
 \(\gamma(0) \geqslant 0\).
 \(\gamma(h) \leqslant \gamma(0)\) for all \(h\).
 \(\gamma(\cdot)\) is even: \(\gamma(h) = \gamma(h)\) for all \(h\).
 \(\gamma(\cdot)\) is nonnegative definite: \[ \sum_{i,j=1}^na_i \gamma(ij)a_j\geqslant 0, \] for all positive integers \(n\) and vectors \(\boldsymbol{a} = (a_1, \dots, a_n)^{\top}\) with realvalued elements \(a_i\).
 The autocorrelation function \(\rho(\cdot)\) has all the properties of autocovariance function plus \(\rho(0)=1\).
 For i.i.d. noise with finite variance, the sample autocorrelations \(\hat{\rho}(h)\), \(h>0\), are approximately \(N(0,1/n)\) for large sample size \(n\). Hence, approximately 95% of the sample autocorrelations should fall between the bounds \(\pm1.96/\sqrt{n}\) (1.96 is the 0.975th quantile of the standard normal distribution) – this is the bound automatically drawn by the R function
acf()
. Autocorrelations that reach outside this bound are then statistically significant. Note that in R as a rule of thumb the default maximal lag is \(10 \log_{10}(n)\), and the same \(n\) is used for the confidence bounds at all lags (however, in reality, samples of different sizes are used for each lag).
Ljung–Box test
Instead of testing autocorrelation at each lag, we can apply an overall test by Ljung and Box (1978):
\(H_0\): \(\rho(1) = \rho(2) = \dots = \rho(h) = 0\)
\(H_1\): \(\rho(j) \neq 0\) for some \(j \in \{1, 2, \dots, h\}\), where \(n > h\).
The Ljung–Box test statistic is given by \[
Q_h = n(n + 2) \sum_{j = 1}^h\frac{\hat{\rho}_j^2}{n  j}.
\] Under the null hypothesis, \(Q_h\) has a \(\chi^2\) distribution with \(h\) degrees of freedom. In R, this test is implemented in the function Box.test()
with the argument type = "LjungBox"
and in the function tsdiag()
.
ACF measures the correlation between \(X_t\) and \(X_{t+h}\). The correlation can be due to a direct connection or through the intermediate steps \(X_{t+1}, X_{t+2}, \dots, X_{t+h1}\). Partial ACF looks at the correlation between \(X_t\) and \(X_{t+h}\) once the effect of intermediate steps is removed.
2.7 Partial autocorrelation function
Shumway and Stoffer (2011) and Shumway and Stoffer (2014) provide the following explanation of the concept.
Recall that if \(X\), \(Y\), and \(Z\) are random variables, then the partial correlation between \(X\) and \(Y\) given \(Z\) is obtained by regressing \(X\) on \(Z\) to obtain \(\hat{X}\), regressing \(Y\) on \(Z\) to obtain \(\hat{Y}\), and then calculating \[ \rho_{XYZ} = \mathrm{cor}(X  \hat{X}, Y  \hat{Y}). \] The idea is that \(\rho_{XYZ}\) measures the correlation between \(X\) and \(Y\) with the linear effect of \(Z\) removed (or partialled out). If the variables are multivariate normal, then this definition coincides with \(\rho_{XYZ} = \mathrm{cor}(X,Y  Z)\).
The partial autocorrelation function (PACF) of a stationary process, \(X_t\), denoted \(\rho_{hh}\), for \(h = 1,2,\dots\), is \[ \rho_{11} = \mathrm{cor}(X_t, X_{t+1}) = \rho(1) \] and \[ \rho_{hh} = \mathrm{cor}(X_t  \hat{X}_t, X_{t+h}  \hat{X}_{t+h}), \; h\geqslant 2. \]
Both \((X_t  \hat{X}_t)\) and \((X_{t+h}  \hat{X}_{t+h})\) are uncorrelated with \(\{ X_{t+1}, \dots, X_{t+h1}\}\). The PACF, \(\rho_{hh}\), is the correlation between \(X_{t+h}\) and \(X_t\) with the linear dependence of everything between them (intermediate lags), namely \(\{ X_{t+1}, \dots, X_{t+h1}\}\), on each, removed.
In other notations, the PACF for the lag \(h\) and predictions \(P\) is \[ \rho_{hh} = \begin{cases} 1 & \text{if } h = 0 \\ \mathrm{cor}(X_t, X_{t+1}) = \rho(1) & \text{if } h = 1 \\ \mathrm{cor}(X_t  P(X_t  X_{t+1}, \dots, X_{t+h1}), \\ \quad\;\; X_{t+1}  P(X_{t+h}  X_{t+1}, \dots, X_{t+h1})) & \text{if } h > 1. \end{cases} \]
To obtain sample estimates of PACF in R, use pacf(X)
or acf(X, type = "partial")
.
Correlation and partial correlation coefficients measure the strength and direction of the relationship, changing within \([1, 1]\). The percent of explained variance for the case of two variables is measured by squared correlation (rsquared; \(R^2\); coefficient of determination) changing within \([0, 1]\), so a correlation of 0.2 means only 4% of variance explained by the simple linear relationship (regression). To report a partial correlation, for example, of 0.2 at lag 3, one could say something like ‘The partial autocorrelation at lag 3 (after removing the influence of the intermediate lags 1 and 2) is 0.2’ (depending on the application, the correlation of 0.2 can be considered weak or moderate strength) or ‘After accounting for autocorrelation at intermediate lags 1 and 2, the linear relationship at lag 3 can explain 4% of the remaining variability.’
The partial autocorrelation coefficients of i.i.d. time series are asymptotically distributed as \(N(0,1/n)\). Hence, for lags \(h > p\), where \(p\) is the optimal or true order of the partial autocorrelation, \(\rho_{hh} < 1.96/\sqrt{n}\) (assuming the confidence level 95%). This suggests using as a preliminary estimator of the order \(p\) the smallest value \(m\) such that \(\rho_{hh} < 1.96/\sqrt{n}\) for \(h > m\).
2.8 Conclusion
We have defined components of the time series including trend, periodic component, and unexplained variability (errors, residuals). Our goal will be to model trends and periodicity, extract them from the time series, then extract as much information as possible from the remainder, so the ultimate residuals become white noise.
White noise is a sequence of uncorrelated random variables with zero mean and finite variance. White noise is also an example of a weakly stationary time series. The i.i.d. noise is strictly stationary (all moments of the distribution stay identical through time), and i.i.d. noise with finite variance is also white noise.
Timeseries dependence can be quantified using a (partial) autocorrelation function. We defined (P)ACF for stationary series; R functions also assume stationarity of the time series when calculating ACF or PACF.
After developing several models for modeling and forecasting time series, we can compare them quantitatively in crossvalidation. For time series, it is typical to have the testing set (or a validation fold) to be after the training set. Models can be compared based on the accuracy of their point forecasts and interval forecasts.