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4.3 Time-Invariant Linear Filters 127<br />

of weight functions and to select the one that appears to strike a satisfactory balance<br />

between bias and variance.<br />

The option Spectrum>Smoothed Periodogram in the program ITSM allows<br />

the user to apply up to 50 successive discrete spectral average filters with weights<br />

W(j) 1/(2m + 1), j −m, −m + 1,...,m, to the periodogram. The value of m<br />

for each filter can be specified arbitrarily, and the weights of the filter corresponding<br />

to the combined effect (the convolution of the component filters) is displayed by<br />

the program. The program computes the corresponding discrete spectral average<br />

estimators f(λ),0≤ ˆ λ ≤ π.<br />

Example 4.2.2 The sunspot numbers, 1770–1869<br />

4.3 Time-Invariant Linear Filters<br />

Figure 4.9 displays a plot of (2π) −1 times the periodogram of the annual sunspot<br />

numbers (obtained by opening the project SUNSPOTS.TSM in ITSM and select-<br />

ing Spectrum>Periodogram). Figure 4.10 shows the result of applying the discrete<br />

spectral weights <br />

1 1 1<br />

, , (corresponding to m 1, W(j) 1/(2m+1), |j| ≤m). It<br />

3 3 3<br />

is obtained from ITSM by selecting Spectrum>Smoothed Periodogram, entering<br />

1 for the number of Daniell filters, 1 for the order m, and clicking on Apply. As<br />

expected, with such a small value of m, not much smoothing of the periodogram<br />

occurs. If we change the number of Daniell filters to 2 and set the order of the first<br />

filter to 1 and the order of the second filter to 2, we obtain a combined filter with a<br />

more dispersed set of weights, W(0) W(1) 3<br />

2<br />

1<br />

, W(2) , W(3) . Click-<br />

15 15 15<br />

ing on Apply will then give the smoother spectral estimate shown in Figure 4.11.<br />

When you are satisfied with the smoothed estimate click OK, and the dialog box will<br />

close. All three spectral density estimates show a well-defined peak at the frequency<br />

ω10 2π/10 radians per year, in keeping with the suggestion from the graph of the<br />

data itself that the sunspot series contains an approximate cycle with period around<br />

10 or 11 years.<br />

In Section 1.5 we saw the utility of time-invariant linear filters for smoothing the data,<br />

estimating the trend, eliminating the seasonal and/or trend components of the data,<br />

etc. A linear process is the output of a time-invariant linear filter (TLF) applied to a<br />

white noise input series. More generally, we say that the process {Yt} is the output of<br />

a linear filter C {ct,k,t,k 0 ± 1,...} applied to an input process {Xt} if<br />

∞<br />

Yt ct,kXk, t 0, ±1,.... (4.3.1)<br />

k−∞<br />

The filter is said to be time-invariant if the weights ct,t−k are independent of t, i.e., if<br />

ct,t−k ψk.

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