563489578934
Sec. 6–3 DC and RMS Values for Ergodic Random Processes 437 the ensemble average required for a true x ( f ) of Eq. (6–42). In evaluating T ( f ), the DFT is generally used to approximate X T ( f ). This brings the pitfalls of DFT analysis into play, as described in Sec. 2–8. It should be stressed that Eq. (6–73a) is an approximation or estimate of the PSD. This estimate is called a periodogram, because it was used historically to search for periodicities in data records that appear as delta functions in the PSD. [Delta functions are relatively easy to find in the PSD, and thus, the periodicities in x(t) are easily determined.] It is desirable that the estimate have an ensemble average that gives the true PSD. If this is the case, the estimator is said to be unbiased. We can easily check Eq. (6–73a) to see if it is unbiased. We have and, using Eq. (6–50a) for T finite, we obtain T (f) = c |X T(f)| 2 d T T (f) = cR x (t) a t T bd and then, referring to Table 2–2, sin pfT 2 T (f) = T x (f) * a (6–73b) pfT b Because T (f) Z x (f), the periodogram is a biased estimate. The bias is caused by the triangular window function ∂ (tT) that arises from the truncation of x(t) to a T-second interval. Using Sec. A–8, where a = pT, we see that lim T : q [ T (f)] = x (f), so that the periodogram becomes unbiased as T → q. Consequently, the periodogram is said to be asymptotically unbiased. In addition to being unbiased, it is desirable that an estimator be consistent. This means that the variance of the estimator should become small as T → q. In this regard, it can be shown that Eq. (6–73a) gives an inconsistent estimate of the PSD when x(t) is Gaussian [Bendat and Piersol, 1971]. Of course, window functions other than the triangle can be used to obtain different PSD estimators [Blackman and Tukey, 1958; Jenkins and Watts, 1968]. More modern techniques assume a mathematical model (i.e., form) for the autocorrelation function and estimate parameters for this model. The model is then checked to see if it is consistent with the data. Examples are the moving average (MA), autoregressive (AR), and autoregressive-moving average (ARMA) models [Kay, 1986; Kay and Marple, 1981; Marple, 1986; Scharf, 1991; Shanmugan and Breipohl, 1988]. Spectrum analyzers that use microprocessor-based circuits often utilize numerical techniques to evaluate the PSD. These instruments can evaluate the PSD only for relatively low-frequency waveforms, say, over the audio or ultrasonic frequency range, since real-time digital signal-processing circuits cannot be built to process signals at RF rates. 6–3 DC AND RMS VALUES FOR ERGODIC RANDOM PROCESSES In Chapter 2, the DC value, the RMS value, and the average power were defined in terms of time average operations. For ergodic processes, the time averages are equivalent to ensemble averages. Thus, the DC value, the RMS value, and the average power (which are all
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Sec. 6–3 DC and RMS Values for Ergodic Random Processes 437<br />
the ensemble average required for a true x ( f ) of Eq. (6–42). In evaluating T ( f ), the DFT is<br />
generally used to approximate X T ( f ). This brings the pitfalls of DFT analysis into play, as<br />
described in Sec. 2–8.<br />
It should be stressed that Eq. (6–73a) is an approximation or estimate of the PSD. This<br />
estimate is called a periodogram, because it was used historically to search for periodicities in<br />
data records that appear as delta functions in the PSD. [Delta functions are relatively easy to<br />
find in the PSD, and thus, the periodicities in x(t) are easily determined.] It is desirable that<br />
the estimate have an ensemble average that gives the true PSD. If this is the case, the estimator<br />
is said to be unbiased. We can easily check Eq. (6–73a) to see if it is unbiased. We have<br />
and, using Eq. (6–50a) for T finite, we obtain<br />
T (f) = c |X T(f)| 2<br />
d<br />
T<br />
T (f) = cR x (t) a t T bd<br />
and then, referring to Table 2–2,<br />
sin pfT<br />
2<br />
T (f) = T x (f) * a (6–73b)<br />
pfT b<br />
Because T (f) Z x (f), the periodogram is a biased estimate. The bias is caused by the<br />
triangular window function ∂ (tT) that arises from the truncation of x(t) to a T-second<br />
interval. Using Sec. A–8, where a = pT, we see that lim T : q [ T (f)] = x (f), so that the<br />
periodogram becomes unbiased as T → q. Consequently, the periodogram is said to be<br />
asymptotically unbiased.<br />
In addition to being unbiased, it is desirable that an estimator be consistent. This means<br />
that the variance of the estimator should become small as T → q. In this regard, it can be<br />
shown that Eq. (6–73a) gives an inconsistent estimate of the PSD when x(t) is Gaussian<br />
[Bendat and Piersol, 1971].<br />
Of course, window functions other than the triangle can be used to obtain different PSD<br />
estimators [Blackman and Tukey, 1958; Jenkins and Watts, 1968]. More modern techniques<br />
assume a mathematical model (i.e., form) for the autocorrelation function and estimate parameters<br />
for this model. The model is then checked to see if it is consistent with the data. Examples are the<br />
moving average (MA), autoregressive (AR), and autoregressive-moving average (ARMA) models<br />
[Kay, 1986; Kay and Marple, 1981; Marple, 1986; Scharf, 1991; Shanmugan and Breipohl, 1988].<br />
Spectrum analyzers that use microprocessor-based circuits often utilize numerical techniques<br />
to evaluate the PSD. These instruments can evaluate the PSD only for relatively<br />
low-frequency waveforms, say, over the audio or ultrasonic frequency range, since real-time<br />
digital signal-processing circuits cannot be built to process signals at RF rates.<br />
6–3 DC AND RMS VALUES FOR ERGODIC RANDOM PROCESSES<br />
In Chapter 2, the DC value, the RMS value, and the average power were defined in terms<br />
of time average operations. For ergodic processes, the time averages are equivalent to ensemble<br />
averages. Thus, the DC value, the RMS value, and the average power (which are all