next up previous print clean
Next: An example of the Up: SPECTRAL FLUCTUATIONS Previous: SPECTRAL FLUCTUATIONS

Paradox: large n vs. the ensemble average

Now for the paradox. Imagine $n \rightarrow \infty$ in Figure 8. Will we see the same limit as results from the ensemble average? Here are two contradictory points of view:

We will see that the first idea contains a false assumption. The autocorrelation does tend to an impulse, but the fuzz around the sides cannot be ignored--although the fuzz tends to zero amplitude, it also tends to infinite extent, and the product of zero with infinity here tends to have the same energy as the central impulse.

To examine this issue further, let us discover how these autocorrelations decrease to zero with n (the number of samples). Figure 9 shows the autocorrelation samples as a function of n in steps of n increasing by factors of four. Thus $\sqrt{n}$ increases by factors of two.

 
fluct
fluct
Figure 9
Autocorrelation as a function of number of data points. The random-noise-series (even) lengths are 60, 240, 960.


view

Each autocorrelation in the figure was normalized at zero lag. We see the sample variance for nonzero lags of the autocorrelation dropping off as $\sqrt{n}$.We also observe that the ratios between the values for the first nonzero lags and the value at lag zero roughly fit $1/\sqrt{n}$.Notice also that the fluctuations drop off with lag. The drop-off goes to zero at a lag equal to the sample length, because the number of terms in the autocorrelation diminishes to zero at that lag. A first impression is that the autocorrelation fits a triangular envelope. More careful inspection, however, shows that the triangle bulges upward at wide offsets, or large values of k (this is slightly clearer in Figure 8). Each of these observations has an analytic explanation found in PVI.


next up previous print clean
Next: An example of the Up: SPECTRAL FLUCTUATIONS Previous: SPECTRAL FLUCTUATIONS
Stanford Exploration Project
3/1/2001