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Project Cyclops, A Design... - Department of Earth and Planetary ...

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asshownin AppendixD, if thenoisein successive<br />

samples isuncorrelated, theprobability thatthisaverage<br />

exceeds agiventhresholdvalue<strong>of</strong>y =YT is<br />

n-1<br />

poO, T) = e -YT _ yTkk! (35)<br />

k=O<br />

If both signal <strong>and</strong> noise are present, the probability<br />

that the same threshold is not exceeded is:<br />

n-!<br />

pl(yT) = n + Y) ln_l(2nx/"_)dy<br />

foYT (Y) 2 e -n(r<br />

(36)<br />

I i i T I I q<br />

a<br />

bJ<br />

o<br />

x<br />

LI3<br />

Figure 5-5. Probability that signal plus noise fails to<br />

exceed power P.<br />

Z<br />

Figure 5-5 shows pl(x) plotted against 10 log x for<br />

various values <strong>of</strong> r expressed in decibels. By noting the<br />

value <strong>of</strong> pl(x) for 10 log x = 4.053 dB <strong>and</strong> plotting this<br />

versus the corresponding value <strong>of</strong> r, we obtain the curve<br />

shown in Figure 5-6. We see that if the probability <strong>of</strong><br />

failing to exceed the threshold is to be 0.07865, then r,<br />

the input signal to noise ratio must be 6.06 (i.e., 7.83<br />

dB).<br />

Thus for a square law detector with short time<br />

averaging (r _ 1/B), the limiting range is<br />

IJ<br />

..3<br />

dr Pelf (0.165 - b.<br />

R = -- - (34)<br />

f I 1/2<br />

4 _B<br />

.01 I I I t I I<br />

3 4 5 6 7 B 9 I0<br />

_o log _<br />

where we have written 0.165 for (6.06) -n .<br />

The n-bbM Average. lfy = -- _ x i is the average <strong>of</strong><br />

n<br />

i=0<br />

n samples <strong>of</strong> the output <strong>of</strong> a square law detector, then,<br />

1<br />

n<br />

Figure 5-6. Probability <strong>of</strong> missing signal.<br />

The same graphical method can be used with these<br />

expressions that was illustrated with equations (31)<strong>and</strong><br />

(33) for the case n = 1. (This is the procedure used in<br />

45

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