Suppose that you have a noisy receiver of weak signals (e.g., a communications receiver). You are expecting
Question:
Suppose that you have a noisy receiver of weak signals (e.g., a communications receiver). You are expecting a signal s(t) with finite duration and known form to come in, beginning at a predetermined time t = 0, but you are not sure whether it is present. If it is present, then your receiver’s output will be
where y(t) is the receiver’s noise, a random process with spectral density Sy(f) and with zero mean, ȳ = 0. If it is absent, then Y(t) = y(t). A powerful way to find out whether the signal is present is by passing Y(t) through a filter with a carefully chosen kernel K(t). More specifically, compute the quantity
If K(t) is chosen optimally, then W will be maximally sensitive to the signal s(t) in the presence of the noise y(t). Correspondingly, if W is large, you infer that the signal was present; if it is small, you infer that the signal was either absent or so weak as not to be detectable. This exercise derives the form of the optimal filter, K(t) (i.e., the filter that will most effectively discern whether the signal is present). As tools in the derivation, we use the quantities S and N defined by
Note that S is the filtered signal, N is the filtered noise, and W = S + N. Since K(t) and s(t) are precisely defined functions, S is a number. But since y(t) is a random process, the value of N is not predictable, and instead is given by some probability distributionp1(N).We shall also need the Fourier transform K̃(f) of the kernel K(t).
(a) In the measurement being done one is not filtering a function of time to get a new function of time; rather, one is just computing a number, W = S + N. Nevertheless, as an aid in deriving the optimal filter it is helpful to consider the time-dependent output of the filter that results when noise y(t) is fed continuously into it:
Show that this random process has a mean squared value
Explain why this quantity is equal to the average of the number N2 computed using (6.60c) in an ensemble of many experiments:
(b) Show that of all choices of the kernel K(t), the one that will give the largest value of
is Norbert Wiener’s (1949) optimal filter, whose kernel has the Fourier transform
where s̃(f ) is the Fourier transform of the signal s(t), and Sy(f ) is the spectral density of the noise. Note that when the noise is white, so Sy(f ) is independent off , this optimal kernel is just K(t) = const × s(t) (i.e., one should simply multiply the known signal form into the receiver’s output and integrate). By contrast, when the noise is not white, the optimal kernel (6.62a) is a distortion of const × s(t) in which frequency components at which the noise is large are suppressed, while frequency components at which the noise is small are enhanced.
(c) Show that when the optimal kernel (6.62a) is used, the square of the signal-to noise ratio is
(d) As an example, suppose the signal consists of n cycles of some complicated wave form with frequencies spread out over the range fo/2 to 2fo with amplitude ∼ A for its entire duration. Also suppose that Sy is approximately constant (near white noise) over this frequency band. Show that
so the amplitude signal to noise increases linearly with the number of cycles in the signal.
(e) Suppose (as an idealization of searches for gravitational waves in noisy LIGO data) that
(i) We do not know the signal s(t) in advance, but we do know that it is from a set of N distinct signals, all of which have frequency content concentrated around some fo;
(ii) We do not know when the signal will arrive, but we search for it for a long time τs (say, a year);
(iii) The noise superposed on the signal is Gaussian. Show that, in order to have 99% confidence that any signal found is real, it must have amplitude signal-to-noise ratio of
where
This is so small because the Gaussian probability distribution falls off so rapidly. If the noise is non-Gaussian, then the minimum detectable signal will be larger than this, possibly much larger.
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Modern Classical Physics Optics Fluids Plasmas Elasticity Relativity And Statistical Physics
ISBN: 9780691159027
1st Edition
Authors: Kip S. Thorne, Roger D. Blandford