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plot(f,magnitude),grid
xlabel('Frequency')
ylabel('Power')
title('Power Spectral Density Estimate')
Let us increase the noise level. The gaussian noise has now a standard devia-
tion of fi ve and zero mean.
randn('seed',0);
n = 5*randn(size(y));
yn = y + n;
[Pxx,f] = periodogram(yn,[],1024,1);
magnitude = abs(Pxx);
plot(f,magnitude), grid
xlabel('Frequency')
ylabel('Power')
title('Power Spectral Density Estimate')
This spectrum resembles a real data spectrum in the earth sciences. The
spectral peaks now sit on a signifi cant noise fl oor. The peak of the high-
est frequency even disappears in the noise. It cannot be distinguished from
maxima which are attributed to noise. Both spectra can be compared on the
same plot (Fig. 5.6):
[Pxx,f] = periodogram(y,[],1024,1);
magnitude = abs(Pxx);
Power Spectral
Density Estimate
Power Spectral
Density Estimate
1000
1000
f 1 =0.02
800
800
f 1 =0.02
600
600
f 2 =0.07
f 2 =0.07
f 3 =0.2 ?
Noise
floor
400
400
f 3 =0.2
200
200
0
0
0.1
0.3
0.4
0.5
0.5
0
0.2
0
0.1
0.2
0.3
0.4
Frequency
Frequency
a
b
Fig. 5.6 Comparison of the Welch power spectra of the a noise-free and b noisy synthetic
signal with the periods
τ 3 =5 ( f 3 =0.2). In particular, the
peak with the highest frequency disappears in the noise fl oor and cannot be distinguished
from peaks attributed to the gaussian noise.
τ 1 =50 ( f 1 =0.02),
τ 2 =15 ( f 2 §0.07) and
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