Digital Signal Processing Reference
In-Depth Information
TABLE 5.1: RMSEs of the Magnitude Estimates Obtained via the
WFFT, GAPES, and MAPES-EM Spectral Estimators
WFF T
GAPES
MAPES-EM1
MAPES-EM2
Signal 1
0.420
0.175
0.010
0.011
Signal 2
0.417
0.205
0.010
0.010
Signal 3
0.419
0.169
0.010
0.009
Signal 4
0.205
0.164
0.009
0.011
Next, we increase the number of missing samples to 77 (60% of the original
data). The results of WFFT, WFFT GAPES, MAPES-EM 1, and MAPES-
EM2are shown in Figs. 5.5(a)-5.5(d), respectively. The signal amplitudes in the
WFFT spectrum are low presumably due to the small (40%) amount of avail-
able data samples. The artifacts are so high that we can hardly identify the signal
components. GAPES also performs poorly [see Fig. 5.5(b)], as expected. The
MAPES-EM algorithms provide excellent spectral estimates with relatively minor
artifacts.
In our next experiment, we keep the 40% data missing rate but increase the
noise variance to
2
n
σ
=
0
.
1 (10 dB higher than in the previous experiments). The
TABLE 5.2: RMSEs of the Phase (Radian) Estimates Obtained via the
WFFT, GAPES, and MAPES-EM Spectral Estimators
WFF T
GAPES
MAPES-EM1
MAPES-EM2
Signal 1
0.077
0.042
0.021
0.021
Signal 2
0.059
0.038
0.024
0.025
Signal 3
0.099
0.037
0.012
0.013
Signal 4
0.133
0.029
0.022
0.022
Search WWH ::




Custom Search