TABLE 3
CORRELATION COEFICIENT RANGES
classes HH-VVc HH-VVp HV-VHp
sugar beet "0.66 .56-.61 .38-.61
stubble «50—.71 «12—.60 ‚04-.18
wheat «27—.34 .18-.28 ‚07-.31
potato ‚51-.54 2437.57 «70—.78
Lower stability is noticeable for the cases when
the correlation coefficient is low. For example,
the anomalous value -118 degrees for HH-VVp
(stubble) occurs when the correlation is .12. The
greater variability of wheat coincides with low
correlations.
Special note has to be given to HV-VHp: for stubble
and wheat classes the correlation is low, in
contradiction to that is expected by the theory.
This result can be explained due to cross-talk and
the influence of noise in low backscatter regions,
as discussed in [5]. HV-VH phases differences for C
band were “103 degrees, which goes to zero when
calibration is done. No discrimination was observed
when using HV-VH. All other remaining correlations
were zero and no other phase information was
observed.
4. CONCLUSIONS
The overall conclusion is that the phase
information can be observed, that is, it is
possible to have well peaked phase differences but
only HH-VV phases can be discriminatory, and
independent from amplitude information. Amplitude
information seems to have influence on the level of
noise included in the phases statistics and so in
the phase information quality. These results
reinforce the importance of working with complex
data, and suggest that, even without calibration,
phases differences can be potentially used for
classification.
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