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In order to apply our resolution enhancement method to SASS data, conditions must
be imposed on the data and various assumptions made. As an example of the
former, in order to estimate both
and
for the resolution elements, each
element must be observed with a diversity of incidence angles. Our assumptions in
applying this method to SASS data for this region are listed below.
- The instrument calibration remains stable over the data acquisition
interval. Limited tests of this assumption over the Amazon rainforest
have indicated the calibration stability to be adequate [4].
- Over the study regions, there is no dependence of
or
on
the azimuth angle of the measurement, i.e., there is no azimuthal modulation of
. The validity of this assumption for Amazon data is borne out by
previous investigators [6][1]. We plan further study of this
issue for this and other regions in later papers.
- The effects of surface topography are small and can be neglected. Surface
slope affects the local incidence angle which, in turn, may affect the estimates
of
and . However, , which describes the incidence angle dependence of
, is relatively small (globally,
dB/deg). Given
the small value of , the relatively flat topography of the Amazon basin,
and the relatively large size of the resolution elements, this assumption is
reasonable.
- The dependence of the time of day on
is small or known and
correctable. Previous researchers [4][1] have noted some
time-of-day variation in
over the Amazon region. In the early morning
hours
dropped approximately 0.5 dB, possibly due to the accumulation
of dew [4]. However, only a limited number of scatterometer
measurements were made during this time with most occurring later in the day.
Uncorrected diurnal variations is treated as ``noise'' in the imaging algorithm.
This variation appears to have very little impact on our results
and has, therefore, been ignored (see the discussion below). Further studies of
the diurnal variability are being conducted.
- The
and
parameters over the target region remain constant
over the imaging time interval. For a sufficiently short imaging time interval
this assumption is justified. However, in applying the method to SASS data, the
imaging time interval must be very long (days to weeks) to obtain sufficient
measurement overlap in order to achieve the desired resolution.
Kennett and Li [5] specifically examined the time dependency of
and
at
resolution in their search for extended
scatterometer calibration regions. During the 3 month SASS mission in the late
summer of 1978 they observed time-dependent changes in the
parameter in some
areas. However, over the extended Amazon basin, the only variation occurred
during the first 2-3 weeks of the mission and was limited to less than 1 dB
(compare Fig. 3). We have considered imaging time intervals which include and
exclude these first weeks. In this paper, the full data set was used. In a
later paper we will report on seasonal variations.
Assumptions 2, 4, and 5 may be relaxed when applying the method to suitably
modified future scatterometers [7].
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