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Barret et al).
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1al Infrared and
At one end of
ened to produce
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oduce estimates
r periods of one
d was designed
| a global scale.
Combined MW and IR algorithms using SSM/I radiometric data
were first oriented to monthly averages over wide areas ( Adler et
al., 1993) or to global products as it is for the Global Precipitation
Climatology Project (GPCP) (Huffman et al., 2001). At the other
end of time- scale there has been number of techniques developed
for very short period ‘near real-time’ estimation of rainfall at the
best spatial resolution possible from geostationary satellites (4-8
km data produced every 30 minutes). These techniques have been
tried for flash flood warnings, etc. Classification of various
techniques is according to number of channels, sampling and
number of predictors. Sampling includes spatial and temporal
dimensions. All the techniques are empirical in nature.
Depending on whether a technique is based on geostationary
satellite data or on polar orbiting satellite data, several important
parameters governing the amount of rainfall results from clouds
can be stated as follows:
- Bright clouds in the visible imagery and clouds with
cold tops in the IR imagery that are expanding in area
coverage produce more rainfall than those that are not
expanding.
- Decaying clouds produce little or no rainfall.
- Clouds with cold tops in the IR imagery produce more
rainfall than those with warmer tops.
- Clouds with cold tops that are becoming warmer
produce little or no rainfall.
- Merging of cumulonimbus clouds increases the rainfall
rate of merging clouds.
The principles of most of the current techniques for estimating
rainfall from the temperature of the cloud tops, are associated
with relating rainfall with cold clouds assuming that these are the
tops of active storms. The rate of vertical or horizontal growth of
clouds or their minimum temperature can give further information
on the type of cloud and its likelihood of producing rain.
Techniques incorporating such features are known as the ‘life
history’ methods.
2.2 Rainfall estimates from cold cloud statistics
2.2.1 General: The University of Reading, UK, developed this
method for using on operational basis. The basic methodology of
the cold cloud statistics procedures is simple. A regular series of
thermal infrared (TIR) images of an area is received, pixels with
apparent temperatures lower than some predetermined threshold
are classified as “cold cloud’, and their characteristics
accumulated over some period. The resultant map is converted to
a rainfall estimate. The procedures adopted as a statistical model,
which is calibrated through comparisons between the cold cloud
characteristics and sets of conventional raingauge data. To
establish the utility of the method, it must subsequently be
validated, by comparing estimates from some area or period
distinct from that used for the calibration.
2.2.2 Space and time considerations: Space and time intervals
of satellite data are important factor to be considered besides
spatial resolution. Studies have shown that there is little
difference between the results obtained from using half-hourly or
hourly satellite data (Milford and Dugdale, 1989). However, if a
system is to be dedicated to rainfall estimation, there is no
disadvantage in acquiring and processing half-hourly data, must
be used for calibration and validation purposes because the spatial
variability of rainfall is high and we wish to compare a raingauge
IAPRS & SIS, Vol.34, Part 7, “Resource and Environmental Monitoring”, Hyderabad, India,2002
(point) measurement with the rainfall estimate for the
corresponding satellite pixel.
2.2.3 Calibration and validation: The objective is to select a
temperature threshold that will discriminate between clouds,
which are producing rainfall, and inactive clouds. This threshold,
which can be applied to convective cloud, is a function of the
dynamic and physical structure of the storm, which may vary
widely. Fortunately, over the tropics, these features are usually
related to the region and season. Having chosen a threshold there
is still no information on the rainfall distribution beneath an
individual cloud so one cannot make estimates of the
instantaneous rate of rainfall over a satellite pixel. Instead,
estimates must be aggregated over a period of time and/or a large
area to reduce the influence of the short period, small-scale
variability of rainfall. The minimum periods over which single
pixel rainfall estimates are useful are probably about 10 days.
However, if spatial as well as time aggregation is included daily
rainfall estimates can be made. This is the approach used for
catchment rainfall estimation. Calibrations may be achieved either
in terms of mm of rainfall over the catchment per hour of cold
cloud duration or, if a rainfall/stream flow model is to be used and
flow gauge measurements are available, it may be possible to use
the average clod top temperature as a direct input to the model as
a surrogate for rainfall. The regressions have to be made for the
average daily cloud top temperature to the observed daily rainfall.
These are very similar in terms of mm of rain per day and the
average cold cloud temperature. The validation can be made by
repeating the calibration procedure with an independent data set
for subsequent years/months. Another validation technique is to
monitor the performance of flow prediction models using satellite
rainfall estimates as inputs and to compare them to the
performance using the best available raingauge data. A major
problem in using raingauge data to calibrate or validate satellite
estimates of rainfall is the poor representative of area rainfall
given by raingauge data.
3.0 STUDY AREA
Godavari basin has been chosen as study area. Godavari river
rises near Nasik in Maharashtra at an elevation of 1067 m and
flows for a length of about 1465 km before outfalling into the Bay
of Bengal. The principal tributaries of the river are the Parvara,
the Purna, the Manjra, the Penganga, the Wardha, the Wainganga,
the Indravati and the Kolab. The catchment area of Godavari
basin is about 3,12,800 sq.km. The catchment area of the basin is
bounded on the west by the Western Ghats, on the east by the
Eastern Ghats and on the north by the Satmala hills. These hill
ranges play an important role in the distribution of the seasonal
rainfall in the basin (G Nageswara Rao). The seasonal rainfall is
very high over the hilly regions of the extreme west and in the
north and east. Immediately after crossing the Western Ghats, the
rainfall decreases rapidly and then starts increasing gradually
towards the east. The north- eastern parts of the basin also
receives heavy rainfall due to the passage of monsoon
disturbances from the Bay of Bengal in a northwesterly direction
across and to the north of the basin. It receives about 85% of its
annual rainfall during the monsoon season. There are about 32
raingauges in the basin for rainfall measurement.