a generalized soil-adjusted vegetation index
TRANSCRIPT
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A generalized soil-adjusted vegetation index
M.A. Gilabert *, J. González-Piqueras, F.J. Garcı́a-Haro, J. Meliá
Departament de Termodinà mica, Facultat de Fı́ sica, Universitat de Valè ncia, Dr. Moliner, 50, 46100-Burjassot, Valencia, Spain
Received 31 July 2001; received in revised form 27 March 2002; accepted 27 March 2002
Abstract
Operational monitoring of vegetative cover by remote sensing currently involves the utilisation of vegetation indices (VIs), most of them
being functions of the reflectance in red ( R) and near-infrared (NIR) spectral bands. A generalized soil-adjusted vegetation index (GESAVI),
theoretically based on a simple vegetation canopy model, is introduced. It is defined in terms of the soil line parameters ( A and B) as:GESAVI=(NIR BR A)/( R + Z ), where Z is related to the red reflectance at the cross point between the soil line and vegetation isolines. As Z is a soil adjustment coefficient, this new index can be considered as belonging to the SAVI family. In order to analyze the GESAVI
sensitivity to soil brightness and soil color, both high resolution reflectance data from two laboratory experiments and data obtained by
applying a radiosity model to simulate heterogeneous vegetation canopy scenes were used. VIs (including GESAVI, NDVI, PVI and SAVI
family indices) were computed and their correlation with LAI for the different soil backgrounds was analyzed. Results confirmed the lower
sensitivity of GESAVI to soil background in most of the cases, thus becoming a very efficient index. This good index performance results
from the fact that the isolines in the NIR- R plane are neither parallel to the soil line (as required by the PVI) nor convergent at the origin (as
required by the NDVI) but they converge somewhere between the origin and infinity in the region of negative values of both NIR and R. This
convergence point is not necessarily situated on the bisectrix, as required by other SAVI family indices.
D 2002 Published by Elsevier Science Inc.
1. Introduction
Vegetation indices (VIs) derived from satellite data are
one of the primary sources of information for operational
monitoring of the Earth’s vegetative cover. These VIs are
radiometric measures of the spatial and temporal patterns of
vegetation photosynthetic activity that are related to canopy
biophysical variables such as leaf area index (LAI), frac-
tional vegetation cover, biomass, etc. (Asrar, Kanemasu, &
Yoshida, 1985; Baret & Guyot, 1991; Gilabert, Gandı́a, &
Meliá, 1996; Richardson, Wiegand, Wajura, Dusek, &
Steiner, 1992). Most of them are called broadband VIs
because they are based on algebraic combinations of reflec-
tance in the red, R, and that in the near infrared, NIR, spectral
bands (Bannari, Morin, Bonn, & Huete, 1995; Baret, 1995;
Elvidge & Chen, 1995; LePrieur, Verstraete, & Pinty, 1994).
These algebraic combinations are designed to minimize the
effect of external influences such as solar irradiance changes
due to the atmospheric effect or variations in soil background
optical properties in the vegetation canopy spectral response.
The soil line concept is a key concept in understanding
the functionality of VIs. This is the linear relation between
the reflectances R and NIR that best fits the values measured
for bare soils with varying amount of moisture, roughness,
etc. The soil type is the main factor of variation of the soil
line, and hence a different soil line should be defined for
each soil type (Baret, Jacquemoud, & Hanocq, 1993).
However, a ‘‘global’’ soil line is often used when dealing
with large satellite scenes, being allowable in this case a
certain range of variation of the soil line parameters (i.e., the
coefficients in the linear relation between R and NIR).
Soil background is one source of variation that has
received much attention in recent years, and soil-adjusted
indices such as SAVI, TSAVI, and OSAVI have been
introduced to address this issue (see Table 1). These indices
attempt to minimize brightness-related soil effects by con-
sidering first-order soil vegetation interaction by means of a
soil-adjustment parameter ( L, X , and Y in the equations
shown in Table 1), which usually depends on the vegetation
amount and has to be empirically determined, although it
can also be measured or modeled (e.g., in MSAVI). In
particular, for the case of intermediate vegetation canopy
levels, their respective authors have suggested the values:
L = 0.5, X = 0.08, and Y = 0.16.
0034-4257/02/$ - see front matter D 2002 Published by Elsevier Science Inc.
PII: S 0 0 3 4 - 4 2 5 7 ( 0 2 ) 0 0 0 4 8 - 2
* Corresponding author. Tel.: +34-96-3983118; fax: +34-96-3983385.
E-mail address: [email protected] (M.A. Gilabert).
www.elsevier.com/locate/rse
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In this work we aim at designing a new VI from a simple
canopy model that accounts for the contribution of soil and
vegetation to R and NIR, offering new insights into theexisting soil-adjustment factor. To analyze the performance
of this index, we conducted three experiments and com-
pared background effects for a variety of broadband VIs. All
these indices, including the new one, have been evaluated in
terms of their ability to accurately estimate LAI in the
presence of diverse backgrounds.
2. Theoretical basis of the GESAVI
2.1. Vegetation isolines and the SAVI-family indices
As mentioned above, the reflectances R and NIR of
bare soils distribute along the line NIR soil = A + BR. Due to
the presence of green vegetation, the measured values of
NIR increase while those of R decrease. Then, their
representation in the NIR- R plane yield points in a region
located in the upper left part of the soil line. This region is
called reflectance triangle and delimits the domain of
variability of NIR and R of a given vegetation canopy.
As an example, Fig. 1 exhibits the total spectral measure-
ments obtained in a laboratory experiment from a vegeta-
tion canopy for different LAI values and over different soil
backgrounds (these measurements are discussed later).
Lines connecting points corresponding to a similar vege-
tation amount over different soils are called vegetation
isolines. In particular, the isoline corresponding to absence
of vegetation is the soil line. In general, the vegetation
isolines can be represented rather accurately by straight
lines, but these lines are neither parallel nor convergent at
the origin. They can converge somewhere between theorigin and infinity, in the region of negative values of both
NIR and R, which seems to be a consequence of the
multiple scattering of the NIR radiation inside the vegeta-
tion canopy. But it can also occur that the isolines may not
converge at all. However, they all intersect with soil line,
at different locations. The distance between a given point
in the NIR- R plane and the soil line (measured either as
Euclidean distance or angular difference) is related to the
amount of vegetation. The slopes and intercepts of the
vegetation isolines in the R-NIR plane are related to the
optical properties of the canopy medium.
A VI performs satisfactorily when it predicts vegetation
isolines in agreement with the observations. Early indices
such as RVI and NDVI, the most widely used by far, predict
isolines convergent in the origin of the NIR- R plane. Other
indices such as PVI, which is based on the Euclidean
distance to the soil line, predict parallel isolines. Most
indices of the SAVI family (SAVI, TSAVI, and OSAVI)
predict that isolines converge in a point situated on the
bisectrix of the domain of negative values of NIR and R.
MSAVI, however, modeled the adjustment factor, recogniz-
ing that the locations do vary. As mentioned before, the
experimentally observed vegetation isolines do not match
those predicted by traditional indices, and they seem to
converge in a point situated in the domain of negative valuesof NIR and R. This point is not necessarily situated on the
bisectrix. Anyway, isolines predicted by SAVI family indi-
ces seem to better reproduce the experimental behaviour of
vegetation isolines, and this is the reason of the better
performance of these last VIs.
Table 1
Vegetation indices analyzed in this work. The soil line is NIR soil = A + BR
Vegetation index Reference
RVI ¼ NIR R
Pearson & Miller,
1972
NDVI ¼ NIR R NIR þ R
Rouse, Haas, Schell,Deering, & Harlan,
1974
PVI ¼ NIR BR A ffiffiffiffiffiffiffiffiffiffiffiffiffiffi1 þ B2
p Richardson &Wiegand, 1977
SAVI ¼ NIR R NIR þ R þ L ð1 þ LÞ
Huete, 1988
TSAVI ¼ Bð NIR BR AÞ R þ Bð NIR AÞ þ X ð1 þ B2Þ
Baret & Guyot, 1991
MSAVI
¼2NIR þ 1
ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffið2NIR þ 1Þ2 8ð NIR RÞ
q 2
Qi, Chehbouni,
Huete, Kerr, &
Sorooshian, 1994
OSAVI ¼ NIR R NIR þ R þ Y
Rondeaux, Steven,
& Baret, 1996
Fig. 1. NIR reflectance versus red reflectance for the Quercus canopy, as
described in Section 3 (Experiment I). Different symbols are used for
different LAI values, which are also indicated in the graph. The straight line
corresponding to LAI = 0 (bare soils) is the soil line for this particular data
set. Similar isolines were found in the other experiments.
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2.2. Designing the GESAVI
A vegetation canopy scatters and transmits a significant
amount of NIR radiation towards the soil surface, irradiating
the soil underneath as well as in between individual plants.
A fraction of the NIR radiation incident on the soil, fraction
that is determined by the optical properties of the soilsurface, is reflected back towards the sensor and scattered
and transmitted by the canopy. By contrast, red light is
strongly absorbed by the uppermost leaf layers of the
canopy, and irradiance at the soil surface is limited to that
received direct ly from the sun and sky through canopy gaps
(Huete, 1988).
Since the variance of reflectance appears to be mainly
associated with the fractions of illuminated and viewed soil
and plant components, it is reasonable to assume that the
reflectances R and NIR of a vegetation canopy vary propor-
tionally to a soil parameter s and a vegetation parameter v .
Reflectance in the red region increases with s and decreases
with v , while the near-infrared reflectance increases propor-
tionally to both s and v . The reflectance NIR incorporates
also a nonlinear (interaction) term related to multiple scat-
tering. Thus, it can be written that
R ¼ a þ bs cv ð1aÞ
NIR ¼ d þ es þ fv þ gsv ð1bÞ
where a, b, c, d , e, f , and g are unknown constants. To reduce
the number of constants, the soil line NIR soil = A + BR can be
used as a reference. Since v = 0 for this line, elimination of
parameter s between Eqs. (1a) and (1b) yields
A ¼ d eab
ð2aÞ
B ¼ eb
ð2bÞ
The vegetation isolines (i.e., lines with constant v )
predicted by this model are given by
NIR ¼ A Vþ B V R; v constant ð3Þ
with
A V ¼ ðd þ fv Þ ðe þ gv Þða cv Þb
ð4aÞ
B V ¼ e þ gv b
ð4bÞ
These vegetation isolines are linear but not parallel to the
soil line (except for the trivial case g = 0) since B V p B.
They intercept the soil line at a cross point with a red
reflectance given by
Rcross ¼ A V A B V
B ¼ bf þ ec ag þ cgv
g
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interpretation: GESAVI is proportional to tan(h), which
adopts a similar value for all the points situated over the
same vegetation isoline (for example, 1 and 1 V), independ-
ently of soil background optical properties.
The isolines predicted by this index are neither parallel
(as the ones derived from PVI) nor convergent at the origin
(like NDVI or RVI). As shown in Eq. (5), the vegetationisolines intercept the soil line at different cross points
depending on the vegetation amount. This can also be
observed in Fig. 2. In general, Z decreases at increasing
the vegetation cover. However, in this paper variations in
Rcross are considered negligible for simplicity. This fact
allows us to consider that all the isolines are convergent
in a point, usually situated in the third quadrant, but not
necessarily on the bisectrix of the third quadrant, unlike the
SAVI. This hypothesis may be more limited for dense
canopies. Future refinements are being investigated to
parameterize Z as a function of the canopy condition.
3. Materials and methods
To analyze the sensitivity of GESAVI to soil brightness
and soil color, two high-resolution reflectance data sets (I
and II) from two laboratory experiments (Garcı́a-Haro,
Gilabert, & Meliá, 1996; González-Piqueras, 1998) and a
third data set (III), obtained by applying a radiosity model to
simulate heterogeneous vegetation canopy scenes (Garcı́a-
Haro, Gilabert, & Meliá, 1999), were used. VIs (including
GESAVI, RVI, NDVI, PVI, and other SAVI-family VIs)
were computed and their performance was investigated
based on their correlation with LAI in the presence of diverse soil backgrounds.
In Experiment I, a set of 21 plots was designed, consist-
ing of seven varying amounts of vegetation (Quercus ilex
rotundifolia) over three different soil backgrounds. Cano-
pies with different vegetation amounts (LAI compressed
between 0 and 2.4) were obtained by uniformly inserting
Quercus plants of about 25-cm height in finely spaced holes
distributed over boxes of dimensions 30 50 cm. Theoriginal soil background was mainly composed of red clay
conglomerate. Changing soil brightness effect was obtained
by covering the soil with two varying levels of coal (16 and
40 g m 2, respectively). Coal was proved to have a low
reflectance in all wavelengths and therefore it reduces the
soil brightness. Similarly, in Experiment II, different vege-
tation canopies of Pinus pinea with LAI between 0 and 2.14
were obtained over three soil backgrounds (phyllite, red
clay, and marl) with a clearly different spectral response. In
this case, a previous series of reflectance measurements was
carried out to better estimate the soil line. It consisted of
changing arbitrarily the moisture content of the three soils
considered in the Experiment II.
As mentioned before, in these two laboratory experi-
ments, the biophysical parameter selected to characterize the
vegetation canopies was the LAI. LAI measurements were
t aken by means of a LICOR-2000 LAI canopy analyzer
(Welles & Norman, 1991), which provides an indirect
procedure to estimate LAI based on the attenuation of the
diffuse hemispherical sky radiation in the ultraviolet region
through the canopy. The standard deviation of the data was
below 0.1 in all the cases.
Concerning the reflectance data, the mean and standarddeviation reflectance spectrum (from 400 to 2500 nm)
were obtained for each plot using a GER SIRIS spectror-
adiometer. Standard deviations were found to be less than
1% for wavelengths from 400 to 900 nm. Beyond 900 nm,
the standard deviations rose continuously due to random
instrumental noise. The reflectances for the red and near-
infrared bands for Landsat Thematic Mapper (TM3 and
TM4, respectively) were derived by convolving the high-
spectral-resolution data with the relative response cur ves
(Markham & Barker, 1985) for these two TM bands. Fig.
1 shows the data set corresponding to Experiment I.
Different symbols have been used to represent plots with
different LAI values, which has been indicated in the
graph.
In Experiment III, simulation modelling of canopy BRF
was applied to obtain different scenes with varying soil
background and vegetation architectural characteristics by
means of a radiosity model (Garcı́a-Haro et al., 1999)
developed for heterogeneous canopies. These canopies are
approximated by an arbitrary configuration of plants or
clumps of vegetation, placed on the ground surface in a
prescribed manner. Plants are treated as porous cylinders
formed by aggregations of layers of leaves. This model
explicitly computes the radiation leaving each individual
surface, taking into account multiple scattering processes between leaves and soil, and occlusion of neighbouring
plants. In the actual case, R and NIR reflectance scenes
corresponding to 2-m shrub canopies with varying LAI
values (from 0 to 2.35) over three different soil backgrounds
(phyllite, red clay, and marl) were generated.
In Experiments I and II, the maximum LAI value
corresponds to dense canopies with a 100% fractional cover,
whereas in Experiment III the maximum LAI value corre-
sponds to a canopy with a fractional cover about 50%. Thus,
the reflectance distribution for this last experiment does not
reach the upper side of the reflectance triangle, indicating
that at maximum LAI levels the canopy reflectance is still
seriously affected by soil optical properties (González-
Piqueras, 1998).
4. Results
In all cases, the soil line equation has been obtained (see
Table 2) in addition to its cross point with each vegetation
isoline. An average value of Z u Rcross was found for theExperiment III data set, which resulted to be very close to
0.35. This value translated into low GESAVI errors for a
range of canopy densities, primarily sparse and intermediate
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(González-Piqueras, 1998). The choice of parameter Z
appears to be critical in minimizing the soil background
effect. However, we considered an identical Z value for data
sets I and II, in order to test the reliability of GESAVI as
computed without empirical adjustment of Z to the specific
conditions of each particular experiment, thus enabling its
direct comparison with other general indices.
With R and NIR reflectance and the soil-adjustment
coefficient values ( L = 0.5, X = 0.08, Y = 0.16, Z = 0.35) all
the vegetation indices shown in Table 1 and the GESAVI
were calculated and next they were represented versus LAI.
As an example, Fig. 3 shows NDVI, SAVI, and GESAVI as
a function of the LAI, for the reflectance data obtained in thethree experiments. Each symbol corresponds to a different
soil background. The quantitative comparison of GESAVI
with other common indices (e.g., improved versions of
SAVI) is presented later.
It can be seen that, in the LAI interval considered, the
three vegetation indices increase with LAI, although the first
one shows a more pronounced exponential behaviour pre-
senting a plateau after a threshold value depending on the
reflectance data set. This saturating effect of NDVI has been
widely reported in the literature. The SAVI and the GESAVI
show a more linear variation with LAI. As shown, plots with
identical canopy cover present different NDVI values for the
three soil backgrounds. There seems to be a systematic
tendency to produce larger VI values for darker soils than
for lighter ones as demonstrated by Bausch (1993) anddiscussed by Garcı́a-Haro et al. (1996). On the contrary,
SAVI and GESAVI values seem to be less affected by soil-
brightness variations and, thus, VI values obtained for a
given canopy cover are rather the same, independently of
soil background. As expected (Huete, 1988), soil influences
are prevalent in partially vegetated canopies (in the actual
case, they are more significant in the range from LAI = 0.5
to LAI = 1.5). From an operational point of view, this
reveals a more efficiency of SAVI and GESAVI to normal-
Table 2
Soil line equation for each experiment
Experiment I NIR = 0.009+ 1.34 R (r 2 = 0.99)Experiment II NIR =0.010 +1.17 R (r 2 = 0.98)
Experiment III NIR = 0.011 + 1.16 R (r 2 = 0.99)
Fig. 3. NDVI, SAVI, and GESAVI values versus LAI obtained in the three experiments for the three soil backgrounds. Experiment I: Symbols (.), ( ), and (o)refer to plots with 0, 16, and 40 g m 2 coal cover, respectively. Experiments II and III: Symbols (.), ( ), and (o) refer to plots with phyllite, red clay, andmarl background, respectively.
Table 3
Value of the signal-to-noise ratio for all the vegetation indices considered
and for the three data sets (Experiments I, II, and III)
Vegetation index Experiment I Experiment II Experiment III
RVI 0.012 0.040 0.025
NDVI 0.013 0.040 0.029
PVI 0.016 0.100 0.040
SAVI 0.037 0.083 0.077TSAVI 0.025 0.111 0.048
MSAVI 0.023 0.067 0.083
OSAVI 0.027 0.125 0.050
GESAVI 0.045 0.200 0.071
Outstanding values appear in bold face.
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Fig. 4. Efficiency of the different VIs as measured by means of T (%) (see text) as a function of LAI for the three data sets.
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ize the soil effect and consequently, a major applicability in
areas presenting sparse vegetation and high lithological
variability. Although not shown for brevity improved ver-
sion of SAVI, such like OSAVI and MSAVI, showed a
similarly good behavior.
To establish a quantitative comparison among the effi-
ciency to normalize soil spectral contribution of all the VIsconsidered in the study, two parameters that take into
account the VI dispersion for each LAI level as due to soil
background and their global ranges of variation were
considered. They will both result to be independent of the
range of variation of each VI.
The first one was defined by Leprieur et al. (1994) based
on the concept of signal-to-noise ratio (S/N). They propose
that the ‘‘signal’’ of interest is given by the difference
between the average index value for the maximum LAI
canopy and the average index value for the minimum LAI
canopy. The measurement of ‘‘noise’’ is taken by the area
between the maximum and minimum curves (i.e., the
product of the range of variation of the index due to changes
in soil spectral properties by the interval of LAI for which
this range is valid). As we are interested in selecting an
index as sensitive as possible to vegetation amount but also
as insensitive as possible to the soil optical properties, the
signal-to-noise ratio should increase in proportion to VI
efficiency. The first criterion to evaluate the efficiency of a
VI is then based on
S ðVIÞ N ðVIÞ ¼
VIðLAImaxÞ VIðLAIminÞZ LAImaxLAImin ½
maxVI
ðLAI
Þ minVI
ðLAI
Þd
ðLAI
Þ ð8Þ
Results obtained for the three data sets considered in the
present study are shown in Table 3. The three best VIs for
each case appear in bold face.
It can be seen that, in all the cases, the new index
(GESAVI) presents one of the highest signal-to-noise ratios.
Some other indices such as SAVI and OSAVI also present
high values and, thus, can be considered as belonging to the
most efficient VI group. Traditional indices (RVI and
NDVI) present low values for the signal-to-noise ratio,
indicating their worse performance to retrieve biophysical
characteristics from the vegetation canopies independently
of the soil background.
Results confirmed the lower sensitivity of GESAVI to
soil background in most of the cases, thus becoming the
most efficient index. This good index performance results
from the fact that the isolines in the NIR- R plane are neither
parallel to the soil line (as required by the PVI) nor
convergent at the origin (as required by the NDVI) but they
converge somewhere between the origin and infinity where
the NIR and R negative values are located. This conver-
gence point is not necessarily situated on the bisectrix, as
required by the SAVI family indices.
The second criterion to evaluate the VIs is based on an
LAI dependent parameter (Gilabert et al., 1998), which is
defined as
T VIðLAIÞ ¼ rLAIr̄ 100 ð9Þ
where rLAI refers to the standard deviation for the VI valuescorresponding to given value of LAI and r
¯refers to the
standard deviation of the VI values taking into account the
whole range of variation of LAI. Conversely, this parameter
diminishes as the VI efficiency increases. By using this
procedure, we have obtained the T (%) values as a function
of the LAI for the three data sets of the work. Fig. 4 shows
the values obtained for the three experiments.
It is observed again that RVI and NDVI hardly normalize
soil effects, presenting the maximum T values for inter-
mediate canopies, where the contribution of soil background
is prevalent and multiple scattering effects are more pro-
nounced. For dense canopies (LAI maximum) all the
vegetation indices present the lowest T value since soil
contribution is then less important. As previously shown,
the GESAVI is the index that better normalizes the soil-
induced effects and presents, for the overall range of LAI,
the lowest values for T .
In general, taking into account the data from the three
experiments, it can be observed that the new generation of
indices (SAVI family indices) present a better performance
than the traditional ones. Although the OSAVI shows in
most of the cases a good performance, the new index
defined in this work (GESAVI) presents even a better
efficiency to normalize soil background effects.
5. Discussion
The vegetation index introduced in this work needs a
prior knowledge of the soil line parameters and the soil-
adjustment factor to be suitable for operational monitoring
of vegetation from remotely sensed data. Several studies
(Baret et al., 1993) have shown that a universal soil line
cannot be defined and, therefore, this straight line has to be
determined for each case. A remaining question to be solved
in further studies concerns the sensitivity of GESAVI to the
soil line determination. In fact, a poor knowledge of the soil
line would affect the detection of low amounts of vegeta-
tion.
On the other hand, regarding the soil-adjustment term, a
single value ( Z = 0.35) appears to be optimal to normalize
soil effects. The value of this coefficient was selected to
minimize the variation of canopy reflectance with soil
background for intermediate LAI levels. Nevertheless, its
determination is a crucial point in the performance of
GESAVI, and some more reflectance data sets would be
required to establish a general optimal value of Z . In this
context, different analysis conducted very recently on real
and simulated satellite data have indicated that Z = 0.35 is
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well suited for a range of canopy densities, even though this
value could be less appropriate for very dense canopies. The
variation of Z with LAI has not been still quantitatively
established to recommend the best correction term for
different LAI ranges of the vegetation canopies. However,
the more common situation in a remote sensing context
involves no prior knowledge of LAI. The limitations of GESAVI thus need to be analyzed over several vegetation
canopies. A further study concerning different vegetation
canopies and a wider range of densities would be needed to
ensure GESAVI applicability on a global basis. In that
context, some research is now being carried out to param-
eterize the soil adjustment coefficient Z in terms of infor-
mation contained in the image, to operationally calculate the
GESAVI from satellite.
Acknowledgements
This work was partially supported by the MEDALUS III
Project funded by the European Communities (ENV4-
CT95-0019) and by the CICYT (AMB97-1000-C02-02 and
REN2000-1507-C03-02 GLO).
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