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SMOS L2 algorithm over forests: Description and generation of global maps
Rachid Rahmoune, Paolo Ferrazzoli
Tor Vergata University, DICII, Via del Politecnico 1, Roma, Italy
Yann Kerr, Philippe Richaume
CESBIO, Avenue. Edouard Belin 18, Toulouse, France
Corresponding author:
Rachid Rahmoune
Tor Vergata University, DICII,
Via del Politecnico, 1
Rome, Italy
Tel. +39 06 72597425
Fax +39 06 72597460
E-mail: [email protected]
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SMOS L2 algorithm over forests: Description and generation of global maps
Rachid Rahmoune, Paolo Ferrazzoli
Tor Vergata University, DISP, Via del Politecnico 1, Roma, Italy
Y. Kerr, P. Richaume
CESBIO, Avenue. Edouard Belin 18, Toulouse, France
Abstract This paper shows global maps of optical depth and soil moisture over land, obtained using the SMOS Level 2
algorithm. The focus is on forested areas, where the approach adopted to develop the algorithm can be subdivided into
different steps. First a theoretical model, which was previously developed and tested using ground based and airborne
measurements, generated parametric outputs. By fitting this output data set, the albedo and the optical depth of a simple
first order radiative transfer model were estimated. Then, this simplified forest model was included in the general Level
2 algorithm described in the Algorithm Theroretical Baseline Document (ATBD). The paper describes the details of this
procedure and shows some retrieval results. First, the algorithm was run with three free parameters: Soil moisture,
optical depth, and albedo. The retrieved albedo resulted to be close to the initial estimate (0.08) for Boreal forests, while
it was lower for Tropical forests. Running again the algorithm with the albedo fixed, a global map of optical depth was
generated. The spatial features of the map follow the global information about forest biomass available in the literature.
Finally it was found that, on average, the influence of seasonal effects on optical depth is moderate.
Keywords: Microwave radiometry, Forests, Optical depth
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I INTRODUCTION
Over land, the Soil Moisture and Ocean Salinity (SMOS) mission has the objective to retrieve soil moisture over several
kinds of land cover, including low vegetation and forests [1]. Developing a reliable forward model and a valid retrieval
algorithm for forests is important for several reasons. First of all, forest cover dominates several SMOS pixels.
Moreover there are mixed pixels, and even when other land covers (e.g. agricultural fields, grass) are dominant, a
correct characterization of forest emission improves the retrieval accuracy [2].
It is well established that soil moisture retrieval is difficult under forest cover [3]-[5]. In fact the attenuation related to
the high wood biomass reduces the contribution of the soil surface to the overall emission, thus reducing the sensitivity
to variations of soil moisture. A further reduction of sensitivity is associated to litter cover [3], [5]-[6]. At C band and
higher frequencies, crown attenuation makes soil moisture retrieval very difficult in most of cases. At L band some
sensitivity to soil moisture is expected, since crown attenuation is lower than at the higher frequencies, but establishing
quantitative models is not simple. While for low vegetation the optical depth can be simply related to biomass with a
reasonable accuracy [7], the same relationship cannot be easily extended to arboreous biomass, which is characterized
by different dielectric and geometrical properties.
Important ground-based and airborne experiments have been undertaken, providing an insight into this problem.
Multitemporal measurements of brightness temperature were carried out over coniferous and broadleaf forests using L
band radiometers mounted on a tower [3]-[5], [8]-[11], and were accompanied by detailed measurements of ground
variables, such as soil moisture, wood biomass, and forest geometrical properties. In some cases, outputs were used to
test theoretical models [5], [11], or fit the parameters of semi-empirical models [8], [10]. Upward looking radiometric
data were also collected in some forests [8], [10]. Moreover, airborne campaigns have provided useful data for
investigating the relationship between emissivity and forest biomass [12]-[14], and soil conditions [15]. Although these
efforts are very important, they are not yet sufficient to reach a complete understanding of the forest emission problem,
and to draw conclusive considerations. While some studies indicate the radiometric sensitivity to variations of soil
moisture to be poor in developed forests [3]-[5], others over moderately dense forests with thin litter show the
sensitivity to be appreciable [9]-[10], [15], although still lower than over low vegetation. Moreover, further efforts are
required to establish if the sensitivity to soil moisture is mostly reduced by crown attenuation or by litter cover. In
summary, modelling forest attenuation is an important issue which requires further research.
This paper investigates the problem using SMOS data and the L2 algorithm, which is described in the Algorithm
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Theroretical Baseline Document (ATBD) [16], [17]. The algorithm is based on two main components. The first consists
of a forward model, which estimates the brightness temperature emitted by land nodes of SMOS using a priori
information (auxiliary data) about land cover, surface temperature, Leaf Area Index (LAI), etc., and initial estimates of
soil moisture taken by the data base of the European Centre for Medium-Range Weather Forecasts (ECMWF). The
second consists of an inversion process, which estimates the actual soil moisture and optical depth by using
multiangular measurements, forward model outputs and a Cost Function [17]. For all SMOS nodes classified as soil
covered by vegetation, the brightness temperature is estimated by a simple first order radiative transfer model [7]. In
order to keep the algorithm consistent, and to consider the case of mixed pixels, the same approach is kept for both low
vegetation and forests [17]. For the case of forests, the radiative transfer parameters (optical depth) and (albedo) are
estimated using the synthetic outputs of the theoretical model described in [18], according to the procedure which was
further developed in [19]. The theoretical model was tested and revised using sets of ground based and airborne
measurements carried out over various forests in different environments [20]-[22].
This paper describes the procedure adopted to obtain the parameters of the simple first order model, which will be
named ATBD forest model. Then, global maps of variables retrieved by L2 algorithm will be shown. Initially, the
algorithm was run with three free variables to be retrieved: Soil Moisture (SM), vegetation optical depth (), and
vegetation albedo (). Histograms of retrieved will be shown, and compared against the first estimate of this variable
based on the theoretical model. Then, the algorithm was run keeping fixed the previously retrieved values, in order to
generate global maps of and SM. Finally, seasonal effects were evaluated by comparing maps of obtained in July and
November.
II. THE FORWARD MODEL
A. The basic theoretical model
As stated in the Introduction, the initial values of and for forests were estimated by fitting the outputs of a
theoretical model, which is based on the radiative transfer theory and adopts a discrete approach [18]. Trunks and
branches are represented as dielectric objects with the shape of cylinders, while leaves are represented as needles or
disks. The bistatic scattering cross sections and extinction cross sections are computed by using suitable
electromagnetic approximations [18]. The bistatic scattering coefficient of the soil is computed by using the Integral
Equation Model, in its bistatic version [23]. Single contributions are combined by using the matrix doubling algorithm,
which allows us to compute the overall bistatic scattering coefficient in all directions, including multiple scattering
effects. The overall reflectivity is finally computed by integration over the upper half space and the emissivity is
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obtained by the energy conservation law. Details about the electromagnetic model are given in [18].
For litter, the model published in [20], which considers the litter as a dielectric layer over the soil, was applied. At first,
air-litter and soil-litter interfaces are assumed to be flat. The layer is a mixture of air and dielectric material. The weight
of the dielectric material is the basic input, and can be related to the litter-fall by using relationships available in the
literature [24]. The litter moisture is related to soil moisture, using an empirical relationship based on field
measurements [3]. The permittivity of the dielectric material is computed as a function of moisture, and the permittivity
of the layer mixture is computed by means of the quadratic refractive model for mixtures [25]. The overall reflectivity
of this composite medium, made by soil and litter, is computed using a coherent multiple reflection model. Further
details about the procedure, which leads to computing the bistatic scattering coefficient of the ensemble litter/soil
included it in the general model are given in [20].
This theoretical forest model was previously tested against ground based and airborne measurements [20]-[22]. Rms
errors were in the range 2.5 K 4.0 K. The objective of this paper is not to make further direct tests of this theoretical
model, but to show how its outputs were used to compute the parameters of the simplified ATBD forest model [16]-
[17] and to estimate how the SMOS algorithm performs at large scale over forests.
B. Input variables and estimate of parameters
The procedure assumes to know, besides soil variables, the following inputs:
Leaf Area Index contributed by forest leaves LAIF
Leaf Area Index contributed by herbaceous vegetation LAIV
distribution of trunk diameters at breast height dbh [cm]: p(dbh)
moisture [g/g] and dry matter density D [g/cm3] of trunks, branches and leaves.
A general scheme of the procedure is given in Figure 1.
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Figure 1. General scheme of the modeling procedure.
For specific forest plots, the dbh distribution depends on the age and the type of trees. At the scale of SMOS pixels, the
differences are smoothed. A Gaussian distribution is assumed here, with an average value of 20 cm and a
standard deviation of 5 cm. A parametric study indicated that the selection of this parameter is not critical, provided the
woody biomass is lower than about 400 m3/ha, and the cases of very young forests (dbh =10 cm) are excluded [21]. For
the range of dbh values, a lower limit dbhmin equal the average minus three times the standard deviation, and an
upper limit dbhmax equal to plus three times the standard deviation is imposed. The input data set required by the
theoretical model is obtained according to the procedure outlined in Appendix A. A key variable is the actual maximum
yearly value of Leaf Area Index LAIFmax.
The theoretical model is used to predict the trends of emissivity (in full leaf development) as a function of LAIFmax.
Examples for the case of broadleaf forests are given in Figure 2. The case of no litter is also considered. As expected,
the dynamic range is reduced by increasing LAIFmax, while it is still significant for LAIFmax lower than about 3. The
effects of litter are low for dry soils, but become important for moist soils. Litter properties are also related to LAIFmax
using the relations described in Appendix A.
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Figure 2. Simulated trends of emissivity vs. soil moisture content (m3/m3) for broadleaf forests in full leaf development.
Polarization: vertical (left), and horizontal (right). Maximum yearly value of forest LAI: 1, 2, 3, 4. Continuous lines:
with litter. Dashed lines: without litter.
The simulation outputs are used to fit the equivalent parameters F (forest optical depth) and F (forest albedo),
contributed by arboreous vegetation and assumed to be independent of polarization, of the ATBD forest model [16],
[17]. The fitting procedure was subdivided into various steps. First, a height standard deviation of soil roughness equal
to 1.5 cm was selected. The roughness factor HR of the ATBD model was set by imposing the surface emissivity of the
ATBD model to be equal to the surface emissivity of the theoretical model. The theoretical model was run at both
polarizations for an angular range of 5-55 and a SMC range of 5%-30%. Then, the ATBD model was run for the same
conditions, and F and F were selected in order to yield the minimum rms difference between brightness temperature
(K) outputs of the two models. We verified that the obtained results are scarcely affected by the initial choice about
roughness, provided the same roughness is selected for the two models.
The trends of F and F as a function of LAIFmax , for the case of broadleaf forests, are shown in Figure 3. Values of F
lower than about 0.6 are achieved for sparse forests with LAIFmax
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Figure 3. Trends of fitted radiative transfer parameters F and F as a function of maximum yearly value of forest LAI,
for broadleaf forests.
Figure 4. Rms error in the estimate of F (albedo) as a function of maximum yearly value of forest LAI, for broadleaf
forests.
developed forests, the fitting of the albedo is less reliable, in that the emisivity is more influenced by soil properties.
A linear regression was then applied to the relationship between the optical depth and LAIFmax, in order to compute the
coefficients of a linear relationship such as:
F = bF LAIFmax (1)
The resulting coefficients are:
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bF = 0.29 for broadleaf forests.
bF = 0.36 for coniferous forests.
Equation (1) gives the maximum yearly value of F, which is achieved in full leaf development. If the forest is
deciduous, F decreases in late autumn and winter due to the absence of leaves. Further model simulations, not shown
here, indicated that the corresponding decrease of bF coefficient is 0.03 units. Therefore, a general expression is:
F = bF LAIFmax 0.03 ( LAIFmax - LAIF) (2)
The total optical depth, including contributions of both forest vegetation and herbaceous vegetation is given by:
= F + bV LAIV (3)
The bV coefficient is set equal to 0.06, which is the value adopted by the ATBD for low vegetation [17].
Then, we assumed:
LAIF = fF LAI
LAIV = fV LAI
LAI is the total Leaf Area Index, available by ECOCLIMAP data base [26].
fF and fF represented the fractions of LAI contributed by arboreous leaves and herbaceous vegetation, respectively.
Some data are available in the literature [27]-[29], showing some dispersion. In order to simplify the initial guess of
we made an assumption which was verified in some broadleaf and coniferous forests [28]-[29]: fF = 0.6, fV = 0.4
For the albedo, the value achieved fitting the outputs of the theoretical model (as described above) for the dense forests
(higher values of LAIFmax in Figure 3) is used:
F = 0.08
This value represented a good fit for both broadleaf and coniferous forests.
The roughness parameter HR [17] has been set equal to 0.3. This value corresponds to a height std. of about 1.0 cm,
which is quite realistic [30].
The procedure described in this Section leads to compute the optical depth and the albedo of the ATBD forest model.
The performance of this model against SMOS signatures will be estimated in the next Sections.
III THE L2 ALGORITHM
The SMOS SM L2 algorithm [17] is iterative. It estimates the soil moisture and the optical depth by minimizing the rms
difference (Cost Function) between the measured multiangular brightness temperatures (L1C data) and the forward
model simulations. In this process, the algorithm uses as initial values the soil moisture predicted by ECMWF and the
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optical depth predicted by the procedure illustrated in Section II.B
In this work, the algorithm was run for the SMOS data collected in the time intervals form July 1 to July 4, 2011, and
from November 1 to November 4, 2011. For each SMOS node [17], all the passes for which the retrieval was successful
were considered and the results were averaged.
A. Estimate of the albedo
Initially, the algorithm was run with three free parameters: Soil moisture, optical depth and albedo. The histograms of
retrieved albedo, computed using data collected from July 1, 2011 to July 4, 2011 and subdivided into main continental
regions, are reported in Figure 5. The value initially estimated by the forward model (=0.08) is reported for
comparison. For Boreal forests of North America and Europe/Asia, this value is close to the maximum of the
histograms. However, for tropical and Subtropical forests of South America and Polynesia the maximum of the
histograms is close to 0.06. Explaining in detail this difference is the subject of future work. At present time, it can be
stated that the forward model described in Section II and Appendix A is based on assumptions and allometric equations
mostly derived for Boreal forests [31]-[34]. Parametric investigations [21] showed that the emissivity simulated for the
higher biomass, which is directly related to , can be appreciably influenced by geometrical properties, such as
distribution of branch dimensions.
Figure 5. Histograms showing number of SMOS nodes with retrieved albedo equal to abscissa value. The dashed
vertical bar indicates the initial value (0.08) predicted by the theoretical model.
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B. Global maps of optical depth and soil moisture
Figure 6. Global map of retrieved optical depth.
Using again the data collected from July, 1, 2011 to July, 4, 2011, global maps of optical depth and soil moisture were
generated. In this running of the algorithm, was set equal to 0.08 for boreal forests and 0.06 for tropical and
subtropical forests, considering the results reported in Figure 5. The algorithm described in [17] was used for low
vegetation. The resulting map of optical depth is shown in Figure 6.
As expected, the optical depth in the areas covered by forests is higher than in low vegetation. In general, the map
shows a correspondence with forest biomass maps available in the literature [35]-[36]. More detailed quantitative
comparisons are in progress. values higher than 1.0 are obtained in large part of the dense and thick Amazon forest,
while a decrease is observed moving towards the subtropical Chaco forest, mostly covering Paraguay and Northern
Argentina, where the vegetation is less dense. A high optical depth is also observed in Polynesia. Moderate values,
typically in the range 0.7-0.9 are obtained in Boreal forests of Canada, US, and Siberia. The retrieval is unsuccessful in
the Congo forest, where the forest is dense and the quality of L1C data resulted to be poor. In many regions of Europe
and Asia, the retrieval was hampered by heavy RFI effects [37], as confirmed by the specific flag included in L1C data.
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Figure 7. Ratios between retrieved and initial values of optical depth for forest nodes.
The initial estimate of is based on the procedure depicted in Section II, which contains several approximations. The
iterative L2 algorithm starts from this initial estimate and uses SMOS L1C data in order to find the minimizing the
Cost Function for each node [17]. For forest nodes, a map of the ratio between retrieved and initial values is reported in
Figure 7. In general, the ratio is close to the unity over Amazonia, while is appreciably lower than 1 are in most of
Boreal forests, particularly in the case of Coniferous trees. These variations are partially due to approximations of the
model, but can be also attributed to inaccuracies of ECOCLIMAP data base.
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Figure 8. Global map of retrieved soil moisture.
The world map of retrieved soil moisture is reported in Figure 8. When the retrieved optical depth is moderate, as in
Canada and most of Siberia, SM is retrieved. When the optical depth is high, there are areas where the retrieval fails,
since the sensitivity to variations of SM can be too low with respect to the noise of L1C data.
This global map confirms some expected spatial trends, such as the decrease of SM from Atlantic to Pacific coast of
South America (for a latitude lower than about -20). Detailed ground truth of SM below forests are available in few
sites only. Multitemporal tests are in progress.
C. Seasonal effects
Figure 10. Map of differences between values retrieved in November and July, 2011, for North America.
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Figure 11. Histogram of differences between values retrieved in November and July, 2011, for North America.
Finally, seasonal effects were investigated. The retrieval of optical depth was made again using SMOS data averaged in
the time interval from November 1, 2011 to November 4, 2011, using previous assumptions about albedo. A map of the
differences between values obtained in November and July is reported in Figure 10 for the North American continent,
where large forests are present and seasonal effects are expected. Positive and negative changes are mixed in a complex
way, probably due to combined effects of leaf cycle and change of litter biomass. Of course, variations can be also due
to errors in the estimate. Histograms of variations is reported in Figure 11. The maximum is close to zero, which
confirms the previous considerations. Most of variations are in a range +/- 0.2, which is low with respect to optical
depth values of July (0.7-0.9). This result confirms that an important contribution to forest optical depth is constant with
time, since is due to branches, in agreement with previous experimental results [9]-[10], and model simulations [21].
V. CONCLUSIONS
The forward model used for forests in the SMOS L2 algorithm has been described. The coefficients were obtained by
fitting the outputs of a theoretical model.
The retrieval algorithm was run to estimate the forest albedo and to generate global maps of retrieved optical depth and
soil moisture. The retrieved albedo is close to the initial estimate for Boreal forests, while is lower for Tropical and
Subtropical forests. Explaining this result is the subject of future investigations.
The global map of optical depth follows the spatial trends expected on the basis of available information about forest
biomass. The SM map follows some expected spatial patterns, although more in depth quantitative investigations are
needed.
Seasonal effects on forest optical depth are moderate. This variable shows positive and negative variations from July to
November, but a general tendency is not observed.
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APPENDIX A
THE INPUT DATA SET
Let the minimum and maximum values of diameter at breast height dbh be defined as dbhmin and dbhmax, respectively.
The dbhmax-dbhmin range is subdivided into MT intervals, of width given by:
dbh=dbh maxdbhmin
M T (A1)
For the i-th interval, the number NTi of trees per unit area [ha-1] with dbh value within the interval is given by:
dbh+dbh
d(dbh)p(dbh)N=Ni
idbhTTi (A2)
NT is the tree density [ha-1], and dbhi is the value of dbh at the lower limit of the interval.
Using allometric equations [31], the total dry biomass and its subdivision into trunk, branch and leaf fractions, can be
related to the diameter at breast height (dbh). For each interval i, the tree dry biomass DBi (kg) is estimated by means of
the allometric equation [31]:
)](dbhb+[b=DB i1i lnexp 0 (A3)
b0 and b1 are coefficients depending on tree species.
For broadleaf forests, average coefficients are:
b0 = - 2.48
b1 = 2.483
For coniferous forests, average coefficients are:
b0 = - 2.54
b1 = 2.481
Other allometric equations [31] give the biomass components (kg) contained in trunks (DBti ), leaves (DBli ), and
branches (DBbi ).
For trunks:
)dbha+(aDB=DB
i
t1t0iti exp (A4)
For broadleaf forests:
at0 = - 0.30
at1 = - 5.42
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For coniferous forests:
at0 = - 0.37
at1 = - 1.8
For leaves:
)dbha+(aDB=DB
i
l1l0ili exp (A5)
For broadleaf forests:
al0 = - 4.08
al1 = 5.88
For coniferous forests:
al0 = - 2.96
al1 = 4.47
For branches:
DBbi =DB iDB tiDB li (A6)
The maximum yearly value of leaf dry biomass per unit area DBL (t/ha) can be derived as a function of the maximum
yearly value of arboreous Leaf Area Index LAIFmax by means of empirical formulas.
For broadleaf forests, we have adopted the formula given in [30]:
DBL=LAI Fmax
1 .72 (A7)
For coniferous forests, the coefficient has been estimated by fitting the data made available by [24]:
DBL=LAI Fmax
0 .43 (A8)
The tree density NT can be obtained by using (A2) and by imposing:
dbh+dbh
d(dbh)p(dbh)DBN=DBN=DBLi
idbh
N
=iliT
N
=iliTi
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0.0010.001 (A9)
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The required variables for trunks, branches, leaves, and litter can be computed as indicated below.
1) Trunks
Trunks are modelled as equivalent cylinders. For the i-th interval of dbh values, the cylinder diameter is assumed to be
equal to dbhi. The dry biomass DBti (kg) is computed by (A3) and (A4), and converted into woody volume WVti (m3),
according to the procedure described in Appendix A. The height of the cylinders is given by:
22/0.01 )dbh(WV
=Hi
titi
(A10)
Since there is a trunk per tree, the number of trees with diameter equal to dbhi is given by equation (A3). Trunks are
assumed to be vertical.
2) Branches
Branches are subdivided into sections, and sections are modelled as cylinders. For the i-th interval of dbh values, the
branch dry biomass DBbi can be computed by (A3)-(A6) and converted into woody volume WVbi. Branches are
subdivided into primary and secondary branches. The latter are assumed to contain 30% of the overall branch volume,
according to the estimate given by [33].
For primary branches belonging to a tree with dbh equal to dbhi, the maximum diameter db_maxi has been related to dbhi..
For coniferous forests, the relationship made available by [34] has been used. For broadleaf forests, the maximum
diameter db_maxi has been assumed to be equal to 0.25 dbhi. This coefficient, which was aleady adopted in [21], agrees
with available photos of some broadleaf forests. The branch diameters are assumed to follow a Gaussian pbi distribution,
centered at db_maxi/2. The range between 0 and db_maxi is subdivided into Mbi intervals of width d. For the j-th interval, dj
is the central value, and pbij gives the fraction of total branch volume filled by branches with diameter internal to the
interval. This assumption is in general agreement with the measured data reported by [33], although they were fitted by
different functions. The length of the cylinder is equal to 50 dj, with an upper limit at 25 cm [33].
Also for secondary branches the distribution of filled volumes pbsi is assumed to be Gaussian. The average diameter is
equal to 0.6 cm and the length is computed similarly to the case of primary branches.
Finally, the total number of cylinders with diameter dj is given by:
)p+(pN=N bsijbijTM
=iTibj
1 (A11)
This distribution is used by the electromagnetic model as input. Both primary and secondary branches are assumed to
be randomly oriented.
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3) Leaves
Broad leaves are described as circular disks with a radius of 2 cm and a thickness of 0.02 cm. Coniferous leaves are
decribed as needles with a height of 10 cm and a diameter of 2 mm. The number of elements is obtained as the ratio
between LAIF and element area. Elements are randomly oriented.
4) Litter
For litter, the dry biomass DBLI (kg/m2) is related to litter-fall. Typically, 2 years of litter-fall are considered. By fitting
data of broadleaf forests provided by [24] we have assumed:
DBLI=1.25 DBL for broadleaf forests
DBLI=0.25 DBL for coniferous forests
DBL is the maximum yearly value of dry leaf biomass, and can be computed by (A7), (A8).
The litter thickness is related to the litter biomass using the formula given in [38].
ACKNOWLEDGMENTS
This work was partially supported by ESA, European Space Agency, under Contracts 21527/08/I-LG and
4000101152/LO/I-AM
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