r
s,g
/r
s
r
( 7)
and
J r
s.ir s,r
( 8)
If we assume that we are able to determine the
constants Cj and , merely by measuring the required
reflectance values at the same soil moisture content,
then equations (2), (3), (6), (7) and (8) offer us
five equations with five unknown variables: the
corrected infrared reflectance (r! ), soil cover (B)
and the soil reflectance in the tliree bands (r ,
r and r . ). After solving these equations 3 ' g for
till 1 correcl4^ r infrared reflectance we obtain:
r !
ir
r.
ir
. r
v,r
r
r
r
V, r
r
v,g
. r
y,g
)
( 9)
In the situation of bare soil only, r , r and r.
, , g r ir
equal r Si g f r S/r and r s ^ r , respectively, and equation
(9) results in: r£ r =0. In the situation of complete
soil cover, rg and r r equal r Vj g and r V/r , respecti
vely, and equation (9) results in: r 1 = r ; in
. 13T 1IT
other words no correction for soil background is
applied if the soil is not visible.
In order to deduce the relationship between soil
cover and LAI, the process of extinction of radiation
in a canopy should be considered. If a canopy has a
certain extinction coefficient per leaf layer as well
as a certain LAI (abbreviated as L in the formulae),
the product of both factors equals the mean extinction
of that canopy. The mean extinction consists of two
components:
1. extinction in the direction of the sensor, indica
ted by K.L, where K is the extinction coefficient
per leaf layer in the sensor direction;
2. extinction in the direction of the sun, indicated
by k.L, where k is the extinction coefficient per
leaf layer in the direction of the sun.
Consider the process of extinction in a very small
part (or element) of the canopy. In the visible
spectral bands, extinction in an element occurs when
a leaf is hit by radiation. The probability of hitting
i elements among n independent elements has a binomial
distribution. If the number n of independent elements
increases to infinity while the probability of hitting
a specific element decreases to zero, the binomial
distribution can be approximated by a Poisson distri
bution. The Poisson distribution states:
P(x=i) = e X . X 1 i = 0,1,2,3,... d°)
i;
The random variable x is the number of independent
elements of the canopy in which extinction occurs; X
is the mean or expected number of elements in which
extinction occurs. The probability that no element is
hit (i=0) equals:
P(x=0) = e (11)
The probability of soil being visible in the direction
of the sensor equals: e~ K * L .
The probability of soil being illuminated by the sun
equals: e~k.L.
If one assumes both events to be independent, the
probability of sensing illuminated soil equals:
e-K.L * e - k - L = e-< K+k > - L
The complementary probability is equal to the appa
rent soil cover (new definition). This means that
soil cover may be described as:
B
. -(K+k).L
1 - e
(12)
Inserting equation (12) into (5) gives:
r '
r
V
(1
-(K+k).L
e )
(13)
The relationship between LAI and infrared reflec
tance (cf. Bunnik, 1978) greatly resembles a
"Mitscherlich curve" (y=A-b.exp(-k.t)). In the
special situation of such a curve running through the
origin (A = b) , the curve defined by y=A. (1-exp(-k.t) )
has only two parameters. For describing the relation
ship between the corrected infrared reflectance and
LAI (which runs through the origin) an empirical
equation similar to equation (13) could be used:
r !
ir
(1
-O.L
(14)
parameter r«, being the asymptotic value for the
infrared reflectance and a a combination of extinction
and scattering coefficients. Both parameters are
estimated empirically from a training set. Finally the
LAI is solved from equation (14):
L = -l/a . ln(l - r i r / r 00>ir ) (15)
This is the inverse of the special case of the
Mitscherlich function.
4 COMPARING THE MODEL WITH THE SAIL MODEL
In this section the model derivations presented earlier
will be verified by means of calculations with the
more complicated SAIL model (Verhoef, 1984) . This
model simulates reflectances as a function of plant
variables and measurement conditions (cf. section 2.2).
The following variables for the SAIL model have been
used:
- three soil types:
. dry soil (green reflectance = 20.0%, red reflec
tance = 22.0%, infrared reflectance = 24.2%);
. wet soil (green reflectance = 10.0%, red reflec
tance = 11.0%, infrared reflectance = 12.1%);
. black soil (green, red, infrared reflectance =
0%) .
- spherical leaf angle distribution.
- direct sunlight only (solar zenith angle: 45°).
- direction of observation was assumed to be vertically
downwards.
- reflectance and transmittance of a single leaf were
assumed to be equal: green reflectance = 8%, red
reflectance = 4% and infrared reflectance = 45%.
Model calculations were carried out using the follow
ing LAI values: 0 (0.1) 1.0 (0.2) 2.0 (0.5) 5.0 (1.0)
8.0.
The green, red and infrared reflectance factors were
calculated according to the SAIL model for each of the
above situations. The SAIL model was also able to
calculate the complement of the illuminated soil
detectable by the sensor (this equals soil cover with
the new definition introduced in this paper).
The results obtained with the SAIL model clearly
show that the relationship between soil cover, accor
ding to the new definition, and green or red
reflectance was nearly perfectly linear for a dry soil
(figure 3). Similar results were obtained for a wet
soil (Clevers, 1986b). These results support the
validity of equations (2) and (3) if the new definition
of soil cover taking shadow and vegetation together
is used. Clevers (1986b) showed that equations (2)
and (3) are not valid with the conventional definition
of soil cover.
In estimating LAI the infrared reflectance is cor
rected for soil background and subsequently this
corrected infrared reflectance is used for estimating
LAI. This latter step may be investigated by using
the calculations with the SAIL model for a black
background. Then the infrared reflectance does not
require correction and the validity of equation (15)
may be checked. The results, shown in figure 4,
support the validity of this equation for describing
the relationship between "corrected" infrared
reflectance and LAI at constant leaf angle distribu
tion. Results presented by Clevers (1986b) show that
distinct leaf angle distributions cause quite distinct