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2. MATERIALS AND METHODS 2.2. Field spectroscopic data
2.1. Agronomic data
The study area was located in the
Laureinepolder in Watervliet, close to
the border with the Netherlands. The
geographical coordinates are 51°17’ N
and 3°40’ E. The soil is a fertile
Aquic Udifluvent .
The winter wheat cultivars included in
the experiments were 'Granta' in 1984,
'Castell' in 1985, 'Sarno' in 1986 and
'Cas tell' in 1988.
In 1984 and 1985 the experiments were
carried out on commercial fields, and
the crops received normal amounts of
fertilizer. In 1986 and 1988 the
experiments were conducted on
experimental test plots which received
different amounts of N-fertilizer: 0
kg, 200 kg and 275 kg in 1986, 0 kg,
100 kg, 150 kg, 250 kg and 325 kg in
1988. Green (1987) showed that
increased nitrogen application causes
an increase of the leaf area without
changing leaf properties and leaf
angle. Hence a wider range of biomass
data were available allowing for more
accurate reflectance/LAI relationship
modelling.
For each day that field measurements
took place in 1984 and 1985, three
random colour infrared (CIR)
photographic and LAI samples were
taken. Samples measuring 20 cm x 40 cm
were randomly harvested in the area
covered by colour infrared photography.
Harvested green leaf blades were
spread out on a matt-black painted
surface (60 cm x 80 cm) and recorded on
black-and-white film.
In the dark room, after development of
the negatives, a transparent dot grid
(dot dimension 1.13 mm 2 , each dot
representing .14 cm 2 ) was placed
directly on the light-sensitive paper
(18 cm X 24 cm) during exposure.
The actual dot counting was facilitated
by an in-house developed
electro-mechanical counting device.
Knowing the total amount of dots
falling on leaves, LAI could be
computed as dimensions of black
background and sample plot were known.
In 1986 and 1988, one (CIR)
photographic and LAI sample was taken
of each test, plot per field day. In
1986 and 1988 leaves of 10 and 25
plants were photocopied on a well-tuned
photocopier. The data collected in 1986
were counted using a transparent dot
grid overlay. The data collected in
1988 were digitized with a CCD camera.
Density slicing of a videodigitized
photocopy allowed for the calculation
of white (non-leaf) and black (leaf)
areas. The LAI could be calculated
from the average plant density of the
experimental plots.
Ground-based multispectral photography
was chosen as the field spectroscopy
method to obtain multispectral
reflectance data of agricultural
crops. The used method is described in
detail by De Wulf and Goossens (1988).
Field spectroscopic data were collected
10 times during the growing season with
approximately 10 days intervals,
starting at the end of April and ending
at harvest around mid August. Hence the
phenological stages between
stem-elongation and maturity were
covered.
The camera-to-ground distance was kept
constant at 2.30 m. The covered ground
area measured 2.1 m 2 .
The Kodak neutral test card (20 cm x
25 cm) was used throughout the
experiments as reflectance standard.
For each recording it was positioned at
the height of the crop canopy and
covered approximately 2.5 % of the
photographed area.
A few exceptions notwithstanding,
measurements were taken close to solar
noon in nadir viewing position.
Due to the latitude of the test area,
the solar zenith angles ranged between
28° and 52°.
To obtain consistency in azimuthal
position, as recommended by Milton
(1987), all measurements were taken
with the sun either left or right of
the operator (azimuth angles of 90° and
270°). This symmetrical configuration
had the additional effect that the
target and the grey card were never
shaded by the recording platform.
The extraction of relative reflectance
from CIR transparencies has also been
described in detail by De Wulf and
Goossens (1988).
Following vegetation indices were
calculated from green (G) , red (R) and
infrared (IR) reflectance.
1. Simple ratio (SR) (Rouse et al.,
cit. Bariou et al. 1985)
SR = IR / R
2. Ratio Infrared/Visible (RIV)
RIV = IR/VIS
with VIS = average reflec
tance in the
covered visible
part of the E.M.
spectrum
= (G+Rl/2
3. Normalized Difference (ND) (Rouse et
al.. cit. Bariou et al. 1985)
ND = (IR-R)/(IR+R)
4. Normalized Difference of Infrared
and Visible (NDIV)
NDIV = (IR-VIS)/(IR+VIS)