view factor matrix, is the geometric ratio of energy leaving element i that can reach the element j, E the radiance
due to the direct ill umina tion vector which gives the energy directly incident «1 each element and p fie
individual reflectance vector which gives the reflectance factor for each element, assumed lambertian in this
preliminary study. What is unknown in this equation is then die luminance of element i, called radiosity By. The
so called “radiosity equation”, which balances meaning and outgoing radiation fluxes on discrete surface
elements, can be written as:
N
B. ■ E +p. V F.B.
1 1 K i L* u 1
j- i.j*i
where N is die total number of elements.
B,: Radiosity on surface element i (total radiation flux density leaving that surface).
E ( : Radiance due to direct ill uminati on (equivalent to “emission” of the element),
reflection coefficient
Fy-:’View facta”: specifies the fraction of radiant flux leaving another surface j that reaches
surface i.
As it can be seen on this equation, an element cannot see itself. This equation leads to a rigorous energy balance:
the total radiation flux leaving any surface element i is equal to the sum of its emitted and reflected flux
originating from all other surfaces. As said by Gerstl and Borel (1990), the strengh of die radiosity method cones
from the fact that leaves are treated as individual surfaces that reflect and transmit radiations. This allows the
analysis of radiative effects due to die discrete nature of leaves and stems and their heterogeneous distribution,
e.g. mutual shading and clustering of leaves.
Figure 1: Each element of the canopy is defined by its height h, its length L, its width 1, its orientation 6 and
optical characteristics.
Computing view facta allows to account at once fa all possible direct radiative interactions occuring between
the different elements. The view facta matrix F is computed according to the fish eye method, also described in
Borel et al. (1991). The basic principle is to compute, fa a given element, a fish eye image of the visible
hemisphere from this element, then to compute die relative areas occupied by all the surrounding elements on this
image (figure 2).
The direct illumination vector, E is computed by rj»lmliitin£ for each eiggnent , with a given
resolution, what part of its surface is directly lightened by the sun. The individual reflectance vecta p is given as
input, using field measurements. After the radiosity equation is solved through a Gauss-Jordan algorithm, images
of the canopy are computed. These images can be generated fa any geometric configuration and allow to
simulate the bidirectional reflectance of the canopy in all die directions, with any kind of direct illumination.