Light microclimate determines many aspects of plant growth. Introducing the
light-vegetation interactions into a plant model requires a radiative mode
l computing fluxes at the spatial scale described in the plant model. The t
hree-dimensional (3D) architectural models describe plants functionally and
geometrically as sets of interconnected organs. As the geometry of each or
gan is defined, the 3D canopy structure is explicitly described. These mode
ls require calculation of the distribution of light energy on the 3D plant
structure, to integrate physiological processes from organ to plant level.
This has motivated the development of new radiative models. We introduce fi
rst the principles governing the physical interactions between light and a
plant canopy. We present then operational models. Fast methods have been de
veloped for calculating sun and sky light directly intercepted by plant org
ans. Such methods may be used for the simulation of processes depending on
the UV or PAR radiations. Models taking into account the multiple scatterin
g between plant elements are based either on Monte Carlo ray tracing or on
the radiosity method. We present the principle of these approaches and rece
nt developments on their applications to crop modelling. ((C) Inra/Elsevier
, Paris.).