This work aims at presenting the numerical solution to a natural conve
ction problem concerning the use of a passive solar system for buildin
g heating purpose. The system consists of a modification of the well-k
nown Trombe-Michel passive system. The main differences consist of the
rmal insulation on the southern wall surface, the presence of two sola
r ducts separated by a thin metallic plate with collector function, an
d a thermal storage over the ceiling of the heated rooms. The numerica
l solution to the simple mathematical model -based on energy and mass
conservation equations -is achieved by a finite difference method, whi
ch allows to determine both the time-dependent temperature profile on
each component of the system and the air flow pattern in the solar duc
ts. A comparison between the numerical results and some experimental d
ata is reported: it shows a very satisfactory agreement. At last, the
hour by hour energy fluxes are shown in some graphs. (C) Elsevier, Par
is.