Although CO2 snowfall has never been directly observed on Mars, it has
been suggested that such precipitation may explain the puzzling infra
red measurements obtained by Mariner 9 and Viking during the polar nig
ht in each hemisphere. The radiative effect of the snow would strongly
alter the radiative balance of the condensing polar caps and thus the
CO2 cycle and the global climate. We have simulated this phenomenon w
ith a general circulation model (GCM). For that purpose, a new paramet
erization of CO2 condensation in the atmosphere and on the ground has
been developed, paging particular attention to mass and energy conserv
ation and allowing for the possible sublimation of sedimenting COL ice
particles. Atmospheric condensation may result from radiative cooling
on the one hand (especially when the atmosphere is dust laden) and fr
om adiabatic cooling in upward motions on the other hand. This latter
process can be very efficient locally. On this basis, we have modeled
the effect of the CO2 snowfall on the infrared emission by decreasing
the local emissivities when atmospheric condensation was predicted by
the model. This parameterization is based on physical considerations (
radiative transfer through the CO2 ice particles, snow metamorphism on
the ground). Without tuning the model parameters, we have been able t
o accurately reproduce the general behavior of the features observed b
y Viking in the thermal infrared. These modeling results support the C
O2 snowfall scenario suggested from the observations. Overall, this ne
w parameterization, used in combination with the digital terrain model
topography and with allowance for a varying atmospheric dust content,
allows the GCM to simulate the CO2 condensation-sublimation cycle rea
listically. In particular, the seasonal variations of the surface pres
sure recorded by the Viking Landers can now be reproduced without arti
ficially decreasing the condensation rate as was done in previous stud
ies. (C) 1998 Academic Press.