We have made a series of general circulation model (GCM) and chemical
transport model (CTM) simulations to examine further the consequences
of biomass burning. We take a three-pronged approach to this study; (1
) examine only the direct short-wave forcing of the smoke clouds by im
posing smoke 'clouds' in the model, (2) examine the indirect effect of
biomass smoke by allowing the biomass smoke to modify the optical pro
perties of existing clouds, reducing the effective (mass) droplet radi
us, and (3) examine the downstream effect by advecting biomass smoke u
sing semi-Lagrangian transport in the GCM. Preliminary results from th
e GCM simulations suggest strong local coolings (2-4 degrees C or more
) where biomass burning occurs with somewhat reduced regional coolings
. Initial results of the transport of smoke by the Australian National
University CTM (ANU-CTM) show the biomass smoke to remain fairly loca
lized with the advection of smoke extending the effects downwind. Copy
right (C) 1996 Elsevier Science Ltd