V.V. Filyushkin, D.K. Lilly, Y.L. Kogan
Cooperative Institute for Mesoscale Meteorological Studies
University of Oklahoma
Norman, OK 73019
ph. 405-325-6091; fax 405-325-7614
Internet: victorf@geohub.gcn.uoknor.edu
A Marine Stratocumulus-Topped Planetary Boundary Layer is an important
climate-forming element. This is due to the high solar radiation reflectivity
of cloud deks which, with relatively small changes, can compensate or enhance
the warming due to "greenhouse" gases. A number of mechanisms potentially
capable of influencing the properties of marine stratocumuli has been proposed
recently. However, the overall effect depends on the interaction between
microphysics, 3D dynamics, radiation, and chemistry The results of 3D Large
Eddy Simulation Model of a Sc-Topped Layer with explicit microphysics are
analyzed in this study, with emphasis on the interaction of microphysical
processes with 3D convective dynamics. We analyze cycles of cloud condensation
nucleus turnover due to condensation in updrafts and regeneration from
evaporating drops in downdrafts. Similar analysis of drop lifecycles is made
for different stages of stratocumulus development.