Monday, 15 July 2002
Effects of domain size and numerical resolution on the simulation of shallow cumulus convection
David E. Stevens, LLNL, Livermore, CA
Poster PDF
(3.2 MB)
This talk presents three-dimensional numerical simulations of oceanic
trade cumulus clouds underlying stratocumulus clouds. They are based on
a case studied in a Global Energy and Water Experiment Cloud System
Study (GCSS) model intercomparison that is loosely based on observed
conditions during the Atlantic Trade Cumulus Experiment (ATEX). It is
motivated by the importance of this cloud type to global cloud radiative
forcing, and their role as a feeder system for deep convection in the
tropics. This study focuses on the sensitivity of the modeled cloud
field to the domain size and the grid spacing. Domain widths from 6.5 to
20 kilometers and horizontal grid spacings ranging from 10 to 80 meters,
with corresponding vertical grid spacing ranging from 5 to 40 m, are
studied, involving massively parallel computations on up to 2.5 billion
grid-cells. The combination of large domain size and small grid
resolution provides an unprecedented perspective on this type of
convection.
The mean stratocumulus cloud fraction, optical depth, and vertical
fluxes of heat, moisture and momentum are found to be quite sensitive to
both the domain size and the resolution. The sensitivities are
associated with a strong feedback between cloud fraction, cloud-top
radiative cooling, and entrainment. The properties of individual cumulus
clouds rising into the stratocumulus are less affected than the
stratocumulus clouds. The simulations with 80 m horizontal/40 m vertical
resolution are clearly under-resolved, with distinctly different
distributions of liquid water within the clouds. Increasing the
resolution to finer than 40 m horizontal/20 m vertical affects the
inversion structure and entrainment processes somewhat, but has less
impact on the structure of individual clouds. Large-domain simulations
exhibit mesoscale structure in the cloud organization and liquid water
path. This mesoscale variability feeds back on the domain-mean
properties through the cloud-radiative feedback. These simulations
suggest that very large computations are required to obtain meaningful
cloud statistics for this case.
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