Chemistry, Aerosols & Dynamics
Interactions Research
Goal:
To develop an understanding of the interactions between atmospheric
dynamics, aerosols and chemistry at the meso- and cloud- scales,
particularly with respect to the coupling between transport, cloud
physics, and chemistry.
Atmospheric chemistry can be greatly influenced by
the dynamics governing air motion and meteorology at meso- and cloud-scales.
For example, deep convection can rapidly transport species and aerosols,
such as anthropogenically produced nitrogen oxides, into the upper
troposphere where they have a longer lifetime and are more effective
at modifying ozone concentration, which plays an important role
in oxidizing trace gases in the troposphere. Similarly, mixing across
the top of the planetary boundary layer can redistribute constituents
into the free troposphere. In addition, liquid and solid particles
in clouds provide locations for chemical reactions to occur. Gas-phase
chemistry (in particular sulfur chemistry) influences the quantity
and size of aerosols, which can become cloud condensation nuclei,
providing surfaces for cloud drop formation. In the clouds, chemical
reactions and microphysical processes alter aerosols and their properties
as nuclei for cloud and ice formation. Thus, interactions of chemistry,
aerosols, and the dynamics of clouds are important to several aspects
of atmospheric research.
MMM continues to take a lead
role in research on the coupling of dynamics, chemistry and aerosols
at small scales. We are developing several state-of-the-art cloud-chemistry
models for cloud-topped convective boundary layers and for deep
convective storms.
To understand dynamical interactions with chemical reactions, chemistry
has been incorporated into MMM's LES model and into the COMMAS convective-cloud
model. The LES focuses on eddy transport and entrainment at the
top of the convective PBL. Ongoing development of this coupled LES
includes incorporating cloud and aerosol physics and chemistry,
so that it can be applied to the cloud-topped marine boundary layer.
Transport, turbulent mixing and chemistry within deep convection
are being investigated using COMMAS coupled with chemistry. This
model is currently being applied to thunderstorms observed during
the STERAO-Deep Convection Experiment to determine the contributions
of transport from the boundary layer and from lightning to the nitrogen
oxides. This model is also being used to assess the relative importance
of chemical species transport versus chemical reactions for the
high-plains thunderstorms observed during STERAO. On a larger scale,
ACD's Regional Chemistry and Transport Model (HANK) and MM5 simulations
of STERAO cases are being used to examine the regional/synoptic
scale transport and chemistry for the STERAO convective events.
Information learned from the convective cloud model coupled with
chemistry simulations can be incorporated into HANK to improve descriptions
of convective clouds and chemistry.
Sulfur chemistry directly affects the number and mass of sulfate
aerosols, which are the predominant cloud condensation nuclei. This
in turn affects the development of precipitation through the condensation-coalescence
or the ice process when aerosols act as ice nuclei. These changes
can have large effects on radiative balance, precipitation rates,
and even dynamics. MMM scientists are playing significant roles
in the Indian Ocean Experiment (INDOEX) and subsequent analysis,
examining how aerosols affected cloud microphysical properties.
Studies that parameterize these effects for numerical models and
that investigate interactions between radiation, microphysics, and
aerosols are also underway. Future studies will further examine
effects of aerosols and entrainment on drizzle suppression and cloud
radiative properties, possibly through participation in ACE-Asia.
MMM is collaborating with the development of an NCAR-wide box model
that describes size segregated aerosol physics and chemistry in
detail. This model will be used to guide the model development of
prediction of mass, number concentration, and composition of aerosols
and cloud hydrometeors in the 3-D cloud and meso-scale models mentioned
above.
To provide better representations of chemical transport and the
interactions between chemical species, aerosols, and dynamics, chemistry
is being incorporated in the Weather and Research Forecast (WRF)
model. This coupled chemistry-meteorological model will be used
for the cloud scale and the regional scale, will replace the COMMAS
coupled with chemistry convective model, and will be merged with
ACD's HANK model. Work on this project began with a workshop that
assessed the approaches and methodologies of chemistry modeling
in cloud and mesoscale models. Next a version of WRF coupled with
chemistry will be created so that subgrid parameterizations and
depiction of chemistry processing can be developed, working towards
a complete description of chemical processing on the mesoscale.
The completed model can then be used for many studies including
chemical redistribution by convection, regional-scale transport
of chemical species, and aerosol-cloud interactions.
Coupling of the modeling and
theoretical studies with field programs is crucial; many specific
questions being addressed do not have sufficient observational datasets
to guide the theory and modeling. Efforts in organizing and leading
the STERAO experiment will be continued with similar participation
in upcoming field programs emphasizing deep convection, chemistry,
and aerosols in the mid-latitudes and the tropics. The Dynamics
and Chemistry of Marine Stratocumulus (DYCOMS-II), which was conducted
during the summertime 2001 off the California coast and used several
trace species as tracers of entrainment and mixing within and across
the top of marine stratocumulus. The ongoing work represents cooperative
and interdisciplinary investigations coupling small-scale dynamics
with chemistry, aerosols, and cloud physics. Ultimately, issues
to be addressed are either small-scale in nature, such as air quality
(local, regional), or larger scale in nature, such as climate/chemistry
issues related to ozone production-loss and the role of sulfur species
on cloud microphysics and dynamics. The investigations into clouds
and chemistry will also lead to improvements in, or development
of, parameterizations for large-scale models. Thus, the work directly
supports the goals of the GTCP (Global Tropospheric Chemistry Program)
and climate research.