https://gmd.copernicus.org/preprints/gmd-2023-79/

*Authors*
Simone Tilmes <[email protected]>, Michael J. Mills, Yunqian Zhu, Charles G.
Bardeen, Francis Vitt, Pengfei Yu, David Fillmore, Xiaohong Liu, Brian Toon
, and Terry Deshler
How to cite. Tilmes, S., Mills, M. J., Zhu, Y., Bardeen, C. G., Vitt, F.,
Yu, P., Fillmore, D., Liu, X., Toon, B., and Deshler, T.: Description and
performance of the CARMA sectional aerosol microphysical model in CESM2,
Geosci. Model Dev. Discuss. [preprint], https://doi.org/10.5194/gmd-2023-79,
in review, 2023.
*Received: 15 Apr 2023 – Discussion started: 25 Apr 2023*

Abstract. We implemented the Community Aerosol and Radiation Model for
Atmospheres (CARMA) in both the high and low-top model versions of the
Community Earth System Model Version 2 (CESM2). CARMA is a sectional
microphysical model, which we use for aerosol in both the troposphere and
stratosphere. CARMA is fully coupled to chemistry, clouds, radiation, and
transport routines in CESM2. This development enables the comparison of
simulations with a sectional (CARMA) and a modal (MAM4) aerosol
microphysical model in the same modeling framework. The new implementation
of CARMA has been adopted from previous work with some additions that align
with the current CESM2 MAM4 implementation. The main updates include an
interactive secondary organic aerosol description in CARMA using the
volatility basis set (VBS) approach, updated wet removal, and the use of
transient emissions of aerosols and trace gases. In addition, we
implemented an alternative aerosol nucleation scheme in CARMA, which is
also used in MAM4. Detailed comparisons of stratospheric aerosol properties
after the Mt Pinatubo eruption reveal the importance of prescribing sulfur
injections in a larger region rather than in a single column to better
represent the observed evolution of aerosols. Both CARMA and MAM4 in CESM2
are able to represent stratospheric and tropospheric aerosol properties
reasonably well compared to observations. Several differences in the
performance of the two aerosol models show, in general, an improved
representation of aerosols using the sectional aerosol model in CESM2.
These include a better representation of the aerosol size distribution
after the Mt Pinatubo volcanic eruption in CARMA compared to MAM4. MAM4
produces on average smaller aerosols and less removal than CARMA, which
results in a larger total mass. Both CARMA and MAM4 reproduce stratospheric
Aerosol Optical Depth (AOD) within the errorbar of the observations between
2001 and 2020, except for recent larger volcanic eruptions that are
overestimated by both model configurations. The CARMA background surface
area density and aerosol size distribution in the stratosphere and
troposphere compare well to observations, with some underestimation of the
Aitken-mode size range. MAM4 shows shortcomings in reproducing coarse-mode
aerosol distributions in the stratosphere and troposphere. This work
outlines additional development needs for CESM2 CARMA to improve the model
compared to observations in both the troposphere and stratosphere.

*Source: European Geosciences Union*

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