4.6 Article

Climate, Variability, and Climate Sensitivity of Middle Atmosphere Chemistry Configurations of the Community Earth System Model Version 2, Whole Atmosphere Community Climate Model Version 6 (CESM2(WACCM6))

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AMER GEOPHYSICAL UNION
DOI: 10.1029/2022MS003579

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CESM; climate; stratosphere; ozone

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Simulating the dynamics, chemistry, and physics of the entire atmosphere is computationally expensive. Simplified chemistry configurations can reliably simulate the whole atmosphere with reduced computational resources, except for cases requiring an accurate representation of tropospheric organic chemistry and secondary organic aerosols.
Simulating whole atmosphere dynamics, chemistry, and physics is computationally expensive. It can require high vertical resolution throughout the middle and upper atmosphere, as well as a comprehensive chemistry and aerosol scheme coupled to radiation physics. An unintentional outcome of the development of one of the most sophisticated and hence computationally expensive model configurations is that it often excludes a broad community of users with limited computational resources. Here, we analyze two configurations of the Community Earth System Model Version 2, Whole Atmosphere Community Climate Model Version 6 (CESM2(WACCM6)) with simplified middle atmosphere chemistry at nominal 1 and 2 & DEG; horizontal resolutions. Using observations, a reanalysis, and direct model comparisons, we find that these configurations generally reproduce the climate, variability, and climate sensitivity of the 1 & DEG; nominal horizontal resolution configuration with comprehensive chemistry. While the background stratospheric aerosol optical depth is elevated in the middle atmosphere configurations as compared to the comprehensive chemistry configuration, it is comparable among all configurations during volcanic eruptions. For any purposes other than those needing an accurate representation of tropospheric organic chemistry and secondary organic aerosols, these simplified chemistry configurations deliver reliable simulations of the whole atmosphere that require 35% and 86% fewer computational resources at nominal 1 and 2 & DEG; horizontal resolution, respectively.

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