Davis, N.A. orcid.org/0000-0002-5691-2020, Visioni, D. orcid.org/0000-0002-7342-2189, Garcia, R.R. orcid.org/0000-0002-6963-4592 et al. (11 more authors) (2023) 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)). Journal of Advances in Modeling Earth Systems, 15 (9). e2022MS003579. ISSN 1942-2466
Abstract
Abstract
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° 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° 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° horizontal resolution, respectively.
Key Points
There are differences in stratospheric aerosol optical depth between comprehensive and simplified chemistry configurations
Simplifying the chemistry scheme generally has smaller global impacts than coarsening the horizontal resolution
All configurations have similar climate sensitivities and responses to forcings
Plain Language Summary
Modeling the entire atmosphere, or at least from the surface to an altitude of 140 km (87 miles), takes a lot of computer resources. Simulating 1 year can require the equivalent of thousands of personal computers running for 1 day, for example, which is only realistic for researchers with access to a supercomputer. There are many people who would like to simulate the whole atmosphere to study climate change, space weather, and extreme events, but even with access to a supercomputer, it is still computationally expensive to run. We examined a whole atmosphere model with a simpler chemistry scheme, and at a lower horizontal resolution, to see if it still reproduces major features of climate and climate change. The two configurations perform similarly to the high resolution simulation with complex chemistry, with some minor and understandable differences. Anyone looking to simulate the whole atmosphere, using fewer computational resources, can do so confidently using the described model configurations, as long as they are aware of some of the deficiencies.
Metadata
Item Type: | Article |
---|---|
Authors/Creators: |
|
Copyright, Publisher and Additional Information: | © 2023 The Authors. Journal of Advances in Modeling Earth Systems published by Wiley Periodicals LLC on behalf of American Geophysical Union. This is an open access article under the terms of the Creative Commons Attribution-NonCommercial License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited and is not used for commercial purposes. |
Keywords: | CESM; climate; stratosphere; ozone |
Dates: |
|
Institution: | The University of Leeds |
Academic Units: | The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds) > Astrophysics (Leeds) |
Depositing User: | Symplectic Publications |
Date Deposited: | 16 Oct 2023 10:08 |
Last Modified: | 16 Oct 2023 10:08 |
Published Version: | https://doi.org/10.1029/2022MS003579 |
Status: | Published |
Publisher: | American Geophysical Union |
Identification Number: | 10.1029/2022ms003579 |
Related URLs: | |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:204224 |