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On the lack of stratospheric dynamical variability in low-top versions of the CMIP5 models
Cited 256 time in
Web of Science
Cited 279 time in Scopus
- Authors
- Issue Date
- 2013-03
- Publisher
- American Geophysical Union
- Citation
- Journal of geophysical research - Atmospheres, Vol.118 No.6, pp.2494-2505
- Abstract
- We describe the main differences in simulations of stratospheric climate and variability by models within the fifth Coupled Model Intercomparison Project (CMIP5) that have a model top above the stratopause and relatively fine stratospheric vertical resolution (high-top), and those that have a model top below the stratopause (low-top). Although the simulation of mean stratospheric climate by the two model ensembles is similar, the low-top model ensemble has very weak stratospheric variability on daily and interannual time scales. The frequency of major sudden stratospheric warming events is strongly underestimated by the low-top models with less than half the frequency of events observed in the reanalysis data and high-top models. The lack of stratospheric variability in the low-top models affects their stratosphere-troposphere coupling, resulting in short-lived anomalies in the Northern Annular Mode, which do not produce long-lasting tropospheric impacts, as seen in observations. The lack of stratospheric variability, however, does not appear to have any impact on the ability of the low-top models to reproduce past stratospheric temperature trends. We find little improvement in the simulation of decadal variability for the high-top models compared to the low-top, which is likely related to the fact that neither ensemble produces a realistic dynamical response to volcanic eruptions. Citation: Charlton-Perez, A. J., et al. (2013), On the lack of stratospheric dynamical variability in low-top versions of the CMIP5 models, J. Geophys. Res. Atmos., 118, 2494-2505, doi:10.1002/jgrd.50125.
- ISSN
- 2169-897X
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Related Researcher
- College of Natural Sciences
- Department of Earth and Environmental Sciences
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