Pattern Recognition Methods to Separate Forced Responses from Internal Variability in Climate Model Ensembles and Observations
Abstract
Ensembles of climate model simulations are commonly used to separate externally forced climate change from internal variability. However, much of the information gained from running large ensembles is lost in traditional methods of data reduction such as linear trend analysis or large-scale spatial averaging. This paper demonstrates how a pattern recognition method (signal-to-noise-maximizing pattern filtering) extracts patterns of externally forced climate change from large ensembles and identifies the forced climate response with up to ten times fewer ensemble members than simple ensemble averaging. It is particularly effective at filtering out spatially coherent modes of internal variability (e.g., El Niño, North Atlantic Oscillation), which would otherwise alias into estimates of regional responses to forcing. This method is used to identify forced climate responses within the 40-member Community Earth System Model (CESM) large ensemble, including an El-Niño-like response to volcanic eruptions and forced trends in the North Atlantic Oscillation. The ensemble-based estimate of the forced response is used to test statistical methods for isolating the forced response from a single realization (i.e., individual ensemble members). Low-frequency pattern filtering is found to skillfully identify the forced response within individual ensemble members and is applied to the HadCRUT4 reconstruction of observed temperatures, whereby it identifies slow components of observed temperature changes that are consistent with the expected effects of anthropogenic greenhouse gas and aerosol forcing.
Additional Information
© 2020 American Meteorological Society. Manuscript received 25 November 2019, in final form 16 July 2020. R.C.J.W. and D.S.B. acknowledge support from the National Science Foundation (Grant AGS-1929775) and the Tamaki Foundation. R.C.J.W. and K.C.A. acknowledge support from the National Science Foundation (Grant AGS-1752796). R.C.J.W. is also supported by the University of Washington eScience Institute. T.S. is supported by Eric and Wendy Schmidt by recommendation of the Schmidt Futures program and by the Earthrise Alliance. The CESM project is supported primarily by the National Science Foundation (NSF). This material is based on work supported by the National Center for Atmospheric Research, which is a major facility sponsored by the NSF under Cooperative Agreement no. 1852977. We thank Dennis Hartmann, Cristian Proistosescu, Flavio Lehner, Elizabeth Maroon, Mingfang Ting, and David Bonan for valuable input on this work. The code for S/NP filtering is available at github.com/rcjwills/forced806 patterns. The code for LFCA is available at github.com/rcjwills/lfca.Attached Files
Published - jclid190855.pdf
Supplemental Material - 10.1175_jcli-d-19-0855.s1.pdf
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Additional details
- Eprint ID
- 104645
- Resolver ID
- CaltechAUTHORS:20200729-145256584
- NSF
- AGS-1929775
- Tamaki Foundation
- NSF
- AGS-1752796
- University of Washington
- Eric and Wendy Schmidt
- Schmidt Futures Program
- Earthrise Alliance
- National Center for Atmospheric Research (NCAR)
- NSF
- AGS-1852977
- Created
-
2020-07-29Created from EPrint's datestamp field
- Updated
-
2023-06-01Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences