Abstract
An observationally constrained time series of historical aerosol effective radiative forcing (ERF) from 1750 to 2019 is developed in this study. We find that the time history of aerosol ERFs diagnosed in CMIP6 models exhibits considerable variation and explore how the time history of aerosol forcing influences the probability distributions of present-day aerosol forcing and emergent metrics such as climate sensitivity. Using a simple energy balance model, trained on CMIP6 climate models and constrained by observed near-surface warming and ocean heat uptake, we derive estimates for the historical aerosol forcing. We find 2005–2014 mean aerosol ERF to be −1.1 (−1.8 to −0.5) W m−2 relative to 1750. Assuming recently published historical emissions from fossil fuel and industrial sectors and biomass burning emissions from SSP2-4.5, aerosol ERF in 2019 is −0.9 (−1.5 to −0.4) W m−2. There is a modest recovery in aerosol forcing (+0.025 W m−2 decade−1) between 1980 and 2014. This analysis also gives a 5%–95% range of equilibrium climate sensitivity of 1.8°C –5.1°C (best estimate 3.1°C) with a transient climate response of 1.2°C –2.6°C (best estimate 1.8°C).
| Original language | English |
|---|---|
| Article number | e2020JD033622 |
| Number of pages | 20 |
| Journal | Journal of Geophysical Research: Atmospheres |
| Volume | 126 |
| Issue number | 13 |
| DOIs | |
| Publication status | Published - 16 Jul 2021 |
Bibliographical note
Funding Information:The authors thank Tim Andrews and Adriana Sima for the provision of prototype versions of the HadGEM3‐GC3.1‐LL and IPSL‐CM6A‐LR model outputs respectively, and Maria Rugenstein and Dirk Olivié for helpful discussions. The authors acknowledge the World Climate Research Program, which, through its Working Group on Coupled Modeling, coordinated and promoted CMIP6. The authors thank the climate modeling groups for producing and making available their model output, the Earth System Grid Federation (ESGF) for archiving the data and providing access, and the multiple funding agencies who support CMIP6 and ESGF. C. J. Smith. was supported by a NERC/IIASA Collaborative Research Fellowship (NE/T009381/1). P. M. Forster and G. Myhre were supported by European Union's Horizon 2020 Research and Innovation Program under grant agreement no. 820829 (CONSTRAIN). G. Harris, M. D. Palmer and M. Ringer were supported by the Joint UK BEIS/Defra Met Office Hadley Center Climate Program (GA01101). W. Collins acknowledges funding received from the European Unions Horizon 2020 research and innovation program under grant agreement No 641816 (CRESCENDO). The Energy Exascale Earth System Model (E3SM) is funded by the U.S. Department of Energy, Office of Science, Office of Biological and Environmental Research. Work at LLNL was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under contract DE‐AC52‐07NA27344.
Funding Information:
The authors thank Tim Andrews and Adriana Sima for the provision of prototype versions of the HadGEM3-GC3.1-LL and IPSL-CM6A-LR model outputs respectively, and Maria Rugenstein and Dirk Olivi? for helpful discussions. The authors acknowledge the World Climate Research Program, which, through its Working Group on Coupled Modeling, coordinated and promoted CMIP6. The authors thank the climate modeling groups for producing and making available their model output, the Earth System Grid Federation (ESGF) for archiving the data and providing access, and the multiple funding agencies who support CMIP6 and ESGF. C. J. Smith. was supported by a NERC/IIASA Collaborative Research Fellowship (NE/T009381/1). P. M. Forster and G. Myhre were supported by European Union's Horizon 2020 Research and Innovation Program under grant agreement no. 820829 (CONSTRAIN). G. Harris, M. D. Palmer and M. Ringer were supported by the Joint UK BEIS/Defra Met Office Hadley Center Climate Program (GA01101). W. Collins acknowledges funding received from the European Unions Horizon 2020 research and innovation program under grant agreement No 641816 (CRESCENDO). The Energy Exascale Earth System Model (E3SM) is funded by the U.S. Department of Energy, Office of Science, Office of Biological and Environmental Research. Work at LLNL was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under contract DE-AC52-07NA27344.
Publisher Copyright:
© 2021. The Authors.
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