UOEXETER-CMIP-1-1-3: Volcanic optical properties and SO2 emissions #142
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While I admittedly not an expert in volcano forcing, I am very concerned at the low background for mall volcano in the pre-satellite period in this dataset. The new dataset show much more high frequency small volcano activity than CMIP6 which is a huge advance, but gives the impression that a higher background should be applied in the pre-satellite era. While I appreciate the volcano community aspiration that the small volcano SAOD forcing should be provided as episodic, the high frequency apparent from the satellite period and multi-year timescale of the climate response suggest that lack of representation of this background will lead to spuriously high sensitivity to large volcanos. My recommendation would be to add a pre-satellite small volcano to give the same small volcano magnitude as the satellite period. I see this as particular concern with respect to the potential role of volcanos in contributing to the "1960's pothole" among CMIP6 models, and am concern that the current approach will induce a spurious additional cooling affect without inclusion of a "best guess" of the satellite-derived background small volcano activity in the decades before and after the pothole. |
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ping thomasaubry! |
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Comparison of draft CMIP7 (cmip6plus) with CMIP6 (v2) volcanic forcing
Special thanks to Thomas Aubry for providing the CMIP6plus volcanic datasets.
1. Comparison of Prescribed Stratospheric Aerosol Properties (Extinction Profile at 550 nm)
The CMIP7 extinction dataset has improved significantly over the CMIP6 version. Specifically:
2. Comparison of Volcanic SO₂ Emissions Between VolcanEESM and CMIP6plus
VolcanEESM (Volcanic Emissions for Earth System Models):
CMIP6plus:
Key differences between the VolcanEESM database and the CMIP6plus dataset include:
Request for Enhancement
In the CMIP6plus volcanic SO₂ emission dataset, it would be helpful to:
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