Aerosol and physical atmosphere model parameters are both important sources of uncertainty in aerosol ERF

REGAYRE, L.A., JOHNSON, J.S., YOSHIOKA, M., PRINGLE, K.J., SEXTON, D.M.H, BOOTH, B.B.B., LEE, Lindsay, BELLOUIN, N. and CARSLAW, K.S. (2018). Aerosol and physical atmosphere model parameters are both important sources of uncertainty in aerosol ERF. Atmospheric Chemistry and Physics, 18 (13), 9975-10006.

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Abstract

© Author(s) 2018. Changes in aerosols cause a change in net top-of-the-atmosphere (ToA) short-wave and long-wave radiative fluxes; rapid adjustments in clouds, water vapour and temperature; and an effective radiative forcing (ERF) of the planetary energy budget. The diverse sources of model uncertainty and the computational cost of running climate models make it difficult to isolate the main causes of aerosol ERF uncertainty and to understand how observations can be used to constrain it. We explore the aerosol ERF uncertainty by using fast model emulators to generate a very large set of aerosol-climate model variants that span the model uncertainty due to 27 parameters related to atmospheric and aerosol processes. Sensitivity analyses shows that the uncertainty in the ToA flux is dominated (around 80 %) by uncertainties in the physical atmosphere model, particularly parameters that affect cloud reflectivity. However, uncertainty in the change in ToA flux caused by aerosol emissions over the industrial period (the aerosol ERF) is controlled by a combination of uncertainties in aerosol (around 60 %) and physical atmosphere (around 40 %) parameters. Four atmospheric and aerosol parameters account for around 80 % of the uncertainty in short-wave ToA flux (mostly parameters that directly scale cloud reflectivity, cloud water content or cloud droplet concentrations), and these parameters also account for around 60 % of the aerosol ERF uncertainty. The common causes of uncertainty mean that constraining the modelled planetary brightness to tightly match satellite observations changes the lower 95 % credible aerosol ERF value from -2.65 to -2.37 W m-2. This suggests the strongest forcings (below around -2.4 W m-2) are inconsistent with observations. These results show that, regardless of the fact that the ToA flux is 2 orders of magnitude larger than the aerosol ERF, the observed flux can constrain the uncertainty in ERF because their values are connected by constrainable process parameters. The key to reducing the aerosol ERF uncertainty further will be to identify observations that can additionally constrain individual parameter ranges and/or combined parameter effects, which can be achieved through sensitivity analysis of perturbed parameter ensembles.

Item Type:	Article
Uncontrolled Keywords:	0201 Astronomical and Space Sciences; 0401 Atmospheric Sciences; Meteorology & Atmospheric Sciences
Identification Number:	https://doi.org/10.5194/acp-18-9975-2018
Page Range:	9975-10006
SWORD Depositor:	Symplectic Elements
Depositing User:	Symplectic Elements
Date Deposited:	12 May 2021 13:46
Last Modified:	12 May 2021 14:00
URI:	https://shura.shu.ac.uk/id/eprint/26692

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