Cloud Feedbacks from CanESM2 to CanESM5.0 and their influence on climate sensitivity
- 1Department of Geography & Environmental Management, University of Waterloo, Waterloo, Ontario, Canada
- 2Canadian Centre for Climate Modelling and Analysis, Environment and Climate Change Canada, Victoria, British Columbia, Canada
- 3Ministry of Health, Government of British Columbia, Victoria, British Columbia, Canada
Correspondence: John G. Virgin (firstname.lastname@example.org)
The newest iteration of the Canadian Earth System Model (CanESM5.0.3) has an effective climate sensitivity (EffCS) of 5.65 K, which is a 54 % increase relative to the model's previous version (CanESM2 – 3.67 K), and the highest sensitivity of all current models participating in the sixth phase of the coupled model inter-comparison project (CMIP6). Here, we explore the underlying causes behind CanESM5's increased EffCS via comparison of forcing and feedbacks between CanESM2 and CanESM5. We find only modest differences in radiative forcing as a response to CO2 between model versions. We find small increases in the surface albedo and longwave cloud feedback, as well as a substantial increase in the SW cloud feedback in CanESM5. Through the use of cloud area fraction output and cloud radiative kernels, we find that more positive low and non-low shortwave cloud feedbacks – particularly with regards to low clouds across the equatorial Pacific, as well as subtropical and extratropical free troposphere cloud optical depth – are the dominant contributors to CanESM5's increased climate sensitivity. Additional simulations with prescribed sea surface temperatures reveal that the spatial pattern of surface temperature change exerts controls on the magnitude and spatial distribution of low-cloud fraction response but does not fully explain the increased EffCS in CanESM5. The results from CanESM5 are consistent with increased EffCS in several other CMIP6 models, which has been primarily attributed to changes in shortwave cloud feedbacks.
Equilibrium climate sensitivity (ECS), defined as the global annual mean surface warming the Earth would exhibit as a response to a doubling of CO2, is a frequently cited emergent property from simplified climate models (Charney et al., 1979), as well as modern Earth system models (ESMs) (Andrews et al., 2012; Vial et al., 2013). The first estimates of ECS from Earth system models ranged from 1.5–4.5 K (Charney et al., 1979). In the latest phase of the Coupled Model Inter-comparison Project (CMIP6), the range of ECS from participating models has widened (1.8–5.5 K), with the mean shifting towards higher values than the previous phase of CMIP (3.2 to 3.7 K from CMIP5 to CMIP6) (Flynn and Mauritsen, 2020; Zelinka et al., 2020). Inter-model spread of ECS is primarily attributed to radiative feedbacks on the climate system, specifically with regards to cloud feedbacks, which are the primary source of spread across models (Caldwell et al., 2016; Vial et al., 2013; Dufresne and Bony, 2008).
Understanding cloud feedback uncertainty and its influence on the ECS of ESMs has been an imperative of researchers in recent decades – particularly with regards to properties such as cloud optical depth, which determine the amount of reflected shortwave (SW) radiation and thus help cool the planet (Vial et al., 2013; Tan et al., 2016; Zelinka et al., 2020; Bjordal et al., 2020). SW cloud feedbacks can be separated based on latitude; middle-latitude SW cloud feedbacks are mostly negative from the optical thickening of clouds due to phase transition towards liquid in ice- and mixed-phase clouds (Goosse et al., 2018; Senior and Ingram, 1989). At high latitudes, sea ice loss exposes the ocean surface and increases surface turbulent fluxes and therefore humidity, which increases low-level cloudiness (Goosse et al., 2018). At low latitudes, the SW cloud feedback is robustly positive in both ESMs and large eddy simulations (LESs), owing to a reduction in the fraction and thickness of marine shallow cumulus and stratocumulus clouds near the planetary boundary layer (PBL) (Bretherton and Blossey, 2014; Bretherton et al., 2013; Ceppi et al., 2017). The physical mechanisms behind SW low-cloud feedbacks are tied to multiple thermodynamic, radiative, and dynamical processes, termed cloud controlling factors (CCFs) (Klein et al., 2017). Specifically, mechanisms favouring an increase in low-cloud fraction in baseline climatology regimes include stronger PBL temperature inversions (Wood and Bretherton, 2006; Klein and Hartmann, 1993; Bretherton et al., 2013), colder sea surface temperatures (SSTs) (Bretherton and Blossey, 2014), less subsidence (Blossey et al., 2013), and increased free troposphere humidity (Van der Dussen et al., 2015).
While the sensitivity of marine low-cloud cover (LCC) to specific factors varies significantly from model to model, differing sensitivities to SSTs have been identified as a explanatory factor for spread across ESMs (Qu et al., 2014). This link suggests the spatial pattern of surface warming has important implications for low-cloud responses (Rose et al., 2014; Zhou et al., 2015) and therefore the SW cloud feedback and climate sensitivity (Andrews and Webb, 2018).
Here, we investigate the causes of increased climate sensitivity in the newest version of the Canadian Earth System Model, which is the highest of all models currently participating in CMIP6 (Flynn and Mauritsen, 2020). We examine the particularly high ECS of the Canadian Earth System Model 5 (CanESM5) in relation to the previous model version that was contributed to CMIP5 (CanESM2). With a particular focus on decomposed cloud feedbacks, we quantify the differences in both forcing and feedback between CanESM2 and CanESM5 in order to establish a physical link for the shift in ECS. Lastly, we examine the spatial pattern of warming in CanESM5 and its influence of both global mean and local cloud feedbacks as a potential explanatory variable for CanESM5's high ECS.
We compare two versions of CanESM in this study. CanESM2, the second-generation Earth system model from the Canadian Centre for Climate Modelling and Analysis (CCCma), consists of their fourth-generation atmosphere model (CanAM4), land surface model (CLASS), terrestrial carbon model (CTEM), CSM ocean model from the National Centre for Atmosphere Research (NCAR), and ocean carbon model (CMOC) (von Salzen et al., 2013; Arora et al., 2009; Zahariev et al., 2008; Arora et al., 2011; Gent et al., 1998). CanESM5 (Swart et al., 2019b) is the newest generation of the Canadian Earth System Model and uses an updated version of CLASS (version 2.7 to 3.6.2) (Verseghy, 2000); CanNEMO, which is based on NEMO3.4.1 (Madec, 2012), for the ocean model; and the Louvain-la-Neuve sea ice model (LIM2) (Fichefet and Maqueda, 1997; Bouillon et al., 2009).
The fifth-generation atmospheric model (CanAM5) has the same horizontal resolution as CanAM4 while increasing the vertical layers from 35 to 49, with majority of the additional layers added to the upper troposphere and lower stratosphere. While there are a number of improvements to radiative transfer, aerosol, and surface parameterization, changes to cloud parameterizations are discussed briefly given their direct potential connection to cloud feedbacks. Ice cloud parameterizations in CanAM5 largely remain the same as in CanAM4 (von Salzen et al., 2013), with the exception of adjustments to uncertain parameters. For liquid clouds, the primary change is autoconversion of cloud liquid to rain in CanAM5, which now uses the parameterization of Wood (2005) instead of the parameterization of Khairoutdinov and Kogan (2000) that was used in CanAM4. The change in autoconversion parameterization includes the second indirect aerosol effect – a process not considered in CanAM4 (von Salzen et al., 2013).
2.2 Forcing-feedback analysis
We consider energy balance at Earth's top of atmosphere (TOA) using the following equation:
where N is net radiation imbalance (in W m−2), F is the effective radiative forcing (ERF) due to that of an external agent (e.g. CO2, in W m−2), ΔTs is the global annual mean surface temperature response (in kelvin), and λ is the net climate feedback parameter (in W m−2 K−1). Equation (1) assumes a linear relationship between radiation imbalance and surface temperature response (i.e. a constant λ). Under this assumption, an Earth system model with a stronger (more negative) λ term will re-establish energy balance faster (and with a weaker surface temperature response) than a weak λ term. We calculate the net feedback parameter using pre-industrial control and abrupt 4×CO2 experiments for each version of CanESM. For CanESM2, we use 150 years of pre-industrial control and abrupt 4×CO2 coupled model output submitted to the Earth System Grid Federation under run 1, initialization 1, and physics 1 (r1i1p1) (Taylor et al., 2012). For CanESM5, we use the same experiments submitted for the core CMIP6 experiment deck (Eyring et al., 2016).
The surface temperature response after the system has reached equilibrium (N=0 W m−2) is defined as the effective climate sensitivity, which is typically measured under a 2×CO2 ERF (). We use the term “effective” above, as opposed to “equilibrium” climate sensitivity, given the linear assumptions in Eq. (1), where equilibrium climate sensitivity is representative of warming once the system as reached true equilibrium and does not require any form of statistical extrapolation (Knutti et al., 2017). The extent that the linear approximation accurately represents both forcing and feedback varies from model to model, where some models exhibit a more linear response to CO2 than others (Andrews et al., 2012). A time-varying net feedback parameter has been at least partially attributable to differences in model timescale and magnitude of “rapid adjustments” in the climate system, where quick tropospheric climate response to CO2 modifies TOA energy balance (Smith et al., 2018; Forster et al., 2013; Sherwood et al., 2015).
We consider the influence of rapid adjustments by diagnosing the ERF using two distinct methods. First, we use an ordinary least-squares linear regression between TOA radiation imbalance (N) and surface temperature response (ΔTs) in abrupt 4×CO2 experiments, where the extrapolated y intercept of the regression line equals 2× the ERF (ERFg, Gregory et al., 2004). Second, we use 30-year fixed sea surface temperature experiments (piClim-control and piClim-4×CO2) submitted to the Radiative Forcing Model Inter-comparison Project (RFMIP) (Pincus et al., 2016). The ERF is calculated by differencing net TOA radiation in 30-year annual mean fixed sea surface temperature experiments (ERFh), where one experiment uses pre-industrial control CO2 and the other uses abrupt 4×CO2 (Hansen et al., 2005; Pincus et al., 2016). Under the ERFh definition, both tropospheric and stratospheric rapid adjustments from clouds, air temperature, water vapour, and surface albedo are included along with CO2.
Using the Gregory regression method, we obtain the net feedback parameter as the slope of the regression line. Furthermore, we quantify the EffCS for an abrupt 2×CO2 forcing as the extrapolated x intercept of the regression line divided by 2. We consider the net feedback parameter as the linear sum of individual radiative feedbacks within the climate system:
where the net feedback parameter is made up of contributions from Planck (λp), lapse rate (λlr), water vapour (λwv), surface albedo (λa), and cloud (λc) feedbacks. A residual term is also included (Re) in order to account for non-linearities. We use a combination of the radiative kernel and Gregory regression methods to diagnose individual radiative feedbacks (Block and Mauritsen, 2013; Soden and Held, 2006). Specifically, we use six sets of radiative kernels to calculate TOA fluxes for temperature, water vapour, and surface albedo responses (Soden et al., 2008; Block and Mauritsen, 2013; Shell et al., 2008; Pendergrass et al., 2018; Huang et al., 2017; Smith, 2018). Following this, each flux is linearly regressed against global annual mean surface temperature response for 150 years, where the slope of the regression line is considered the feedback value (in W m−2 K−1). We use the clear-sky linearity test to validate the accuracy of each radiative kernel (Shell et al., 2008), where the sum of all clear-sky feedbacks is compared against the net clear-sky climate feedback parameter as estimated using the Gregory regression technique with clear-sky TOA flux. Three radiative kernels passed the clear-sky linearity test (relative errors of less than 10 %) (Fig. A1), which are used to calculate an ensemble kernel mean for all feedbacks. The three sets of kernels that passed the clear-sky linearity test are derived from the Geophysical Fluid Dynamics Laboratory (GFDL) ESM (Soden et al., 2008), the Hadley Centre Global Environment Model (HadGEM2) (Smith, 2018), and a combination of the ERA-interim reanalysis data set and the Rapid Radiative Transfer Model (RRTM) (Huang et al., 2017).
2.3 Cloud feedbacks
Cloud feedbacks cannot be calculated via the standard radiative kernel method due to non-linearities associated with cloud vertical overlap (Soden et al., 2008). We estimate cloud feedbacks using two methods – the adjusted cloud radiative effect (CRE) and cloud radiative kernel method. The CRE response is defined as the difference between clear-sky and total radiative fluxes. We adjust the CRE for the effects of environmental masking from other feedbacks using clear-sky radiative kernels (Soden et al., 2004). The CRE “adjustment” using clear-sky radiative kernels takes into account differences in temperature and water vapour between a clear and cloudy atmosphere to isolate the radiative perturbation from clouds. We also account for the masking effect of CO2 forcing by using a globally uniform proportionality constant of 1.16 between clear-sky and total CO2 forcing (Soden et al., 2008; Chung and Soden, 2015). After adjusting the CRE, the cloud flux response is regressed similarly to noncloud feedbacks, where the slope of the regression line equals the cloud feedback. This method is performed twice to yield a value for both the shortwave (SW) and longwave (LW) cloud feedbacks.
We use cloud radiative kernels and cloud area fraction output from the International Satellite Cloud Climatology Project (ISCCP), produced from the CFMIP Observation Simulator Package (COSP) (Bodas-Salcedo et al., 2011) in CanESM2 and CanESM5, to diagnose cloud feedbacks for different cloud top pressures and optical depths (Zelinka et al., 2012a). Specifically, we calculate a cloud area fraction response, relative to a pre-industrial control climatology, for every year, grid point, optical depth, and cloud top pressure bin in the abrupt 4×CO2 simulation. Following this, cloud radiative kernels are applied to the cloud area fraction response to derive TOA flux perturbations. Similar to noncloud feedbacks, each point is then linearly regressed against global annual mean surface temperature response over 150 years, where the slope of the regression line is equal to the feedback value.
In this study, we consider low clouds as having their tops at ≥680 hPa and non-low clouds as having their tops at ≤680 hPa. A key limitation of COSP output is the potential obscuring of low clouds via a shift in the distribution of high-cloud fraction (Zelinka et al., 2018). We account for the obscuring of low clouds via normalizing low-cloud fraction using upper-level clear-sky fraction as in Scott et al. (2020). Using this method, non-obscured low-cloud responses are weighted by the area fraction not covered by high clouds.
To further separate cloud feedbacks into contributions from cloud altitude, optical depth, and amount components, we utilize the refined decomposition technique as in Zelinka et al. (2016). Using this method, cloud kernels are decomposed into individual components for cloud amount, optical depth, altitude, and residuals, while cloud area fraction anomalies are resolved into contributions from altitude and optical depth shifts and total amount separately. For a full mathematical breakdown of this decomposition, see Appendix B in Zelinka et al. (2013) and the Supplement of Zelinka et al. (2016).
For CanESM2, only 40 years of cloud area fraction data (years 1–20 and 120–140) were available in the abrupt 4×CO2 simulation. To test the impact of sample size on our results, we subsample the output from the CanESM5 abrupt 4×CO2 simulation for the same time periods as those available from CanESM2 (years 1–20 and 120–140) and find highly similar results to those obtained from the full 150 years (Fig. A2). Furthermore, we find very similar results for LW and SW cloud feedback components from CanESM2 and CanESM5 computed using the radiative kernel method and the adjusted-CRE method (Fig. A3). This provides confidence that both methods are accurately capturing the pattern and magnitude of cloud feedbacks in these models.
3.1 Effective climate sensitivity and radiative forcing
We begin by quantifying net feedback, forcing, and EffCS for CanESM2 and CanESM5 (Fig. 1a). Relative to CanESM2, CanESM5 has a weaker net feedback parameter (−0.64 W m−2 K−1) and higher EffCS (5.65 K), meaning that EffCS has increased by 54 % between CanESM versions 2 and 5. For comparison, we also show the model range of EffCS for both CMIP5 and 6 using horizontal lines below the x axis in Fig. 1a, illustrating the high EffCS in CanESM5 relative to all other CMIP6 models (Flynn and Mauritsen, 2020). Both versions of CanESM exhibit a strong linear relationship between surface temperature and net TOA flux (correlation coefficients are 0.92 and 0.95 for CanESM2 and CanESM5, respectively). For some ESMs, the influence of a time-varying climate feedback parameter, which could be roughly separated into a “fast response” period in the first few decades and a weaker (less negative) feedback over the latter century, had a significant influence on model's EffCS values calculated via the Gregory technique (Andrews et al., 2015). Here, the strong linearity for both versions of CanESM suggests any lack of robustness in the Gregory technique is not a primary cause of the EffCS increase in CanESM5.
We now turn to the different components of the forcing-feedback framework to elucidate any changes in either forcing, or feedback, and their influence on EffCS. We compare the ERF for CanESM2 and CanESM5 via two methods. The ERFg is determined by the y intercept of the Gregory regression plots (filled in circles on the y axis in Fig. 1a). The ERFg is 7.21 and 7.54 W m−2 for CanESM2 and 5, respectively. For comparison, we also show the ERFh as estimated using fixed-SST simulations submitted to RFMIP (open squares). Both methods produce very similar estimates of ERF – within ±5 % – which strongly suggests that the change in EffCS between CanESM2 and 5 is not explained by a change in radiative forcing. We next decompose the net feedback parameter for both models to elucidate the any potential differences in the strength of radiative feedbacks.
3.2 Radiative feedbacks
Planck, lapse rate, water vapour, surface albedo, and cloud TOA feedbacks are shown in Fig. 1b. Planck and lapse rate plus water vapour feedbacks are roughly equal between CanESM2 and CanESM5. The surface albedo feedback is more positive in CanESM5, showing an increase of 0.05 W m−2 K−1 over CanESM2, which is primarily due sea ice loss over the Arctic (Swart et al., 2019b), as well as a consistently more positive snow albedo feedback over polar land surfaces (not shown).
Lastly, cloud feedbacks increase in CanESM5 – primarily in the SW; the result is a more positive net cloud feedback (+0.34 W m−2 K−1 relative to CanESM2). The net feedback (sum of all individual feedbacks) is also shown in Fig. 1b to demonstrate the strong agreement the sum of kernel derived net feedback parameter (filled circles) and the net feedback parameter obtained from the Gregory regression technique (filled triangles). Strong agreement between both methods indicate that kernel ensemble mean is accurately capturing the extent of net TOA flux perturbation as outputted directly from the models.
We find our results are in line with the literature for assessing causes behind similar increases in EffCS observed by many modelling centres participating in CMIP5 and CMIP6 (Flynn and Mauritsen, 2020; Zelinka et al., 2020; Gettelman et al., 2019; Andrews et al., 2019; Golaz et al., 2019). The LW cloud feedback is positive for both versions of CanESM – increasing by 0.06 W m−2 K−1 from CanESM2 to 5 (Fig. 1b). CanESM2 exhibits a negative SW cloud feedback (−0.21 W m−2 K−1), while in CanESM5 the SW cloud feedback has become weakly positive (0.06 W m−2 K−1), indicating an absolute difference of 0.27 W m−2 K−1 (Fig. 1b).
We quantify each individual feedback and forcing change (in terms of EffCS increase) in Table 1. While the SW cloud feedback exhibits the largest difference between CanESM2 and CanESM5, both the surface albedo feedback and the LW cloud feedback offer non-negligible contributions to CanESM5's high EffCS. The SW cloud feedback is the cause of at least half of the EffCS increase from CanESM2 to CanESM5 (1.08 K), followed by the LW cloud and surface albedo feedbacks, respectively. Notably, there is a 3 % error between the kernel-ensemble-derived and model EffCS values (Fig. A1). As a result, we do not consider the small contributions from the Planck and lapse rate plus water vapour changes as they are close to these error bounds (Table 1). Furthermore, despite the strong linear relationship between net TOA radiation and global annual mean surface temperature response for both versions of CanESM (Fig. 1a), the regression-derived ERF model difference is of opposite sign to the ERF difference calculated from fixed-SST experiments (Fig. 1a).
Given the importance of the cloud feedback in explaining the change in EffCS from CanESM2 to 5, we devote the rest of this article to investigating the causes of this change by further decomposing both the SW and LW cloud feedbacks into their altitude, optical depth, and amount components. Although the change in net LW cloud feedback is small, we will demonstrate in the following section that this is due to compensating differences in individual components.
The SW cloud feedback arises due to changes in cloud amount and/or optical properties. Cloud optical thickness is dependent on water path and cloud droplet size distribution (Slingo, 1989). The phase composition of clouds (liquid, ice, or mixed) is linked strongly to their optical thickness due to liquid droplets and ice crystals having different characteristic size distributions, where clouds composed of predominantly smaller liquid droplets tend to be more reflective (Pruppacher and Klett, 1980). As a result, regions where cloud composition consists entirely of liquid droplets (or where clouds are mixed phase) tend to exhibit higher albedo. In terms of feedbacks, cloud phase and amount changes have been identified as an explanatory factor to EffCS spread in ESMs (Tan et al., 2016; Zelinka et al., 2016). Thus, we now decompose the cloud feedbacks using cloud radiative kernels and ISCCP simulator output for each version of CanESM following the methods described in Zelinka et al. (2012a, b) to investigate individual cloud feedback processes. We apply the decomposition separately to low and non-low clouds.
In Fig. 2, we decompose LW and SW cloud feedbacks into contributions from changes in cloud optical depth, cloud altitude, and cloud amount. The LW total cloud feedback is dominated by contributions from non-low clouds (Fig. 2a), with small negative contributions from low clouds (Fig. 2b). Changes in cloud optical depth or amount have little radiative influence for low clouds given low cloud top temperatures are close to that of the surface, resulting in similar outgoing longwave radiation (i.e. little greenhouse effect). Furthermore, particularly in CanESM2, the strong non-low LW feedback is largely offset by a negative SW feedback of comparable magnitude. For CanESM2, contributions to the LW feedback are comparable for optical depth and amount feedbacks – with the largest contribution coming from altitude. The altitude feedback arises from cloud-temperature-dependent emission properties, and therefore operates predominantly in the longwave for non-low clouds. Tropical free troposphere clouds rise and maintain cooler cloud top temperatures relative to the surface, thereby becoming more efficient at trapping outgoing longwave radiation (Zelinka and Hartmann, 2010; Gettelman and Sherwood, 2016). For CanESM5, the net non-low LW feedback is approximately equal to CanESM2, albeit with a different decomposition makeup. Specifically, CanESM5 has a more positive LW altitude and optical depth feedback. However, these increases are offset by a weaker cloud amount feedback. For low clouds, the LW feedbacks are all small in magnitude. The residuals (yellow) are similarly small in both models (Fig. 2), indicating that non-linear processes are less important for understanding the changes between models.
In the SW, both models exhibit strong negative feedbacks for non-low clouds and strong positive feedbacks for low clouds (Fig. 2). The negative non-low-cloud shortwave feedback is driven by an increase in cloud amount and optical depth with warming. This result is consistent with both modelling and theoretical understanding of non-low-cloud responses to warming. Specifically, an increasing number of liquid droplets relative to ice crystals gives rise to more mixed phase clouds, as well as increases the proportion of liquid to ice in existing mixed phase clouds, resulting in an higher optical depth (Senior and Ingram, 1989), and a positive relationship between mid latitude cloud liquid water content and the slope of the moist adiabat as the troposphere warms (i.e. a function of temperature) (Betts, 1987). For low clouds, the SW is dominated by a strong positive amount feedback (decrease in cloudiness), with a small negative contribution from optical depth feedback (increase in cloud optical depth) (Fig. 2b). For CanESM5, SW feedbacks differ from CanESM2 considerably for both non-low and low clouds. For non-low clouds, CanESM5's optical depth feedback is weaker (less negative) than CanESM2 (+0.06 W m−2 K−1) (Fig. 2a). While the SW non-low-cloud amount feedback is also weaker in CanESM5, the difference is offset in the LW. For low clouds, the SW amount feedback exhibits the largest difference between the two model versions (+0.14 W m−2 K−1). The change in SW cloud feedback strength and sign between CanESM2 and CanESM5 is related to multiple feedback mechanisms operating at different cloud heights. The largest contributor is the SW low-cloud amount feedback, which is more positive in CanESM5. Changes in optical depth feedbacks are mainly important for non-low clouds, and are less negative in CanESM5.
The large difference in SW low-cloud feedback strength between CanESM2 and CanESM5 raises the possibility that a portion of what the COSP interprets as a low-cloud response is actually the result of changes in the spatial distribution of non-low-cloud fraction under climate change; a phenomenon known as “obscuration” (Zelinka et al., 2018). Separating for obscuration does not also separate out the amount and optical depth feedbacks. Therefore, we consider the SW unobscured low-cloud feedback as a combination of changes in proportional cloud amount and optical depth. The black bars in Fig. 2b indicate that both CanESM2 and CanESM5 have a non-negligible obscuration term. However, given that the extent of obscuration is similar between both versions of CanESM (see hatched bars in Fig. 2b), it does not appear to be a major contributor to increased feedback strength in CanESM5 relative to CanESM2.
3.2.2 Spatial distribution
Low-cloud amount feedbacks are considered a robust positive feedback mechanism diagnosed from both observational and modelling studies, albeit with substantial inter-model spread in terms of strength (Eitzen et al., 2011; Clement et al., 2009; Zelinka et al., 2016). The low-cloud amount feedback is closely tied to the distribution of marine stratiform cloud regimes persisting in the subtropics and tropics over eastern boundary current ocean regions (Klein et al., 2017). The non-low-cloud optical depth feedback has been shown to have a rich and sometimes offsetting spatial structure, owing to mostly negative feedback at mid-latitudes and high latitudes and a rich zonal structure at low latitudes (Zelinka et al., 2012b, 2016). As such, we now examine the spatial distribution of both the SW low-cloud amount and non-low-cloud optical depth feedbacks (Fig. 3).
Figure 3 shows annual mean SW non-low-cloud optical depth and low-cloud amount feedbacks for CanESM2 and CanESM5. The SW non-low-cloud optical depth feedback is negative in CanESM2 and 5 (Fig. 3a and c), with minima over the western tropical Pacific Ocean. For the SW low-cloud amount feedback, both models are strongest over subtropical and tropical eastern ocean basins and across the equatorial Pacific (Fig. 3b and d). Notably, these regions have persistent low stratiform cloud regimes that are closely tied to the strong temperature inversions that cap the PBL (Klein and Hartmann, 1993).
For CanESM5, increases in SW non-low-cloud optical depth feedback are exhibited throughout the subtropical Pacific and tropical eastern Pacific Ocean (Fig. 3e). While there is strong positive (negative) feedback over the eastern Indian (western Pacific) Ocean, it is offset by a similar strength and opposing sign in the LW (not shown), and thus it does not exert a major influence on the global mean net cloud feedback (LW + SW). For SW low-cloud amount feedback, CanESM5 exhibits an increase over CanESM2 in every region of persistent low-cloud-cover regimes, as well as across the eastern equatorial Pacific and the western Pacific Ocean basin off the Brazilian coast, relating to the simulation of substantially reduced LCC under a warming climate (Fig. 3f).
Multiple lines of evidence from modelling studies have linked the sensitivity of LCC over the oceans to local changes in SST (Zhou et al., 2017; Andrews and Webb, 2018). Furthermore, the evolving spatial pattern of surface warming from interannual to centennial timescales is associated with differences between interannual and long-term cloud feedback strength (Zhou et al., 2015). The underlying physical mechanisms linking local sea surface warming to reduced LCC are (1) increased surface latent heat flux drying and deepening the boundary layer via increased buoyancy-driven turbulence and resultant downward mixing from free troposphere air (Qu et al., 2015; Rieck et al., 2012) and (2) increased surface specific humidity promoting further moisture contrast between the boundary layer and the free troposphere such that when air is mixed downward it is relatively drier (Van der Dussen et al., 2015; Qu et al., 2015). We use a proxy term, SST#, as a measure of distribution of surface warming in the tropics (Fig. 4) (Fueglistaler, 2019). Specifically, SST# is calculated as the difference between the warmest 30 % of tropical SSTs (i.e. the Indo-Pacific) and the tropical average, and therefore this term provides quantitative information about zonal asymmetries in the tropical SST pattern and how they evolve over time.
The pre-industrial control tropical SST pattern for CanESM2 is shown in Fig. 4a and exhibits a familiar zonally asymmetric pattern, with the warmest SSTs in the Indo-Pacific and cooler waters in the eastern Pacific and southeastern regions of each ocean basin. Relative to CanESM2, CanESM5's control SSTs are substantially cooler – by up to 3 K – over the eastern tropical Pacific (Fig. 4b). Colder SSTs are also prevalent in the northern Pacific, off of the western Australian coast, and in the northern tropical Atlantic Ocean (Fig. 4b). There is little difference between the SSTs in the Indo-Pacific, which has important implications for SST#. Figure 4c shows a time series of SST# for abrupt 4×CO2 experiments. Given that SST# represents the difference between the warmest waters in tropics relative to the average, a higher value indicates greater asymmetry between warmer and cooler regions of tropical SST. The relatively cold waters in CanESM5's control climatology results in a larger SST# term, which is also illustrated at the beginning of the abrupt 4×CO2 time series (Fig. 4c). The difference between the models decreases as the climate warms in response to CO2. The higher SST# term at the beginning of the simulation in CanESM5 suggests a stronger SW CRE in the pre-industrial control (Fueglistaler, 2019). The strong positive SW cloud feedback in CanESM5, particularly from low clouds, warms the eastern Pacific (and other cooler areas) at a faster rate than CanESM2 (Fig. 3f), which gradually decreases the difference in SST# over the course of the abrupt 4×CO2 simulation (Fig. 4c). While the distribution of surface warming in the tropics is known to be important for low clouds (Andrews and Webb, 2018), we also briefly analyze another important controlling factor: estimated inversion strength (EIS) (Fig. 5).
Figure 5 shows EIS for both the control climatology and response abrupt 4×CO2 simulations and is calculated using air temperatures at the surface and 700 hPa as in Wood and Bretherton (2006). Regions with a strong positive EIS are indicative of a boundary layer that is decoupled from the free troposphere, with strong subsidence and cooler SSTs and therefore more low-cloud fraction. Conversely, a strong negative EIS is indicative of a weak inversion and a surface that is coupled tightly to the free troposphere (i.e. unstable vertical temperature profile) and is therefore inefficient at trapping moisture within the boundary layer. In the CanESM2 control period, EIS is strongly positive across all eastern ocean basins and the eastern equatorial Pacific (Fig. 5a). In CanESM5, control EIS mirrors the corresponding SST pattern (Figs. 5b, 4b). In the response period, EIS increases throughout most of the tropics for both models (Fig. 5c and d). CanESM5 exhibits a stronger increase in EIS throughout most of the tropics relative to CanESM2. Given that EIS and low-cloud fraction are strongly positively correlated (Wood and Bretherton, 2006), a stronger response (as seen in CanESM5) would promote more cloud fraction if it were the only cloud controlling factor. However, we find no clear relationship between regions of more positive SW low-cloud feedback and increased inversion strength response (Fig. 5d). Inferring causal changes in cloud feedbacks between models from EIS alone is difficult given its correlation with SSTs (Scott et al., 2020) (see Figs. 4b and 5b). We now turn towards prescribed SST experiments from CFMIP6 to further investigate the role of SST warming distribution as a cloud controlling factor.
3.3 Prescribed SST experiments
To investigate the spatial pattern of surface warming and its influence on SW cloud feedbacks, we present results from an additional experiment from the CFMIP Tier 2 experiment deck – AMIP-piForcing (Webb et al., 2017). The AMIP-piForcing experiment forces the atmosphere model with the reconstructed historical SSTs and sea ice boundary conditions from 1870 to 2014 (Hurrell et al., 2008). An important distinction from the base AMIP experiment is the anthropogenic and natural atmospheric forcings are held fixed to their pre-industrial control levels in AMIP-piForcing, which allows for a more direct comparison to abrupt 4×CO2 experiments, as it removes the influence of non-SST mediated cloud responses. Thus, using AMIP-piForcing, we can isolate the contribution to changes in cloud feedbacks that arises due to changes in the atmosphere model (CanAM4 to CanAM5) independent of the change to the ocean model (NCAR CSM to CanNEMO). We show global mean low-cloud feedbacks and SST# time series for both the AMIP-piForcing and abrupt 4×CO2 CanESM5 experiments in Fig. 6.
For low clouds, the SW feedback is stronger (+0.21 W m−2 K−1) in the abrupt 4×CO2 experiment than AMIP-piForcing – largely due to the cloud amount feedback, but there is also a smaller contribution from the optical depth feedback (Fig. 6a). This result is consistent with theoretical understanding relating warmer local SSTs to reduced boundary layer marine cloud cover as outlined in the previous section, which is further emphasized by the geographic distribution of warming in the AMIP-piForcing experiment (Fig. 6b). In AMIP-piForcing, the eastern Pacific warms only by a small amount relative to the abrupt 4×CO2 experiment (Fig. A4), which is exemplified by the SST# time series. Furthermore, the SST# trend is opposite in AMIP-piForcing, illustrating the warming in the Indo-Pacific warm pool over the historical record (Fig. A4), which is not present in coupled model abrupt 4×CO2 experiments (Andrews et al., 2018).
We summarize feedback results from all experiments considered in this study in Table 2. The Planck response is nearly identical for all three experiments. The combined lapse rate and water vapour feedback is similar in abrupt 4×CO2 experiments for both models, but it is noticeably more negative in the AMIP-piForcing experiment. The combined result is a product of the more negative lapse rate feedback, which arises due to the relatively stronger warming in the Indo-Pacific warm pool (Andrews et al., 2018) from the reconstructed SST data set used as forcing (Hurrell et al., 2008). Surface temperatures in the deeply convective warm pool increase Earth's emission temperature via enhanced latent heat release, which stabilizes the vertical temperature profile and warms the upper troposphere. Outgoing longwave radiation increases and produces a strong radiative cooling effect. The surface albedo feedback is stronger in the CanESM5 for coupled model experiments, but it is reduced in AMIP-piForcing relative to CanESM5's abrupt 4×CO2 experiment, which is likely a result of the constrained sea ice boundary conditions present. The longwave cloud feedback is similar across all three experiments and models, and the SW cloud feedback has strongly increased in CanESM5 for coupled experiments but is reduced to a similar magnitude to CanESM2 abrupt 4×CO2 in the AMIP-piForcing experiment. The net feedback result for the AMIP-piForcing experiment is strongly negative in CanESM5 relative to abrupt 4×CO2, which is due to the combined effect of reduced surface albedo, SW cloud, and lapse rate feedbacks.
In this study, we have analyzed both forcing and feedback in idealized experiments with instantaneous quadrupling of atmospheric CO2 (abrupt 4×CO2) using two versions of CanESM to elucidate the underlying cause behind CanESM5's increased EffCS (5.65 K). Using radiative kernels and output from RFMIP, we find only modest differences in both forcing and non-cloud feedbacks, with a small contribution from a slight increase in the surface albedo feedback. The largest difference in feedback strength between CanESM2 to CanESM5 is from the cloud feedback, particularly in the SW. Further breakdown of the cloud feedback into its individual components (optical depth, altitude, and amount) at distinct cloud top heights (<680 hPa for non-low and ≥680 hPa for low) revealed that the SW low-cloud amount and non-low-cloud optical depth feedbacks are the dominant contributor to CanESM5's increased EffCS (+0.14 and 0.06 W m−2 K−1, respectively) in abrupt 4×CO2 simulations. Analysis of the spatial pattern for each feedback showed the largest model differences in SW low-cloud amount feedback over subtropical eastern ocean basins and across the equatorial Pacific Ocean and in SW non-low-cloud optical depth feedback over the subtropical and extratropical Pacific Ocean.
We analyzed the spatial pattern of surface warming and its influence on the SW low-cloud feedback using the CFMIP tier 2 AMIP-piForcing experiment in CanESM5, which exhibited significantly reduced SW cloud feedback due to the lack of local warming in regions with persistent low-cloud cover – in agreement with studies linking warmer (colder) SSTs to decreased (increased) LCC (Qu et al., 2014; Bretherton and Blossey, 2014; Brient and Schneider, 2016). We found a similar strength in LW cloud feedback from both the abrupt 4×CO2 and AMIP-piForcing experiments and a reduced lapse rate feedback in the AMIP-piForcing experiment due to the relatively strong surface warming in the Indo-Pacific warm pool. While lacking an analogous AMIP-piForcing experiment for CanESM2, the results presented here agree with similar experiments conducted using other ESMs (i.e. more negative lapse rate and SW cloud feedback) that have been studied with respect to pattern effects of warming (Andrews et al., 2018). Furthermore, the SW cloud feedback strength in the CanESM2 abrupt 4×CO2 experiment is equal to that of the CanESM5 AMIP-piForcing experiment despite a different pattern effect of warming (Figs. 4a and 6b). The AMIP-piForcing results presented here confirm the well-documented relationship between local SSTs as a controlling factor for low clouds. This result suggests that both the pattern of warming itself and the sensitivity of low-cloud fraction to this pattern play a key role in CanESM5's higher EffCS. Disentangling the role of the ocean model replacement (The National Centre for Atmospheric Research CSM ocean model for CanESM2 (Gent et al., 1998) to CanNEMO for CanESM5 (Swart et al., 2019b)) and the developmental changes to cloud microphysics in CanAM5 (e.g. the new autoconversion scheme and aerosol indirect effect) is a subject for future work.
Our results add further evidence the recent trend of several ESMs participating in CMIP6 exhibiting higher EffCS than their CMIP5 counterpart – predominantly due to changes in SW cloud feedback strength and/or aerosol–cloud interactions (Gettelman et al., 2019; Andrews et al., 2019; Bodas-Salcedo et al., 2019). However, it is worth noting that several modelling centres report increased EffCS sourced from distinct developments in newer versions of their respective model (e.g. addition of a mixed-phase cloud scheme and improved aerosol–cloud interactions), as well as the higher horizontal ocean model resolution and its influence on SSTs in cold upwelling regions, in HadGEM3 (Bodas-Salcedo et al., 2019; Mulcahy et al., 2018; Andrews et al., 2019).
Finally, we emphasize that the results presented in this study do not seek to comment on the plausibility of climate sensitivity from either version of CanESM. Recently, there has been an expansion of work relating constraints on climate sensitivity through the use of the satellite and paleoclimate observational records (Sherwood et al., 2020). Furthermore, there are limitations when interpreting the validity of climate sensitivity results (as calculated here) due to uncertainties associated with statistical methods (e.g. assuming a time-invariant climate sensitivity parameter via the regression approach) (Gregory et al., 2004). However, we reiterate the scope of this study: establishing a causal link for the increased climate sensitivity from CanESM2 to CanESM5 under long-term, idealized climate change.
All model output from both versions of the Canadian Earth System Model analyzed in this study are publicly available for download via the Earth System Grid Federation (https://doi.org/10.22033/ESGF/CMIP6.1303, Swart et al., 2019c). The particular model version (5.0.3) that contributed output to CMIP6 is available from https://doi.org/10.5281/zenodo.3251113 (Swart et al., 2019a). Code used for analysis of model output and production of figures is located at https://github.com/JohnVirgin/GMD_CanESM_Clouds (last access: 27 August 2021).
JGV performed analysis on model output and created all figures used in this study. JGV, CGF, JNSC, KvS, and TM wrote the manuscript.
The authors declare that they have no conflict of interest.
Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
The authors acknowledge Mark Zelinka, Neil Swart, and Nathan Gillet for providing useful insights and comments that helped improve this study. The authors also acknowledge the World Climate Research Programme's (WCRP) Working Group on Coupled Modelling (WGCM) and the Earth System Grid Federation (ESGF) for their role in providing access to the data used in this study.
This paper was edited by Axel Lauer and reviewed by two anonymous referees.
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