Evaluating and improving the treatment of gases in radiation schemes: the Correlated K-Distribution Model Intercomparison Project (CKDMIP)
Most radiation schemes in weather and climate models use the “correlated k distribution” (CKD) method to treat gas absorption, which approximates a broadband spectral integration by N pseudo-monochromatic calculations. Larger N means more accuracy and a wider range of gas concentrations can be simulated but at greater computational cost. Unfortunately, the tools to perform this efficiency–accuracy trade-off (e.g. to generate separate CKD models for applications such as short-range weather forecasting to climate modelling) are unavailable to the vast majority of users of radiation schemes. This paper describes the experimental protocol for the Correlated K-Distribution Model Intercomparison Project (CKDMIP), whose purpose is to use benchmark line-by-line calculations: (1) to evaluate the accuracy of existing CKD models, (2) to explore how accuracy varies with N for CKD models submitted by CKDMIP participants, (3) to understand how different choices in the way that CKD models are generated affect their accuracy for the same N, and (4) to generate freely available datasets and software facilitating the development of new gas-optics tools. The datasets consist of the high-resolution longwave and shortwave absorption spectra of nine gases for a range of atmospheric conditions, realistic and idealized. Thirty-four concentration scenarios for the well-mixed greenhouse gases are proposed to test CKD models from palaeo- to future-climate conditions. We demonstrate the strengths of the protocol in this paper by using it to evaluate the widely used Rapid Radiative Transfer Model for General Circulation Models (RRTMG).
Despite being fundamental for climate projections, there are still substantial differences in estimates of the radiative impact of greenhouse gases between the climate models used by the Intergovernmental Panel on Climate Change. For example, Soden et al. (2018) showed that the inter-model spread in radiative forcing due to increased CO2 is around 35 % of the mean, a figure that has remained unchanged for nearly 3 decades. DeAngelis et al. (2015) reported an even greater spread in estimates of the sensitivity of shortwave atmospheric absorption to water vapour concentration, a spread responsible for much of the uncertainty in future changes to global-mean precipitation. Collins et al. (2006) compared calculations from climate-model radiation schemes and six line-by-line (LBL) radiation models, finding that the spread in H2O and CO2 radiative forcing estimates was 5–6.5 times less between the LBL models than between the climate models. We conclude that errors in climate-model radiation schemes cannot be blamed primarily on our lack of knowledge of the spectroscopy of greenhouse gases; rather, there must be a problem in the fast algorithms that attempt to mimic the results of expensive LBL calculations. The need to improve these algorithms is one of the main motivations for the intercomparison proposed in this paper.
The gas absorption spectra of planetary atmospheres typically contain hundreds of thousands of spectral lines, so LBL radiative transfer calculations require O(106–107) monochromatic calculations to cover the full shortwave and longwave spectrum, which is far too costly for most applications. The correlated k distribution (CKD) method (e.g. Goody et al., 1989; Lacis and Oinas, 1991; Petty, 2006) underpins most modern radiation schemes in weather and climate models; it avoids the need to resolve spectral lines by reordering the mass absorption coefficient, k(ν), over a particular range of wavenumbers, ν, such that the resulting function k(g) increases smoothly and monotonically from the least absorbing (g=0) to the most absorbing (g=1). The smooth function k(g) may be discretized using far fewer quadrature points than k(ν), with the result that the entire shortwave and longwave spectrum can be represented by O(102) independent pseudo-monochromatic calculations, usually referred to as k terms or g points. In order to perform radiation calculations over the full atmospheric column, we typically need to assume perfect rank correlation between the k spectra at each height. The CKD method has the advantage over random-band models that it is easy to incorporate scattering.
The more k terms we use to discretize the k(g) function, the greater the accuracy we should expect, but at a larger computational cost. Therefore, we have a trade-off to make depending on the application. For climate modelling we require schemes that can accurately compute the radiative forcing of a number of different greenhouse gases over a wide range of concentrations. By contrast, for short-range weather forecasting with present-day greenhouse gas concentrations, the priority is much more on efficiency: the radiation scheme must be called frequently to capture the local radiative impact of evolving cloud fields, and forecasts must be delivered to customers in a timely fashion. The lower model top in many limited-area weather models also means that, in principle, fewer k terms are required to compute the heating-rate profile. The priorities may be different in other applications of CKD models, such as offline calculations to interpret observations (e.g. Loeb and Kato, 2002), computing the 3D radiative effect of clouds (e.g. Chen and Liou, 2006; Jakub and Mayer, 2016) and providing accurate reference spectra (e.g. Anderson et al., 1999).
Unfortunately, the tools and know-how to generate new CKD models and to make this accuracy–efficiency trade-off are available to only a handful of specialists worldwide, with the result that most atmospheric models are available with only one gas-optics configuration, which is often not optimized for the application at hand. Indeed, Hogan et al. (2017) surveyed seven models used for the same application of global weather forecasting and reported that the total number of k terms (shortwave plus longwave) ranged from 68 to 252.
The purpose of the Correlated K-Distribution Model Intercomparison Project (CKDMIP) is to address these issues. First in CKDMIP we will use benchmark LBL calculations to evaluate the accuracy of existing CKD models, followed by the main part of the project in which CKDMIP participants generate new CKD models with different numbers of k terms targeting applications including short-range weather forecasting and climate modelling. By providing participants with common datasets of high spectral-resolution gas absorption, we hope to avoid differences due to inconsistent spectroscopy, enabling the results to be interpreted purely in terms of the algorithms used by each CKD tool. Two different band structures are proposed for them to use. The accuracy versus number of k terms will be computed for each submission, and the results compared to understand how different techniques for constructing CKD models affect their accuracy for the same number of k terms. Participants include the developers of numerous CKD tools, e.g. those described by Edwards and Slingo (1996), Kato et al. (1999), Zhang et al. (2003), Sekiguchi and Nakajima (2008), Hogan (2010), Doppler et al. (2014), André et al. (2018), and Pincus et al. (2019). Finally, it is hoped that the freely available CKDMIP datasets and software will facilitate the development of community tools to allow users to generate their own gas-optics models targeted at specific applications.
The project has similarities to the Radiative Forcing Model Intercomparison Project (RFMIP; Pincus et al., 2016), which used LBL calculations to evaluate the radiation schemes of a number of climate models in terms of surface and top-of-atmosphere (TOA) irradiances for a range of atmospheric profiles and climate scenarios. However, CKDMIP goes further in that it includes the weather forecasting application and provides the means to improve the way that CKD schemes make the trade-off between accuracy and efficiency. This is possible by making available the spectral optical depth of each layer of the atmosphere due to each gas separately. The CKDMIP software package allows participants to combine and scale the optical depths of the gases they are interested in and perform LBL radiative transfer calculations on the result, producing their own reference profiles of spectral or broadband irradiances and heating rates.
This protocol paper describes the design and generation of these datasets and software and what comparisons will be performed. Section 2 describes the overarching design decisions of CKDMIP, including which gases to include, which weather and climate applications to target and, for climate modelling, which range of gas concentrations to consider. Section 3 describes in detail how the datasets are produced, how the spectral resolution has been chosen, and what radiative transfer calculations are performed. Section 4 then describes what is required of CKDMIP participants, the spectral band structures that should be used, the metrics that will be used to quantify errors in irradiances and heating rates, and how errors due to the representation of the spectral variation in cloud properties will be assessed. Section 5 demonstrates the use of the dataset to evaluate an existing, widely used CKD model.
Finally, a note on terminology. Throughout this paper we define a CKD scheme as a software component (usually embedded within the radiation scheme of an atmospheric model) that takes as input profiles of atmospheric temperature, pressure, and the concentrations of a number of gases and that outputs profiles of optical depth for each of a number of k terms. It also includes a means to compute the Planck function to use for each longwave k term and the TOA solar irradiance for each shortwave k term. A CKD model is one configuration of a CKD scheme with a particular number of k terms, which might consist of a set of look-up tables that can be used by the CKD scheme. A CKD tool is a method (which may be fully automated or involve some hand-tuning) for generating individual CKD models, with some means to control the tradeoff between accuracy and the number of k terms.
2.1 Which gases?
The absorption spectra of nine gases are considered in CKDMIP in both the longwave and the shortwave: H2O, O3, O2, N2, CO2, CH4, N2O, CFC-11, and CFC-12. The first two have very variable concentrations and are important in both the longwave and the shortwave. The concentrations of the second two gases may be treated as fixed both spatially and over the timescales commonly considered by climate models. O2 is important mainly in the shortwave but reduces outgoing longwave radiation (OLR) by around 0.11 W m−2 globally (Höpfner et al., 2012). Absorption by N2 is ignored by most operational radiation schemes, yet it reduces OLR by around 0.17 W m−2 (Höpfner et al., 2012) and, as will be shown in Sect. 3.6, has a comparable effect in the shortwave. The concentrations of N2 and O2 are also needed to compute the collision-induced contribution to the continuum absorption and the broadening efficiency of these molecules, where applicable.
The final five gases listed above are well-mixed greenhouse gases with a significant anthropogenic component. There is a much larger number of greenhouse gases that could have been included, many of which have a very small individual impact. However, the purpose of CKDMIP is to evaluate the techniques used by schemes for generating CKD models based on the different requirements of weather and climate modelling rather than to produce a single optimum CKD model that explicitly represents all the greenhouse gases that anyone might want to simulate. Therefore, we have chosen to follow the pragmatic approach of Meinshausen et al. (2017). They stated that 94.5 % of the anthropogenic greenhouse warming (in terms of radiative forcing) between 1750 and 2014 was due to increases in CO2, CH4, N2O, CFC-11, and CFC-12, with the remaining 5.5 % being attributable to 38 further gases. Their “Option 2” approximately represents the radiative forcing of these 38 gases by artificially increasing the concentration of CFC-11 (by around a factor of 3.9 in the present day), and the CMIP6 (Coupled Model Intercomparison Project Phase 6) historic concentrations and future scenarios are available with these “CFC-11-equivalent” concentrations. From Cycle 47R1, ECMWF's Integrated Forecasting System has taken this approach, using concentrations from the CMIP6 SSP3-7.0 scenario (O'Neill et al., 2016), where “SSP3-7.0” is the “regional rivalry” shared socioeconomic pathway of CMIP6 with an anthropogenic radiative forcing of 7.0 W m−2 in 2100.
2.2 Numerical weather prediction
Table 1 lists the three main applications for which we envisage that CKD models could be optimized. The first two correspond to present-day numerical weather prediction (NWP) at the local and global scale. Both need to represent variable water vapour, and ozone but to a good approximation can assume all other gases to have a constant mole fraction or to vary as a function of pressure alone. (Note that since the atmosphere is an ideal gas to a good approximation, we can assume the mole fraction of a gas to be equal to its volume mixing ratio.) In principle, this allows the number of k terms to be reduced since, for example, all the well-mixed gases could be merged into a single “hybrid” or “composite” gas whose optical properties vary as a function of temperature and pressure alone (e.g. Ritter and Geleyn, 1992; Niemelä et al., 2001).
In terms of the present-day concentrations of the well-mixed gases, we assume that O2 and N2 have constant dry-air mole fractions of 0.20946 and 0.78102 mol mol−1, respectively, independent of pressure (Jones and Schoonover, 2002). These concentrations are also assumed for all past and future scenarios in Sect. 2.3. The present-day surface concentrations of the five other well-mixed gases are shown in Table 2 and were taken from the CMIP6 SSP3-7.0 scenario for calendar year 2020. The vertical profiles of these gases are discussed in Sect. 3.2.
The difference between the two NWP applications listed in Table 1 is in the location of the model top. The model top quoted for all current configurations of the ECMWF model and all global configurations of the Met Office model used for weather and climate is 0.01 hPa (around 80 km). In the case of the ECMWF model this actually means that the highest model layer spans the pressure range 0–0.02 hPa. Since the temperature of the highest layer of a model is strongly affected by the “sponge” (Shepherd et al., 1996), we limit evaluation of heating rates to pressures greater than 0.02 hPa. For the limited-area NWP application we evaluate heating rates only for pressures greater than 4 hPa, comparable to the model top used in the Met Office high-resolution UK model.
All heating-rate calculations in CKDMIP make the assumption of local thermodynamic equilibrium (LTE), which becomes invalid in the mid-mesosphere and above. Parameterizations of non-LTE heating rates in the upper atmosphere are typically blended with heating rates from a CKD model assuming LTE; for example, Fomichev et al. (1998) blended smoothly between the two over the pressure range 0.016–0.045 hPa. Therefore, in CKDMIP it is appropriate to evaluate heating rates assuming LTE to a pressure of around 0.02 hPa, but we should be aware that for the most accurate results in an atmospheric model, these heating rates would need to be blended with those from a non-LTE scheme at pressures lower than around 0.045 hPa.
2.3 Climate modelling
CKD models used for climate modelling should be able to simulate a wide range of greenhouse gas concentrations. The first four lines of Table 2 list individual scenarios that will be tested. They include present-day and preindustrial conditions, plus the conditions at a glacial maximum, with the values for CO2 and CH4 taken from Petit et al. (1999) and for N2O from the shorter period reported by Schilt et al. (2010). The fourth row shows a “future” scenario consisting of worst-case conditions for 2110 by extracting the maximum concentrations from any of the CMIP6 scenarios at this time. In this year, the concentration of CH4 peaks at 3500 ppbv in the SSP3-7.0 scenario, and equivalent CFC-11 peaks at 2000 pptv in the SSP5-8.5 scenario.
Scenarios 5–22 in Table 2 show the range of concentrations that will be used in testing the radiative effect of individual gases, keeping all others constant. For each gas we require the capability to simulate the minimum concentrations found in the last million years, which occurred at glacial maxima, up to the maximum concentrations found in any of the CMIP6 future scenarios, which extend until 2250. In the case of CO2 we consider concentrations ranging up to 8 times preindustrial ones. These ranges are very similar to those considered by Etminan et al. (2016). Scenarios 19–22 concern CFC-11 and CFC-12, but as will be shown from LBL calculations in Sect. 3.6, the magnitude of their instantaneous TOA and surface shortwave radiative forcing is less than 0.002 W m−2, so these scenarios are used only for longwave evaluation.
Etminan et al. (2016) reported that due to the overlap of the absorption spectra of CO2, CH4 and N2O, the longwave radiative forcing associated with changing the concentration of one of these gases can depend on the concentration of the other two. To test the ability of CKD models to simulate this effect, the final 12 scenarios in Table 2 perturb the concentrations of pairs of these gases to their extreme values, while keeping the others at present-day concentrations. These scenarios are also only for longwave evaluation since we calculate that overlap effects change shortwave TOA forcings only of the order of 0.001 W m−2.
In principle, there are important applications in addition to those shown in Table 1, such as atmospheric reanalysis, which have been generated back to the mid-19th century (e.g. Compo et al., 2011). A CKD model targeted at this application would only need to span greenhouse gas concentrations from preindustrial to present-day ones. We decided not to include this application in CKDMIP, partly not to overload the participants but also because of the expectation that the number of k terms required would not be very different between the reanalysis and climate modelling applications.
Table 3 lists the four CKDMIP datasets. Each consists of profiles of layer-wise spectral optical depth due to individual gases. The first two (Evaluation-1 and Evaluation-2) each consist of 50 realistic profiles of temperature, water vapour and ozone (described in Sect. 3.1), accompanied by vertical profiles of the well-mixed gases (described in Sect. 3.2). Evaluation-1 is provided to participants and may be used to train individual CKD models, while Evaluation-2 is held back to provide independent evaluation. Section 3.3 describes the last two datasets, which could also be useful in the training of new CKD models. Section 3.4 then describes how the profiles of spectral optical depth were computed for each dataset. Section 3.5 describes the radiative transfer calculations performed on these absorption spectra, an example of which is given in Sect. 3.6 where we estimate the longwave and shortwave radiative importance of each of the seven well-mixed gases.
3.1 Temperature, humidity and ozone
For evaluating radiation schemes in RFMIP, Pincus et al. (2016) extracted a set of 100 contrasting atmospheric profiles from the 60-layer ERA-Interim reanalysis dataset, whose highest model level spans the pressure range 0–0.2 hPa. As well as being 10 times greater than the pressure of the highest model level in the current ECMWF and Met Office global models, this vertical grid is not sufficient to fully resolve the strong peak in atmospheric heating and cooling rates that occurs at the stratopause nor to test solar absorption by carbon dioxide in the mesosphere.
Therefore, we have selected a new set of temperature, pressure, humidity, and ozone profiles from the 25 000 NWP-SAF (Numerical Weather Prediction Satellite Application Facility) profiles of Eresmaa and McNally (2014), which they extracted from ECMWF operational model forecasts in 2013 and 2014. By this time the model used 137 layers with the highest layer spanning pressures 0–0.02 hPa, as in its current configuration. As in the ECMWF operational model, CKDMIP assumes a hydrostatic atmosphere, in which case the mass of a layer is defined purely from the pressure at the layer interfaces and the acceleration due to gravity.
The 50 profiles of the Evaluation-1 dataset consist of 33 randomly taken from the NWP-SAF dataset. An additional 17 profiles are selected to contain the extreme values (both maximum and minimum) in the entire dataset of (a) temperature in the layer nearest the surface, (b) temperature at 400 hPa, (c) temperature at 100 hPa, (d) temperature at 10 hPa, (e) temperature at 1 hPa, (f) specific humidity at 400 hPa, (g) specific humidity at 100 hPa (maximum only), (h) ozone concentration at 10 hPa, and (i) ozone concentration at 1 hPa.
The Evaluation-2 dataset, intended to provide independent evaluation of the CKD models, uses a different set of 33 random profiles from the NWP-SAF dataset, along with 17 profiles containing the extreme values at different levels from those used by Evaluation-1, specifically (a) temperature where the pressure falls to 90 % of its surface value, (b) temperature at 200 hPa, (c) temperature at 50 hPa, (d) temperature at 5 hPa, (e) temperature at 0.5 hPa, (f) specific humidity at 200 hPa, (g) specific humidity at 50 hPa (maximum only), (h) ozone concentration at 5 hPa, and (i) ozone concentration at 0.5 hPa.
It was apparent from an inspection of the data that there was virtually no variability in stratospheric water vapour in the ECMWF model at the time the NWP-SAF profiles were generated, which is a problem for training and evaluating a gas-optics model. Therefore, additional variability has been added by multiplying the humidity profiles by the following function of pressure, p:
where r is a random number drawn from a normal distribution with mean of zero and standard deviation 0.25 and is constant for each individual profile. This function adds around 25 % variability in the stratosphere and mesosphere but leaves the troposphere virtually unchanged. Unrealistically low humidities have been removed by setting the minimum specific humidity to 10−7 kg kg−1. The resulting temperature, humidity, and ozone mixing ratios in the Evaluation-1 dataset are shown by the red and blue lines in Fig. 1.
Training and evaluating a CKD model is costly both in terms of computation and storage due to the high spectral resolution required, and 137 layers is more than needed for evaluating clear-sky radiative transfer. Therefore, we interpolate the profiles on to a coarser grid with 54 layers. We use the Line-By-Line Radiative Transfer Model (LBLRTM; Clough et al., 2005), version 12.8, which takes as input the temperature, pressure, and gas concentrations at the interfaces between layers. The highest two layers of the coarser grid are bounded by pressures of 0.0001, 0.01, and 0.02 hPa; the first of these pressures represents TOA since LBLRTM cannot compute gas properties at zero pressure. As shown in Table 1, the pressure surfaces 0.02 and 4 hPa mark the point at which evaluation of heating rates begins. We assign 15 layers between these two pressure surfaces, with the interfaces between them spaced linearly in p0.15 space. The pressures defining the remaining layers vary according to the surface pressure ps: we assign 35 layers between 4 hPa and ps∕1.005, again spaced linearly in p0.15 space. Finally, a further two layers are added very close to the surface (bounded by ps∕1.005, ps∕1.002, and ps) in order to resolve sharp temperature gradients in the surface layer. The black dots in Fig. 1 mark the corresponding interfaces between layers for the median profiles described in Sect. 3.3.
3.2 Well-mixed gases
Many weather and climate models assume a spatially constant mole fraction for each of the well-mixed gases, whereas for a little more realism they should decrease with height. The radiation scheme in the ECMWF model uses climatologies of these gases that vary with month, latitude, and pressure, with the CO2 and CH4 climatologies taken from the MACC (Monitoring Atmospheric Composition and Climate) analysis system (Inness et al., 2013) and the N2O, CFC-11, and CFC-12 climatologies from the Cariolle chemistry model (Bechtold et al., 2009). Long-term changes due to anthropogenic emissions are represented by scaling these fields so that the global-mean surface values match either historic measurements (for hindcasts and reanalysis) or the CMIP6 SSP3-7.0 scenario (for operational forecasts from model cycle 47R1). We have averaged these climatologies globally and annually and scaled them to the 2020 surface values in SSP3-7.0, to obtain the profiles shown in Fig. 2. Present-day CO2 has a difference of 10 ppmv between the values at 1000 and 0.01 hPa. In the case of CFC-11 and CFC-12, the concentrations from the Cariolle model drop to almost zero in the upper stratosphere and mesosphere, which could be problematic for using them to train the pressure dependence in a CKD model. Therefore, the profiles of these two gases have been artificially modified to fall to no less than 5 % of their surface value. In order to obtain profiles with the surface concentrations shown in Table 2, we simply scale the profiles shown in Fig. 2.
We have computed that the difference in the instantaneous TOA longwave radiative forcing of a gas with a constant mole fraction with pressure, versus the more realistic profiles in Fig. 2 but the same surface concentration, is 10 % for CFC-11, 5 % for CFC-12, and less than 0.2 % for the other three gases.
3.3 Additional training datasets
Two additional datasets are shown at the bottom of Table 3, which are intended to facilitate the development of CKD schemes, while being consistent with the datasets that will be used to evaluate them. The MMM dataset contains the optical properties of all nine gases but using the median, minimum, and maximum temperature profiles derived from the entire 25 000-profile NWP-SAF dataset; these temperatures are shown by the black lines in Fig. 1. In the case of H2O and O3 only, three concentration profiles are used for each temperature, corresponding also to the median, minimum, and maximum of the NWP-SAF profiles (shown in Fig. 1b and c). For all other gases the present-day concentrations shown in Fig. 2 are used. The vertical grid is the same as for the Evaluation-1 and Evaluation-2 datasets, except that surface pressure is set to mean sea level pressure (ps=1013.25 hPa), and the two layers very close to the surface are not used so that the total number of layers is 52 rather than 54.
The final Idealized dataset contains absorption spectra for idealized temperature and concentration profiles that are intended to cover the full range of likely temperature, pressure and concentrations found in the atmospheres that any CKD model would be applied to. Therefore, they can be used to populate look-up tables of molar absorption to be used by CKD models. We envisage that the maximum layer-mean pressure that needs to be accommodated by a radiation scheme is 1100 hPa, so we construct a logarithmically spaced pressure profile of 53 elements, containing 10 points per decade with a maximum layer-mean pressure of 1100 hPa. At each pressure, six temperatures are simulated spanning a 100 K range at 20 K intervals. We use idealized temperature profiles shown in Fig. 3 that are intended to encompass the maximum and minimum temperatures found in the NWP-SAF dataset. For all gases, absorption spectra are computed for mole-fraction profiles that are constant with pressure, using the present-day values for the five well-mixed gases shown in Table 2 and 5 ppmv for O3. Since the molar absorption of these gases is very close to constant with concentration (see Sect. 3.4), only one concentration needs to be simulated for each. In the case of water vapour whose absorption varies with concentration, we simulate 12 logarithmically spaced specific humidities from 10−7 to 10−1.5 kg kg−1, i.e. using two values per decade.
During the course of the project it may become clear that further LBL datasets are required, in which case they will be designed and generated in consultation with the participants. This could arise if some CKD tools are unable to use the CKDMIP datasets, and we suspect that errors are due to inconsistent spectroscopy rather than the CKD algorithms themselves. For example, if it is apparent that CKD schemes differ in their treatment of water vapour, then this could be quantified using a set of profiles in which water vapour alone was perturbed.
3.4 Line-by-line modelling
The spectral optical depths of the individual gases have been computed using version 12.8 of LBLRTM (Clough et al., 2005) developed at Atmospheric & Environmental Research (AER). LBLRTM incorporates the self- and foreign-broadened water vapour continuum via the Mlawer–Tobin–Clough–Kneizys–Davies (MT_CKD) continuum model, version 3.2 (Mlawer et al., 2012). Continua for CO2 and for the collision-induced bands of O2 and N2 are also included in the computations. Line coupling for CO2 is treated as first order with coefficients computed as specified by Lamouroux et al. (2015). It should be noted, however, that line coupling coefficients for the 30012←00001 and 30013←00001 bands of the main isotopologue (at 6348 and 6228 cm−1, respectively) have been calculated from the tridiagonal relaxation matrix parameters of Devi et al. (2007a, b). The spectroscopic input parameters have been taken from the AER line parameter database, version 3.6, which is largely drawn from HITRAN 2012 (Rothman et al., 2013) but with AER customized modifications, most notably for H2O, CO2, and O2. The AER line parameters for CH4 include line coupling parameters for the ν3 (3000 cm−1) and ν4 (1300 cm−1) bands of the main isotopologue.
Rather than defining radiation as “longwave” or “shortwave” depending on whether its wavenumber is less than or greater than some specific value, we define the longwave as any radiation originating from emission by the surface or atmosphere and shortwave as any radiation originating from the sun. The longwave spectrum is taken to span the wavenumber range 0–3260 cm−1, which covers 99.997 % of the Planck function at 0 ∘C and 99.971 % at +50 ∘. The shortwave spectrum is taken to span the range 250–50,000 cm−1 (0.2–40 µm), which misses only 0.012 W m−2 of the solar irradiance at wavenumbers less than 250 cm−1 and 0.103 W m−2 at wavenumbers greater than 50 000 cm−1. These ranges are shown in Fig. 4a and b, while panel c shows the spectral absorption of the nine gases at 100 hPa for the “median” profile of the MMM dataset using present-day concentrations of the well-mixed gases.
An important practical consideration is to determine at what spectral resolution to produce the absorption spectra. They need to be of a fine enough resolution that the most narrow spectral lines are resolved and the resulting irradiance and heating-rate profiles are an accurate benchmark but also a manageable data volume for storage, processing, and distribution. LBLRTM can inform the user of the spectral resolution it needs to resolve the lines at a particular pressure, and for CO2 in the longwave at 0.01 hPa (the most important gas at the pressure where the lines are finest), it recommends a wavenumber resolution such that more than 20 million spectral points are required. Using this resolution as a reference, we have experimented with degrading the spectral resolution in four spectral ranges bounded by the wavenumbers 0, 350, 1300, 1700, and 3260 cm−1. Computing the heating-rate error for each spectral range leads us to adopt spectral resolutions of 0.0002, 0.001, and 0.005 cm−1 in the three spectral ranges 0–1300, 1300–1700, and 1700–3260 cm−1, respectively. This leads to heating-rate errors of no more than around 0.005 K d−1 (all of which occur in the upper stratosphere and mesosphere) in any of the four original wavenumber ranges, even for the most challenging scenario of 8 times the preindustrial concentrations of CO2. This leads to 7 211 999 spectral points in the longwave.
A similar approach has been taken in the shortwave, resulting in spectral resolutions of 0.002, 0.001, 0.002, 0.02, and 1 cm−1 in the spectral ranges 250–2200, 2200–2400, 2400–5150, 5150–16000, and 16000–50000 cm−1, respectively. For overhead sun this also leads to heating-rate errors of no more than around 0.005 K d−1 in any of these wavenumber ranges, for 8 times the preindustrial CO2 concentrations. This leads to 3 126 494 spectral points in the shortwave.
A further significant reduction in data volume is possible if the absorption cross section per molecule is independent of the concentration of that gas and so varies only as a function of temperature and pressure. In this case, for well-mixed gases, the profile of layer-wise optical depth need only be provided for a single concentration profile; if optical depths are required for concentration profiles scaled by a constant, then the optical depths themselves may simply be scaled. We have computed absorption spectra for each gas over the full range of concentrations required in Table 2 and found that to a very good approximation molar absorption can be treated as independent of concentration for all gases except water vapour. Therefore, for the well-mixed gases, absorption spectra are provided only for present-day concentrations. The CKDMIP software accordingly allows the user to scale the optical depth of each gas before performing radiative transfer calculations on the mixture.
The CKDMIP software calculates the spectral optical depth due to Rayleigh scattering using the model of Bucholtz (1995), in which the per-molecule Rayleigh scattering cross section, in square metres, is given by the following for wavelengths of less than 0.5 µm:
where wavelength λ is in µm; it is given by the following for wavelengths greater than 0.5 µm:
A realistic TOA solar irradiance spectrum was extracted from the climate data record of Coddington et al. (2016) by averaging over the last 33 years (1986–2018 inclusive), i.e. three solar cycles. It has a resolution of 1 nm at wavelengths shorter than 750 nm and is interpolated to the spectral resolution of the shortwave gas absorption spectra.
As stated above, the water vapour spectra include the continuum computed using the MT_CKD model, but there is still considerable uncertainty regarding the strength of the water vapour continuum, particularly in the near infrared (Shine et al., 2016), and indeed this could be a source of difference between individual gas-optics schemes and the reference calculations produced in CKDMIP. Therefore, for each dataset, we produce an additional set of water vapour files but with no representation of the continuum. If needed, evaluation can be carried out using only the contribution from spectral lines, or alternatively different models of the continuum can be tried.
The absorption spectra are stored, one gas per file, in netCDF4/HDF5 format with compression, so the file size depends on the spectral extent and degree of fine structure in the spectrum. In the longwave, the volume of a single file (containing 10 profiles) varies from 0.5 GB for CFC-11 to around 10 GB for CH4, and the 50-profile Evaluation-1 dataset amounts to 222 GB in total. In the shortwave the Evaluation-1 dataset amounts to 109 GB.
3.5 Generating irradiance and heating-rate benchmarks
The CKDMIP software takes as input the spectral optical depths of each of a number of gases, optionally scales the optical depths of the well-mixed gases if a different concentration is required, and computes clear-sky aerosol-free irradiances (broadband or spectral) at layer interfaces for each of the test profiles. These can be used to compute broadband or spectral heating-rate profiles. The intention is that the radiative transfer equations are then the same as those used by large-scale atmospheric models, and the same solver is used with the various CKD models in order that any differences to the LBL broadband irradiances are due to the representation of gas optics, not the details of the solver.
In the longwave we use a no-scattering solver with the following properties:
Surface emissivity is assumed to be unity.
The skin temperature of the surface is assumed to be equal to the air temperature at the base of the lowest atmospheric layer.
Local thermodynamic equilibrium is assumed.
The angular distribution of radiation is approximated by four discrete zenith angles in each hemisphere (eight streams in total), chosen using the rules of Gauss–Legendre quadrature. The software supports between one and eight angles per hemisphere, although we find that broadband longwave calculations with four angles agree with those from eight to within 0.05 W m−2 in terms of irradiances and 0.02 K d−1 in terms of heating rates.
The temperature at layer interfaces is taken as input and a linear-in-optical-depth variation in the Planck function within each layer is assumed, leading to the use of Eqs. (6)–(12) of Hogan and Bozzo (2018).
The shortwave scheme has the following characteristics:
It uses a direct-beam calculation plus a two-stream diffuse calculation, with the Zdunkowski et al. (1980) coefficients characterizing the rate of exchange of energy between the three streams and the Meador and Weaver (1980) solutions to the two-stream equations in individual layers. While two streams is fewer than the number used in the longwave, it is of sufficient accuracy because shortwave gaseous absorption in clear skies is predominantly by the direct solar beam.
Calculations are performed at five values of the cosine of the solar zenith angle (μ0): 0.1, 0.3, 0.5, 0.7, and 0.9. This even sampling is appropriate given that the sunlight striking the Earth during daytime has a uniform μ0 distribution between 0 and 1. We do not account for the fact that individual test profiles at a particular latitude would each experience a different μ0 distribution.
No account is made for Earth curvature.
Local thermodynamic equilibrium is assumed.
The atmospheric heating rate in layer i is computed from the net irradiance divergence across a layer, as
where and are the pressure and net downward irradiance, respectively, at the interface between layers i and i+1 (counting down from TOA), g0 is the acceleration due to gravity (standard gravity), and Cp is the specific heat of dry air, taken to be constant at 1004 J kg−1 K−1.
3.6 Radiative forcing of well-mixed gases
Many current CKD models omit some of the gases considered in CKDMIP, particularly in the shortwave. Table 4 provides an estimate of the instantaneous radiative forcing of individual well-mixed gases at present-day concentrations, compared to setting their concentration to zero, computed from averaging over LBL calculations on the 50 Evaluation-1 profiles. This is not an accurate estimate of the climatic impact of each gas since it neglects clouds and fast stratospheric adjustment, and the profiles are not necessarily globally representative, but it gives an indication of the error incurred by neglecting particular gases. The longwave impacts of N2 and O2, ignored by many CKD models, are similar to the values reported by Höpfner et al. (2012). Most shortwave CKD models ignore N2 and N2O, but the results here indicate that this leads to an overestimate of daytime clear-sky net surface solar irradiance by around 0.5 W m−2. It would be interesting to investigate the impact of this on the climate of a global model.
Anyone with a CKD tool can take part in CKDMIP. Participants are provided with access to the Evaluation-1, MMM, and Idealized datasets, and the software described in Sect. 3.5 to perform LBL radiation calculations on them. They may use these or their own datasets as input to their CKD tool. In Sect. 4.1 we describe the band structure that should be used by participants, if possible. Section 4.2 describes the calculations that should be performed by participants and the data they provide. In Sect. 4.3 we outline how these data are processed to quantify accuracy and to investigate the accuracy–efficiency trade-off.
4.1 Common band structures
Virtually all operational CKD models for weather and climate split the longwave and shortwave spectra into bands, and compute k distributions within each one. As shown in the survey of Hogan et al. (2017), the number of bands is strongly correlated to the total number of k terms and therefore to the overall computational efficiency of a CKD model. The choice of bands can be dependent on the constraints of a particular CKD scheme: some require the longwave bands to be narrow enough that the Planck function may be assumed to be constant (e.g. Fu and Liou, 1992); some need to restrict the number of active gases in a band (e.g. Mlawer et al., 1997); and some assume the spectral overlap of different gases is random and invalid for wide bands (e.g. Ritter and Geleyn, 1992); while most assume that cloud and surface properties are constant within each band, which could lead to significant errors in the shortwave if the bands are too wide (Lu et al., 2011). All of these arguments deserve detailed scrutiny within CKDMIP.
We propose two band structures, shown in Table 5 for the longwave and Table 6 for the shortwave. Since the Rapid Radiative Transfer Model for General Circulation Models (RRTMG) (Mlawer et al., 1997) is so widely used, our proposed “narrow bands” are modelled on RRTMG, except that we merge a few of the very narrow or very low-energy bands that RRTMG represents with four or fewer k terms. This leads to 13 bands in both the longwave and shortwave. These bands should be narrow enough to satisfy all the needs for narrowness cited previously. To assist participants who do not wish to download all the large spectral absorption files, much smaller files are available containing benchmark irradiance profiles computed for each scenario of the Evaluation-1 dataset, both broadband values and values averaged in each of the narrow bands.
The “wide bands”, of which there are five in both the longwave and the shortwave, consist of groupings of the narrow bands. In the longwave these are purposefully somewhat wider than in most current CKD models, in order to really test the limits of some of the restrictions cited above. The wide-band models will be compared to the narrow-band models in terms of both accuracy and efficiency, which may allow the advantages of CKD schemes that do not assume the Planck function to be constant across a band or do not assume random spectral overlap to become apparent.
Some participants may wish to use their own sub-bands within these wide bands if they think it will achieve a better accuracy–efficiency trade-off for a particular wide band. For example, Cusack et al. (1999) used two “split bands” in the longwave: one which represented the wings of the main CO2 band (essentially a merger of our narrow bands 3 and 5) and the other which represented the parts of the infrared window on either side of the ozone band (essentially a merger of our narrow bands 6 and 8).
Finally, CKDMIP welcomes submissions using even wider bands. Indeed, the “full-spectrum correlated-k” (FSCK) technique has been proposed as a means to achieve good accuracy using only one band in the longwave (Hogan, 2010) and two in the shortwave (Pawlak et al., 2004). The investigation of the effect of spectral variations in cloud properties within bands and k terms described in Sect. 4.4 will be particularly important for FSCK submissions.
All submissions, whether using narrow, wide, or other band structures, will be compared to each other according to their broadband accuracy and their overall efficiency (total number of k terms).
4.2 Contribution of CKDMIP participants
Ideally, CKDMIP participants would use their tool to generate a CKD model for all combinations of the following:
the longwave and shortwave;
the three applications listed in Table 1;
the narrow and wide band structures described in Sect. 4.1 (and optionally even wider bands);
a range of total number of k terms (at least three configurations), in order that the efficiency–accuracy trade-off can be explored.
This could potentially lead to a full submission involving the generation of 36 CKD models. It is recognized that this is potentially very demanding, so reduced submissions are welcome according to the scientific interests of the participant. In principle, a participant could submit just one longwave and one shortwave CKD model; if the model used the narrow bands specified in Sect. 4.1 and targeted climate modelling, then it could still be tested against other models in all scenarios.
Participants do not submit the code for their CKD models but rather run each of them on the 100 profiles of the Evaluation-1 and Evaluation-2 datasets. For CKD models generated for the two NWP applications, the well-mixed greenhouse gas concentrations use the present-day values given in the third line of Table 2. For CKD models generated for climate modelling, they run each of the 34 scenarios given in Table 2 in the longwave and the first 18 scenarios in the shortwave.
For each of these scenarios, they submit a netCDF file containing the following variables as a function of profile number for the Evaluation-1 and Evaluation-2 datasets:
pressure at layer interfaces, copied from the input file;
the absorption optical depth of all gases in each layer, in each of N k terms;
in the shortwave only, the Rayleigh scattering optical depth in each layer and k term;
in the shortwave only, the TOA solar irradiance integrated over the parts of the spectrum contributing to each k term, scaled such that these numbers sum to a total solar irradiance of 1361 W m−2;
in the longwave only, the Planck function at each layer interface, integrated over the parts of the spectrum contributing to each k term; at a given layer interface, these values should sum to σT4, where σ is the Stefan–Boltzmann constant and T is the temperature at the layer interface (provided in the input file).
These files should be compatible with the CKDMIP software, which can then read them in and compute profiles of upwelling and downwelling irradiances, both at each k term and as broadband values. This ensures that the radiative transfer is identical to that used in generating the LBL benchmarks, so that when the irradiances are compared to the benchmarks, the differences are only due to the spectral approximations made in the CKD model.
A further file is required for each CKD model generated, describing which parts of the spectrum are represented by each k term, to be used in Sect. 4.4 for investigating the representation of cloud optical properties. In the longwave this should be expressed at a resolution of 10 cm−1 and in the shortwave at a resolution of 50 cm−1. This is commensurate with the spectral scale at which the optical properties of clouds vary.
In addition to data files, we require detailed information from each participant about how their CKD tool works, including how the spectrum is reordered, how the number of k terms is chosen in a given band, how g space is partitioned amongst the k terms, how the spectral absorptions are averaged to a k term, and how the spectral overlap of gases is treated. If participants use a different spectroscopic database from the one provided by CKDMIP, then they should describe it in detail. This information will then be invaluable when we come to interpret the results from different tools.
The protocol above assumes that participating radiation schemes have a clean separation between the generation of optical depths in each k term and the radiative transfer performed on them. Allowance will need to be made for some schemes in which the separation is not so clean. For example, SOCRATES (the Suite Of Community Radiation codes based on Edwards and Slingo, 1996) uses the concept of “equivalent extinction” to treat minor gases (Edwards, 1996). In the longwave this involves performing M no-scattering radiation calculations to work out the contribution from minor gases in a band. The net irradiance from these profiles are analysed to work out the equivalent extinction, which is then added to the N k terms for representing the major gases in the band. A full longwave radiative transfer calculation, including scattering, is then performed on these N k terms. This approach could be accommodated in CKDMIP by the participant performing the M initial calculations themselves and providing the resulting N optical depth profiles. The CKDMIP radiative transfer software would then be run on these N k terms (verifying that it gives very similar results to the SOCRATES radiative transfer solver), but when assessing the accuracy–efficiency trade-off, the cost of the scheme would be counted as aM+N, the a factor being optionally less than 1 to account for the fact that equivalent extinction can be computed with a cheaper solver.
In the shortwave, the SOCRATES scheme uses a more sophisticated treatment of gas optics (M+N k terms) for the cheap direct-beam radiative transfer calculation and a simpler treatment of gas optics (N k terms) for the more expensive solver for scattered radiation. This could be accommodated by the participant providing CKDMIP with separate direct and a diffuse optical depths in the N k terms, and again the cost of the scheme being counted as aM+N, with a this time representing the cost of the direct-only versus full shortwave radiation calculation.
4.3 Error metrics
The irradiance profiles computed from the submissions of participants for the relevant scenarios in Table 2 will be compared to the equivalent LBL benchmarks, with differences in upwelling and downwelling irradiances being characterized by the bias and root-mean-squared error (RMSE) over each set of 50 profiles. Particular emphasis will be placed on the surface downwelling and TOA upwelling irradiances.
Atmospheric heating-rate bias and RMSE will be examined as a function of pressure. The profile of heating-rate error will be summarized by a few error metrics, such as the whole-profile RMSE, or the values for the troposphere, stratosphere and (except for the “limited-area NWP” application) mesosphere separately. An appropriate weighting with pressure will need to be specified; rather than weighting linearly with pressure, which overweights the troposphere, Hogan (2010) proposed weighting by the square root of pressure, which increases the weighting of stratospheric errors, but other powers (e.g. the cube root) are possible. Naturally, the heating-rate errors will only be counted down to the lowest pressure for the application in question (see Table 1). The handful of RMSE values will then be plotted as a function of number of k terms to compare how different CKD tools perform in terms of accuracy versus efficiency.
In addition, we will look at the accuracy of the CKD models for climate in terms of the TOA and surface radiative forcing they predict when the five well-mixed anthropogenic greenhouse gases are perturbed as described by the scenarios in Table 2. This will involve simple averaging over the 50 profiles.
Note that we do not propose to define a “cost function” that combines multiple error measures into a single metric, as it may not align with those used explicitly or implicitly by the various CKD tools. Nonetheless, all model output will be freely available for participants to compute their own error metrics should they wish.
4.4 Errors due to the spectral variation in cloud properties
Until this point, we have considered exclusively clear-sky radiation calculations with a spectrally constant surface albedo. It is known that errors can arise in cloudy skies if cloud optical properties are assumed to be constant across spectral bands (Lu et al., 2011), primarily due to the spectral correlation of absorption by water vapour, liquid water, and ice. In principle, this error can be ameliorated by computing cloud properties separately for each k term, possible if we have fine-scale information on which parts of the spectrum each k term contributes to. As described in Sect. 4.2, this information is requested of participants for each of their CKD models.
In the final part of CKDMIP, errors in cloudy skies will be estimated. This may be achieved using the clear-sky submissions of the CKDMIP participants, so requiring no additional simulations from them. Firstly, LBL cloudy-sky benchmarks are produced. For liquid clouds, Mie calculations have been performed for distributions of droplets at a sufficiently high spectral resolution to resolve variations in refractive index. For ice clouds we use the generalized habit mixture of Baum et al. (2014). The CKDMIP software is then used to add horizontally homogeneous clouds of varying optical depth to the gas optical depth in the Evaluation-1 dataset for present-day conditions and to perform LBL calculations. Then the equivalent calculations are performed for the various CKD models, by taking their present-day optical depth files and adding the contribution from clouds. From the information they provide on the spectral contributions to each k term, average cloud properties will be computed for each k term using the appropriate combination of “thick” and “thin” averaging (Edwards and Slingo, 1996). Errors in irradiances and heating rates will then be computed.
A similar procedure would be possible for aerosols, or to quantify errors due to spectrally varying surface albedo, particularly over snow and vegetation where the variations are largest.
In this section we demonstrate the CKDMIP approach by using the Evaluation-1 dataset to evaluate an existing CKD model: RRTMG. This model is very widely used; for example, Hogan et al. (2017) reported in their survey of seven global NWP models that three used RRTMG for gas optics in both the longwave and the shortwave and one used it in the longwave only. We evaluate the RRTMG implementation in the ECMWF radiation scheme (Hogan and Bozzo, 2018), which is only slightly modified from the original implementation by Morcrette et al. (2008) and has been found to be indistinguishable from the gas optics in version 3.9 of RRTMG available from AER.
Figure 5 evaluates longwave irradiances and heating rates for the present-day scenario described in Table 2. The same radiative transfer algorithm is used for the reference LBL calculations and the CKD model: no scattering with four zenith angles per hemisphere. Irradiance errors are almost all within 2 W m−2 at any altitude, and the magnitude of the biases at the surface and TOA are around 0.4 W m−2. Panel (h) shows that for pressures down to 4 hPa, the heating-rate bias is low and the RMSE is only 0.1 K d−1. For lower pressures than this in the upper stratosphere and mesosphere, the heating-rate RMSE is twice as large and the bias profile exhibits distinct “wiggles” with pressure. The equivalent plots for the preindustrial, glacial maximum, and future scenarios may be viewed at the CKDMIP web site, along with an evaluation of the contributions from each of the narrow spectral intervals listed in Table 5.
Figure 6 uses scenarios 5–22 of Table 2 to evaluate the instantaneous radiative forcing associated with perturbing the concentrations of individual well-mixed greenhouse gases from their present-day values. Instantaneous radiative forcing is defined here as the change to the net (downwelling minus upwelling) irradiance at TOA or the surface, keeping atmospheric and surface temperatures fixed. The radiative forcings have been averaged over the 50 Evaluation-1 profiles. We see that in general RRTMG captures the radiative forcings accurately, including CO2 increased to 8 times its preindustrial concentrations. The one exception is the forcing associated with reducing CH4 to 350 ppbv, the magnitude of which is underestimated by around a factor of 2. Recent evaluation (not shown) of the new “parallel” version of RRTMG (RRTMGP; Pincus et al., 2019) has found that this problem has since been fixed, although note that at present RRTMGP uses 256 k terms in the longwave, so is more expensive than RRTMG.
Figure 7 evaluates the shortwave irradiance and heating-rate profiles from RRTMG for present-day concentrations of the well-mixed greenhouse gases. RRTMG up to and including version 3.9 uses a solar spectrum from the mid-1990s that has 7 %–8 % more energy in the ultraviolet than the up-to-date (Coddington et al., 2016) spectrum used in CKDMIP. This results in an overestimate in solar heating by O2 and O3, which the blue line in Fig. 7h shows to peak at on average 1.5 K d−1 at the stratopause. Hogan et al. (2017) reported that the resulting warm bias in the stratospheric climate of the ECMWF model could be reduced by scaling the irradiances in each RRTMG band to match the solar spectral irradiance of Coddington et al. (2016). The red lines and symbols in Fig. 7 show that the effect of doing the same in the 13 bands of Table 6 is to significantly reduce the heating-rate overestimate in the upper atmosphere. Plots evaluating the performance in each of these narrow bands are shown on the CKDMIP web site.
Figure 8 depicts the instantaneous shortwave radiative forcing resulting from perturbing the concentrations of CO2 and CH4 in the range shown in scenarios 5–14 of Table 2. We see that the radiative forcing is underestimated by 25 %–45 % for both gases, yet the heating-rate response is generally good. This implies that there is scope for improvement in the parts of the spectrum where the absorption by CO2 and CH4 is weak but not zero.
The change to the shortwave radiative forcing of perturbing N2O across its 190–540 ppbv range is around 0.03 W m−2 at TOA and 0.15 W m−2 at the surface, which is around 10 % of that from perturbing CH4 across its 350–3500 ppbv range. Since N2O is not represented in the shortwave part of RRTMG, a comparison has not been plotted.
The Correlated K-Distribution Model Intercomparison Project (CKDMIP) is an international collaboration whose aim is to evaluate and improve the treatment of gas optics in the radiation schemes used for weather and climate prediction. In this paper we have described the detailed experimental protocol for CKDMIP, along with the generation of the associated large dataset of gaseous absorption spectra and radiative transfer software.
The nine most radiatively important atmospheric gases in the terrestrial atmosphere have been selected, and via the use of an equivalent concentration of CFC-11, the next 38 most radiatively significant gases are implicitly accounted for. We have found that N2 and N2O each reduce the daytime surface downwelling shortwave irradiance of the order of 0.25 W m−2, so they ought not to be ignored by shortwave CKD models as they generally are at present.
The primary datasets for evaluation consist of 100 profiles extracted from the ECMWF model, a third of which have been chosen to have extremes of temperature, humidity, and ozone. Thirty-four scenarios have been devised for the well-mixed greenhouse gases, intended to span terrestrial concentrations over the last million years and out to the highest concentrations in any of the CMIP6 projections to the year 2250. We have found that the per-molecule absorption is essentially independent of concentration for all gases except water vapour, which means that LBL reference calculations can easily be performed for any scenario (using the CKDMIP software) by scaling the absorption spectra from their present-day values.
We have demonstrated the strengths of the CKDMIP approach by using the dataset and software to evaluate RRTMG, an existing widely used CKD model. This has revealed some particular strengths of RRTMG, such as its ability to estimate the longwave radiative forcing of the main anthropogenic greenhouse gases in future climate scenarios, but it has also uncovered some shortcomings in a few of the bands that will be improved in future versions of RRTMG.
The next step will be to evaluate not just CKD models with fixed numbers of k terms but CKD tools that can generate new CKD models, quantifying how their accuracy varies with the number of k terms (a proxy for the computational cost of an entire radiation scheme). An objective comparison of the performance of different CKD tools will provide crucial insights into which strategies and approximations yield the most accurate CKD models for a given computational cost, hopefully stimulating the replacement of the older and less accurate radiation schemes used by some climate models (see Soden et al., 2018). Moreover, the evidence compiled could form a springboard for the development of a more formal theory to underpin CKD tools, such as how to optimally partition g space. We will also use the submissions by the CKDMIP participants to quantify the errors associated with representing the spectral variation in cloud optical properties and the extent to which these can be mitigated by using different optical properties for each k term rather than just each band. If during the analysis of the results it becomes apparent that further scenarios and LBL datasets are required, then they will be added.
In the longer term it is hoped that CKDMIP will stimulate the development of community tools to allow users of radiation schemes to more easily generate CKD models targeted at specific applications. It could also form the basis for improving the consistency between the broadband irradiance models considered in this paper and the narrowband radiance models used for data assimilation, since the latter are also often trained using LBL calculations on a set of training profiles (e.g. Matricardi et al., 2004). Furthermore, while the focus of the CKDMIP dataset is on the terrestrial atmosphere, what is learned during the project should translate easily to radiative transfer on other planets.
RH carried out the conceptualization, investigation, design of the CKDMIP methodology, writing of the CKDMIP software, data curation, and writing of the paper. MM generated the raw LBL data, contributed to the design of the CKDMIP methodology, wrote the parts of the paper describing the use of LBLRTM, and provided critical review of the rest of the paper.
The authors declare that they have no conflict of interest.
This paper has benefited from valuable discussions with Eli Mlawer, Robert Pincus, James Manners, Keith Shine, Seiji Kato, David Paynter, Jiangnan Li, and Stephen English. Hartwig Deneke is thanked for assistance in comparing various versions of RRTMG with each other.
This paper was edited by Richard Neale and reviewed by two anonymous referees.
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