3.1. Liquid Water Content
Figure 2 shows the medians of CLOUDNET observed liquid water content, ICON simulated grid-scale liquid water content (
Figure 2a, c, e) and its frequency of occurrence (
Figure 2b, d, f) in Munich, Lindenberg and Jülich. The frequency of occurrence of observed and simulated liquid water content was calculated for the values greater than 10
-6 g/m
3.
Table 2 presents the main statistical parameters of the liquid water path according to hourly average measurements and modelling in Jülich, Lindenberg and Munich. For ICON simulations both the grid-scale and the total (grid-scale and subgrid-scale) LWP are shown. Vertical cloud structure is well reproduced by ICON, but there is a slight underestimation of liquid water content throughout the profile. As a result, the simulated grid-scale liquid water path (LWP) is on average underestimated relative to CLOUDNET observations by 68±17 g/m
2. The accounting of subgrid-scale liquid water content leads to the liquid water path increase. However, the total liquid water path is still underestimated by 59±16 g/m
2. In addition, model results provide lower frequency of LWC in Lindenberg and Jülich (
Figure 2b, d). A better agreement of model LWC frequency of occurrence over Munich (
Figure 2f) could be attributed to a successfully forecast of sub-inversion clouds by the ICON model there and, to some extent, much smaller statistics. However, the LWP is underestimated at all CLOUDNET sites, and its interquartile range is lower in Lindenberg and Munich (see
Table 2).
All these differences may be associated with the following:
(1) Insufficient concentration of cloud condensation nuclei for droplets nucleation and liquid water content growth in conditions with CCN=250 cm-3;
(2) Too intensive formation of ice crystals, which can lead to a decrease the excess specific humidity required for the cloud droplet nucleation;
(3) Too intensive processes of autoconversion and accretion, leading to the transition of cloud water mass into precipitation;
(4) The problems with the saturation adjustment scheme, influencing on the deficiency of specific humidity to activate condensation nuclei.
Satellite data provides N
d values that correspond to the cloud base level. ICON model provides height-resolved N
d values. To bring ICON results closer to MODIS estimates of N
d (see
Section 2.3), we considered hourly average vertically maximum simulated number concentrations of cloud droplets. The maximum cloud droplets number concentration in the model can be not only near cloud base. So, we do not limit the simulated N
d and choose the maximum value in each profile. However, even in this case, no more than 25% of the whole ICON sample accounted for N
d concentrations is above 77 cm
-3. The N
d interquartile range of ICON results is 63 cm
-3 with a median of 29 cm
-3. The ice water content is also higher than the simulated one (not shown), so no intensive nucleation and growth of ice crystals are observed. For considering the influence of autoconversion and accretion processes on LWP, we compared the measured liquid water path with simulated liquid and rain water path (LWP+RWP). Even taking into account raindrops, the simulated LWP is generally underestimated by 17±13 g/m
2. This approach does not show enhanced autoconversion and accretion as the principal reason of LWP underestimation. We assume that this mechanism could be important, but there is no observation-based experimental data for proving the level of this process. Therefore, we rely on observational data and the conclusions shown above.
The simulated liquid water content may be less than the observed LWC due to inaccurate prediction of the water vapor path, since water vapor is the main source of the cloud droplet nucleation and growth. However, according to studies of the ICON model [58, 59], this characteristic is predicted quite accurately.
Thus, one of the reasons of the model lower liquid water content and its occurrence may be the saturation adjustment scheme, which is the most important regulator of all microphysical processes. Saturation adjustment leads to a lower condensation and to a higher evaporation rates of droplets in the bulk scheme relative to the spectral microphysical scheme. The work [
11] showed that the saturation adjustment contributes to lower LWC for situations of strato-cumulus clouds. Khain and Pinsky [
3] also showed negative effect of saturation adjustment on the diffusion growth of cloud particles in different cloud types. Unfortunately, we cannot consider this issue in more detail, since this requires a mixed-phase spectral microphysical scheme, which is more close to the real physics of clouds [
10] compared to saturation adjustment scheme used in the ICON model. The liquid water path underestimation in some cases could be due to the low specified CCN of 250 cm
-3, hence, we conducted a numerical experiment with a higher content of cloud condensation nuclei. Based on satellite measurements and upper-air sounding data, we chose September 19, 2021 as the day with the most uniform clouds over the simulation domain.
Figure 3 shows MODIS retrievals of cloud droplet number concentrations at the cloud base according to the method (Equation 4) with the average N
d of 258 cm
-3. We carried out a numerical experiment with high CCN of 1700 cm
-3, since this value is typical for the continental or polluted clouds [19, 55, 60].
Figure 4a shows box plots of simulated cloud droplet number concentration over the CLOUDNET sites with cloud condensation nuclei 250 and 1700 cm
-3. The whole four-dimension (height-field-time) simulated N
d was taken into account to compare results of specified CCNs. The cloud droplet number concentration increases by 94±20 cm
-3 (65%) with this CCN growth. Median (interquartile range) values of N
d are 22 (62) cm
-3 and 84 (127) cm
-3 for CCN=250 cm
-3 and CCN=1700 cm
-3, respectively.
Considering vertically maximum ICON simulated number concentrations of cloud droplets, median Nd increases from 23 cm-3 with NCCN 250 cm-3 to 89 cm-3 with NCCN 1700 cm-3. Thus, not all of ССN were activated in the model.
Vertical velocity (W) is an important factor in the cloud droplet nucleation [53, 61]. Kretzschmar et al. [
62] showed that one of the reasons for the low N
d and liquid water content in ICON may be an unsufficient W, providing lower CCN activation in the parametrization.
Figure 4b illustrates the dependence of cloud droplet concentration on vertical velocity in the Segal-Khain scheme [
19] for CCN of 1700 cm
-3. At low vertical velocities, less than half of the CCN can be available for nucleation. The maximum value of the simulated grid-scale vertical velocity at levels near the cloud base for September 19, 2021 was 0.9 m/s at CLOUDNET sites. Thus, the CCN concentration was actually in the range from 140 cm
-3 to 900 cm
-3 at the simulated vertical velocities instead of the specified 1700 cm
-3. The CCN content of 140 cm
-3 corresponds to the minimum permissible vertical velocity of 0.1 m/s in the cloud droplet nucleation scheme. However, in our experiments the simulated N
d is significantly less than the satellite-derived N
d. This indicates low intensity of cloud droplet nucleation and the contribution of the saturation adjustment scheme together with other microphysical processes, for example, evaporation, to the resulting N
d and LWP values.
In general, an increase in the concentration of cloud condensation nuclei contributed to an increase in the grid-scale liquid water path over the modeling domain (
Figure 4c). Following [
63],
Figure 4c shows only grid-scale liquid water path of more than 10 g/m
2. With the growth of cloud condensation nuclei, there is a shift in the distribution of liquid water path towards higher values. The grid-scale liquid water path increased by an average of 118±2 g/m
2 (40%). As a result, the liquid clouds have become more optically thick (
Figure 4d, the cases with liquid cloud optical thickness of more than 5 are shown). However, taking into account the subgrid-scale clouds, the effect of CCN on the cloud optical thickness is less pronounced. Liquid cloud optical thickness increased by an average of 1 (8%). In order to determine the effect of CCN on the simulated global irradiance at ground, we considered cases of overcast conditions with a solar elevation of at least 25° and liquid cloud optical thickness of more than 5. Under these conditions, the CCN increase from 250 cm
-3 to 1700 cm
-3 provides the solar irradiance decrease by 9 W/m
2 (12%).
3.2. Cloud Optical Thickness and Shortwave Irradiance at Ground
Cloud optical thickness and the cloud fraction are the most important factors in the cloudy atmosphere, which determine the global solar irradiance at ground. Cloud optical thickness is determined by a liquid water content and effective radius of cloud droplets [
64].
In order to exclude the influence of errors in the scheme of clouds optical properties evaluation in the ecRad scheme on the cloud-radiation interaction, we compared the liquid cloud optical thickness (COTliq) according to MODIS and ICON data. We consider the cases with LWP successful prediction, when the absolute error of the simulated LWP was less than 15% (391770 pixels) compared to the MODIS LWP. In this case the median liquid cloud optical thickness and its interquartile range, shown in brackets, are 13.3 (12) and 13.5 (11) according to MODIS and ICON, respectively. The average error of simulated COTliq is +0.04±0.03 (0.02%). If considering all cases, regardless the quality of the simulated cloud water (8642685 pixels), the ICON cloud water path (liquid and ice phases) is on average 52±0.1 g/m2 lower relative to the MODIS retrievals. As a result, the cloud optical thickness is underestimated by 4±0.01 (24%). Hence, the cloud optical thickness is predicted with sufficient accuracy if liquid water path is successfully estimated.
The cloud fraction is a more difficult for evaluation from both numerical forecasting and observations [
65]. Standard verification approaches are not suitable for cloud fraction analysis, therefore other, more sophisticated methods and measurement data are required [66, 67]. Therefore, we analyzed not only cloud fraction, but also considered another characteristic – the ratio (R) of direct radiation at horizontal surface to global solar irradiance using hourly average data. This value can be considered as an analogue of the cloud fraction after the application of hourly average procedure [
68]. The hourly R values actually characterizes the proportion of gaps in the clouds.
According to the BSRN observations in cloudy conditions, ICON simulated hourly global irradiance at ground is overestimated on average by 46±15 W/m
2 (18%). At the same time, the simulated R is overestimated by 0,13±0,02.
Figure 5 shows the hourly average values of global irradiance (Q), liquid water path (LWP) and R averaged over the R intervals according to measurements (
Figure 5a) and according to measurements and simulations (
Figure 5b). The results of ICON simulations are presented using CCN number concentration of 250 cm
-3. In addition, low level cloud fraction (CLCL, dotted lines) and total cloud fraction (CLCT, crosses) are also shown.
According to the ICON numerical experiments, R values are higher than the observed ones (
Figure 5a). For overcast situations (R
obs is equal to 0), average R
sim=0.2±0.04. As a result, simulated global irradiance is higher than the measured one: 263±33 W/m
2 and 162±13 W/m
2, respectively. At different averaging intervals (horizontally), the R
obs grows much faster relative to the simulated R (see
Figure 5a). If we rank the cases based on both the measured and simulated R, the differences between simulated and measured global irradiance decrease (
Figure 5b). Note, that the simulated liquid water path is underestimated compared to the CLOUDNET observations for all considered R intervals (
Figure 5a, b). Thus, improving the quality of the forecast of the R contributes to reducing the error of solar irradiance evaluation even with a general underestimation of the liquid water path.
The total cloud fraction according to the ICON estimates generally corresponds to the observations (
Figure 5a, b), while a more pronounced decrease in the measured CLCLs is observed compared to the simulated values. The model CLCLs are overestimated almost everywhere. However, even at higher model CLCLs we observe the overestimating of Q. In addition, the sensitivity of global solar irradiance to cloud fraction is generally less pronounced than its sensitivity to R (see
Figure 5). The linear correlation coefficients of CLCL and Q are -0.26 and -0.23, while the correlation coefficients between R and Q are 0.78 and 0.86 according to measurement and simulation data, respectively.
Figure 5.
Global solar irradiance (Q), liquid water path (LWP), low level cloud fraction (CLCL), total cloud fraction (CLCT), and the R ratio according to simulations (Rsim) and observations (Robs) as a function of R according to measurements (a, 214 cases) and for consistent R values according to simulations and measurements (b, 84 cases). Lindenberg site. Simulations with CCN 250 cm-3. The solar elevation is above 25°. Confidence intervals are represented by a fill for R and lines for the other variables.
Figure 5.
Global solar irradiance (Q), liquid water path (LWP), low level cloud fraction (CLCL), total cloud fraction (CLCT), and the R ratio according to simulations (Rsim) and observations (Robs) as a function of R according to measurements (a, 214 cases) and for consistent R values according to simulations and measurements (b, 84 cases). Lindenberg site. Simulations with CCN 250 cm-3. The solar elevation is above 25°. Confidence intervals are represented by a fill for R and lines for the other variables.
Hence, the error in R is the main factor determining the overestimation of simulated global irradiance. This could be observed due to inaccurate overlapping procedure between the layers. For example, Kawai et al. [
69] showed the effect of the overlapping scheme on the cloud albedo without changing the total cloud cover in the MRI-ESM2 climate model. Even with the observed liquid water path underestimation, an accurate forecast of R leads to an improvement in the global irradiance prediction. It should be noted that the penetration of direct radiation through the gaps may provide a significant contribution to global solar irradiance and, hence, air temperature. The effect of the liquid water path underestimation on solar radiation is less pronounced, since the sensitivity of global irradiance to cloud optical thickness becomes lower with the increase in COT [
70], which is also noted as an "accumulation effect" [
71]. The quality of cloud fraction forecast at each model level is directly related to the quality of cloud moisture forecast (see
Section 2.1). This means that the underestimation of cloud moisture may also contribute to the modeling of less cloudy conditions.
The forecast of broken clouds is known to be the weakest points of cloud cover forecast [
72]. The errors in cloud fraction prediction are noted in the studies concerning many numerical weather prediction and climate forecasting models [12, 15, 67, 73-75]. The main reasons for inaccuracies in the cloud fraction forecast include the errors in the structure of simulated convective clouds, liquid water content of stratiform clouds and clouds frequency of occurrence in general. Errors of solar irradiance prediction, besides cloud cover schemes, depend on the cloud overlap assumption, which is a difficult task both in modeling and observations [76, 77]. Many forecasting centers try to reduce the systematic errors in cloud fraction prediction in postprocessing, in particular, using neural networks [78, 79]. At the moment, the new ICON diagnostic cloud fraction scheme is developing [
80]. The scheme is generally corresponded to the global trend of complicating microphysical processes by considering a whole complex of physical cloud mechanisms [
81].