Benefit of convection permitting climate model simulations in the representation of convective precipitation
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A major source of uncertainty in regional climate model (RCM) simulations arises from the parameterisation of sub-grid scale convection. With increasing model resolution, approaching the so-called convection permitting scale, it is possible to switch off most of the convection parameterisations. A set of simulations using COSMO-CLM model has been carried out at different resolutions in order to investigate possible improvements and limitations resulting from increased horizontal resolution. For our analysis, 30 years were simulated in a triple nesting setup with 50, 7 and 2.8 km resolutions, with ERA40 reanalysis data at the lateral boundaries of the coarsest nest. The investigation area covers the state of Baden-Württemberg in southwestern Germany, which is a region known for abundant orographically induced convective precipitation. A very dense network of high temporal resolution rain gauges is used for evaluation of the model simulations. The purpose of this study is to examine the differences between the 7 and 2.8 km resolutions in the representation of precipitation at sub-daily timescales, and the atmospheric conditions leading to convection. Our results show that the highest resolution of RCM simulations significantly improves the representation of both hourly intensity distribution and diurnal cycle of precipitation. In addition, at convection permitting scale the atmospheric fields related to convective precipitation show a better agreement with each other. The results imply that higher spatial resolution partially improves the representation of the precipitation field, which must be the way forward for regional climate modelling.
KeywordsRegional climate model COSMO-CLM Convection permitting scale Convection Atmospheric processes Diurnal cycle and precipitation
Precipitation is one of the most crucial variables to assess in a changing climate. However, it is also one of the most difficult to simulate. Although daily precipitation statistics improve with increasing spatial resolution (Boberg et al. 2009, 2010; Berg et al. 2013), problems remain with the sub-daily statistics such as the diurnal cycle (Dai and Trenberth 2004; Dai 2006). Recent investigations have shown the importance of higher temporal resolution in precipitation statistics (Haerter et al. 2010; Berg et al. 2013), especially for assessments of convective type precipitation (Lenderink and van Meijgaard 2008; Haerter and Berg 2009).
A high temporal resolution of precipitation statistics is especially important in summer when precipitation over land is often convective (Dai and Trenberth 2004; Dai 2006). In regional climate models (RCMs) convective precipitation usually occurs too early in the day and the amplitude of its diurnal cycle is usually overestimated (Brockhaus et al. 2008; Yang and Slingo 2001; Dai and Trenberth 2004; Dai 2006). The correct representation of convective precipitation is a very complicated task in modelling because it involves complex interactions between the surface, the boundary layer, and the free troposphere (Khodayar et al. 2013). Furthermore, vertical profiles of temperature and humidity define the convective available potential energy (CAPE; Moncrieff and Miller 1976), thereby affecting the strength of the convective systems and the associated precipitation intensities (e.g. Emanuel 1994). Since convection acts on a scale of only a few kilometres, it is necessary to use parameterisations for typical RCM simulations with grid resolutions of 10–100 km. According to Weisman et al. (1997), 4 km spatial resolution may be sufficient for non-hydrostatic models to explicitly represent convective systems. Previous studies (e.g. Hohenegger et al. 2008; Brockhaus et al. 2008; Bechtold et al. 2004) recognised the parameterisation of convection as a major source of uncertainties and errors in simulating the diurnal cycle of precipitation.
Increasing the spatial resolution towards convection permitting scales provides the possibility to switch off a major part of the convective parameterisations. In addition, a higher resolution model allows a better representation of orography and surface fields which are crucial for the initiation of convection in complex terrain (Hohenegger et al. 2008). Copious literature proves the added value of this spatial resolution in the representation of the precipitation field especially in cases of moist convection and/or in regions with strong orography (Langhans et al. 2013; Mass et al. 2002; Miura et al. 2007; Grell et al. 2000; Richard et al. 2007; Lean et al. 2008; Schwartz et al. 2009; Weusthoff et al. 2010; Baldauf et al. 2011; Hohenegger et al. 2008; Prein et al. 2013). Most of these studies are related to numerical weather prediction (NWP) or limited to few summers. The computational cost is high for running long-term high-resolution simulations, and there is furthermore a shortage of suitable observational datasets available for evaluation.
The goal of this paper is to investigate the possible improvements and limitations in the representation of convective precipitation resulting from increased horizontal resolution in climate model simulations. For this purpose, we compare the performance of two climatological simulations of 30 years each with the COSMO-CLM (COnsortium for Small scale Modelling model-in CLimate Model, here abbreviated CLM); one at 7 km (CLM7) horizontal resolution with parameterisation of convection, and one at 2.8 km resolution (CLM2.8) with most convective parameterisations turned off such that no sub-grid scale precipitation is calculated. A high temporal resolution and spatially dense station observational data set is used for validation. Since the main difference between the two simulations in terms of model setup resides in the convection scheme we explore the differences between the two resolutions in the representation of the conditions leading to convection in detail. In this context, the instability of the atmosphere, vertical profiles of temperature and humidity as well as cloud cover, radiation budget and triggering mechanisms are investigated. In Sect. 2, we present the investigation area and its characteristics, and in Sect. 3 we describe the model configuration for the different simulations, as well as the observational data used for validation purpose. An overview of the methods is provided in Sect. 4. In Sect. 5 we discuss the results on the representation of precipitation and the atmospheric conditions leading to convection and we end with conclusions in Sect. 6.
2 Investigation area
3 Data and models
COSMO is a non-hydrostatic local area model originally created by the German Weather Service (DWD) for weather predictions (Steppeler et al. 2003) and later adapted to perform climatological simulations by the COSMO-CLM community (Böhm et al. 2006). Using ERA40 reanalysis data (Uppala et al. 2005) as driving data for the simulations, a triple nesting procedure in rotated coordinates was employed to reach the final high resolution (Fig. 1a). The coarsest nest at 0.44° resolution (circa 50 km) comprises large parts of Europe (118 × 112 grid points). The next finer nest (here referred to as CLM7) at 0.0625° (circa 7 km) covers all of Germany and the near surroundings (165 × 200 grid points) and the finest nest (here referred to as CLM2.8) used here is at 0.025° (circa 2.8 km) and concentrates on the state of Baden-Württemberg [140 × 116 grid points; similarly to Prein et al. (2013)] in southwestern Germany (Fig. 1). All simulations use 40 vertical levels and nine soil layers, and are carried out for the period 1968–1999 with the first 3 years considered as spin-up time and therefore not included in the analysis. The present study focuses on the added value of resolving convection in the representation of atmospheric conditions leading to precipitation. In this context, the coarser nest at 50 km resolution (see Berg et al. 2013) is not included in the current analysis.
The 7 km resolution is in a spatial range where larger convective processes can be resolved, while smaller ones need a parameterisation; thus, there could be an overlap between resolved and parameterised convection. Therefore, in addition to CLM2.8 and CLM7, a shorter run (1991–1999 including 1 year spin-up time), called CLM7_conv, at 0.0625° was performed over the same simulation domain as CLM7, but without most of the convection parameterisations. The setup used in this study (CLM version 4.8) employs a Runge–Kutta time-stepping scheme and a delta-two-stream radiation scheme according to Ritter and Geleyn (1992) called every hour for CLM7 and CLM7_conv, and every 15 min for CLM2.8. Convective mass flux is parameterised in CLM7 according to the Tiedtke (1989) scheme with a moisture convergence. CLM2.8 and CLM7_conv utilise this parameterisation only for shallow convection, thus no precipitation is produced for the sub-grid. Vertical turbulent diffusion uses prognostic turbulent kinetic energy TKE (Raschendorfer 2001) including effects from subgrid-scale condensation and from thermal circulations. The Kessler scheme (Kessler 1969) is used for the calculation of grid scale clouds and precipitation and it considers the following hydrometeor species: water vapour, cloud droplets, rain, snow, cloud ice, and for CLM2.8 additionally graupel. More details of CLM can be found in Doms et al. (2011).
For the validation of precipitation we used two different observational datasets. REGNIE (REGionalisierung der NIEderschlagshöhen) is a gridded 1 × 1 km precipitation data set developed by the DWD. It is based on daily measurements from around 4,000 stations throughout Germany from 1971 to the present. The gridding strategy includes corrections for orography and the orientation of the terrain in terms of wind exposure (Berg et al. 2013; Dietzer 2003; Bartels et al. 2006). Furthermore, a station dataset with 5 min resolution precipitation gauges maintained by DWD is used. The gauges use the weighting principle and have a lower measurement limit of 0.01 mm (Brommundt and Bárdossy 2007). The station density is generally varying with time, but peaks with a stable density for the period 1997–2004, for which 74 stations are available within the investigation area (Fig. 1b marked by x’s). In order to have a consistent data set in time and space, only gauge data from this time period are used in the analysis.
In order to investigate potential added values of convective resolving scale CLM2.8 versus CLM7, we proceed in two steps. First, we focus on the precipitation statistics between resolutions, and secondly, we examine the atmospheric conditions relevant for convection in order to explain the differences observed in the first part of the analysis. Most of the study is based on the sub-daily scale because a more detailed representation of the spatial pattern should go along with a higher temporal resolution. Besides a better representation of important features such as topography, the main difference among our model runs is the treatment of deep convection, which is parameterized in CLM7 and physically resolved in CLM2.8. Convection is a process lasting usually for few hours; to assess the differences between models and try to understand the underlying reasons a sub-daily scale is necessary.
In the investigation area, precipitation is mainly due to large-scale processes during winter, while in summer convection becomes dominant. Therefore, the first step of the analysis considers both winter and summer seasons (DJF and JJA respectively) to investigate the effects of different horizontal resolutions on precipitation occurring from different synoptic scale. Bias maps and probability distribution plots as well as diurnal cycles are used to evaluate the differences in precipitation between the CLM7 and CLM2.8 simulations. Berg et al. (2012) found that CLM7 produces too much drizzle, which leads to an underestimation of dry days (i.e. days with precipitation less than 1 mm/day) and to an overestimation of low intensities. Therefore, frequency of dry periods and duration of events are also considered in our study.
CLM7, CLM2.8 and REGNIE have different grid resolutions. Therefore, a conservative remapping of CLM2.8 and REGNIE data to the CLM7 grid was necessary to compare the outputs among each other and on equal terms (Berg et al. 2013). The CLM7 resolution is maintained for all data and all analyses. To compare model outputs with station data, the nearest grid point is selected in order to reduce sampling biases in this region of diverse landscape. The same strategy is also applied with the REGNIE dataset. Sensitivity tests were performed for both CLM2.8 and CLM7 on the specific grid point employed. Using the average over five grid points instead of only a single grid point brings a reduction in mean intensity, to be expected when averaging (not shown). However, the shape of the probability distribution and diurnal cycle is kept unchanged, indicating that the results are robust to these types of changes.
Since the station data are available for the 8 year period 1997–2004, which does not completely overlap with the simulated years (1971–1999), the sensitivity of the model and REGNIE results to the chosen time period is also considered. For the REGNIE data set in Fig. 3 and the model simulations in Figs. 3 and 5, the average of their curves for the time periods 1976–1983, 1984–1991, 1992–1999 is plotted. The sensitivity analysis is carried out computing confidence intervals with a bootstrap approach (Efron and Tibshirani 1993) by randomly selecting eight of the years between 1971 and 1999 a large number of times. The standard deviation of these surrogate data is multiplied by 1.64485 to arrive at the 95 % confidence levels plotted in Figs. 3 and 5 as dashed lines and shaded areas. The signal was found robust for around 500 surrogates. In addition, REGNIE data well compare to station data over the overlapping period 1997–2004 on daily base (not shown). Hourly data are less likely to present any significant differences between the periods due to a low signal-to-noise ratio. Thus, the curves for the REGNIE data set in Fig. 3a, b provides a good measure of differences between the periods for all intensities. Note that the paper focuses mainly on the general shape of the intensity distributions (Fig. 3) and the diurnal cycle of precipitation (Fig. 5). For the latter, we find robust results for the timing of the peak and the general shape even for shorter intervals (not shown). Thus a qualitative comparison is certainly possible.
The second step of the analysis aims at investigating differences in the atmospheric conditions leading to precipitation between CLM2.8 and CLM7. Since the main distinction between CLM7 and CLM2.8 is the treatment of deep convection (parameterized or physically resolved), the analysis concentrates on convective precipitation and is thus restricted to the summer period JJA, when convective precipitation is most frequent. In this context, the CLM7_conv simulation was performed to evaluate the influence of the parameterisation at CLM7 resolution on the representation of the atmospheric fields. Therefore, the results from the CLM7_conv simulation only appear in the analysis of the diurnal cycle of precipitation and other selected variables describing the atmospheric conditions.
Although there is no unique recipe for convection, some ingredients should be in place, namely an unstable atmosphere, enough atmospheric moisture and a triggering mechanism allowing the release of the potential energy. In the area under investigation, orography plays a key role in the initiation of convection. In summer mainly “boundary-layer forced” convection occurs (Kottmeier et al. 2008). In addition to the investigation of the atmospheric temperature and water vapour content conditions, simulated CAPE and convective inhibition (CIN; Colby 1984) are used as indicators of the atmospheric degree of stability/instability and thus the potential for convective processes. Note that the analysis is performed on climatological base, meaning that the atmospheric variables are averaged for JJA over 30 years including all weather conditions. Moreover, all the grid points are considered since there is no comparison with observations. The CLM model calculates CAPE and CIN in each grid point independently according to the temperature and moisture of the ascending parcel (parcel theory) and uses the 50 hPa mixed layer (ML) method to compute the air parcel rising. Furthermore, CAPE depends on both humidity and temperature (Emanuel 1994), thus these variables are analysed in more detail using vertical profiles and diurnal cycles. The lifted condensation level (LCL) is calculated to assess the impact of the different boundary layer conditions on the level of base cloud formation. The level of free convection (LFC) is considered in order to estimate how strong the triggering mechanisms for the release of CAPE should be. The investigation also considers cloud cover at both low and middle level (respectively in the range 0–2 and 2–7 km). Differences in the spatial distribution and percentage coverage of clouds in the model simulations could lead to important changes in the atmospheric conditions, such as variation in radiation, temperature and humidity. In addition to enough moisture supply and an unstable atmosphere, a triggering mechanism is necessary for convection. Several studies already pointed out the fact that increasing spatial resolution leads to a better representation of topography, hence wind circulation patterns and resulting vertical velocity (e.g. Barthlott et al. 2006). Since orographic lifting plays a crucial role in triggering convection over complex terrain, the differences between model resolutions in the simulation of the vertical velocity field are assessed in this investigation.
5 Results and discussion
Hereinafter, the results are presented in two steps following the same structure as presented in the method section, since different methodologies are applied for each of them. The first subchapter focuses on the comparison between the model simulations (CLM2.8 and CLM7) and observations (REGNIE and rain gauges) in terms of precipitation statistics for both summer and winter. The second examines the atmospheric conditions in JJA relevant for the occurrence and the development of convection.
5.1 Precipitation statistics
5.1.1 Spatial mean
5.1.2 Intensity distributions
At the hourly temporal resolution, the intensity distributions change character (Haerter et al. 2010). The station data show a probability density function with higher intensities in summer compared to winter, see Fig. 3 (bottom). Note that the seemingly extreme tail of the station curve in winter above about 10 mm/h is due to only a few stations with some extreme events, and is highly uncertain. Both model simulations perform well in the probability of dry hour, i.e. hours with precipitation below 0.1 mm/h. In winter, both CLM7 and CLM2.8 are underestimating (overestimating) intensities above (below) 5 mm/h. In summer, CLM2.8 clearly outperforms CLM7, with probabilities close to those observed for intensities above about 5 mm/h, while CLM7 underestimates (overestimates) probabilities above (below) 5 mm/h.
Figure 4c, d shows scatter plots of the precipitation amount per each event as a function of duration in JJA. The lines in the plots indicate lowess curves (Cleveland and Devlin 1988) fitted to the data. A trivial 1–1 relationship of linear increase of amount with increased duration is shown as a dashed grey line. The observations have a steeper increase of amount versus duration, thus the average intensity of the events increases with longer duration. Such behaviour can be expected from convective precipitation, whereas stratiform precipitation should have a weaker gradient, especially when considering that also non-precipitating times are included in the hourly statistics (although not resolved by the hourly output frequency of the model). CLM2.8, and especially CLM7, show weaker gradients. A possible explanation for this behaviour is connected with low intensity precipitation between 0.1 and 5 mm/h, which are overestimated by the model (Fig. 3d). If a given event is surrounded by low intensity precipitation above 0.1 mm/h, this will both increase the duration of the event (Fig. 4a) and decrease the mean intensity of the event (Fig. 4c, d). For the daily temporal resolution, the intensity will increase as there are less zero-intensities surrounding the events, thus explaining the overestimation of intense events for CLM2.8 in Fig. 3 (top right).
5.1.3 Diurnal cycle
In summer, CLM2.8 produces a main peak at 15:00–17:00 (Fig. 5b), in good agreement with the observations, and a secondary peak occurs around 02:00–03:00. Thus, CLM2.8 sensibly improves the representation of the diurnal cycle in comparison with coarser resolution, creating a pattern, which is similar in shape to observations in summer. Particularly relevant is that CLM2.8 correctly simulates the time of maximum convection, which is the main failure of CLM7. To understand the reasons behind this, we examine in more detail how the models simulate the atmospheric conditions leading to convective precipitation, starting from the instability of the atmosphere, proceeding with the analysis of the vertical profiles of temperature and humidity, cloud cover, radiation and finishing with triggering mechanism of convection. The focus is on the comparison between CLM2.8 and CLM7 while the use of CLM7_conv is limited to help understanding the effect of the parameterisation on the results. In the area under investigation, deep convection occurs mainly in the summer early afternoon when the atmosphere is most unstable and it is almost negligible in the winter period. Therefore, the analysis in the next section is focused only on the summer period.
In spring (MAM) and autumn (SON) precipitation is due to a mixture of local and large scale forcing conditions and thus it is difficult to clearly identify the added values gained in switching off the convective scheme at finer spatial resolution. Nevertheless, a quick overview of the diurnal cycle in spring and autumn is provided for completeness (not shown). In spring, the observational diurnal cycle of precipitation shows a similar picture to the summer, but the intensities are reduced and the maxima occur later. CLM7 postpones the maximum and reduces the peak intensity, but still overestimates the precipitation compared to observations. CLM2.8 presents the same shape as in JJA but the maximum intensities highly overestimate observations. In autumn, the observational diurnal cycle changes completely showing the main maximum at 4:00 and a secondary one around 10:00. CLM2.8 interprets the diurnal cycle quite well, although it slightly underestimates the morning maxima. CLM7 shows only one maximum at 6:00 which is of lower amplitude than either of the observed morning maxima. The differences between the two resolutions are much reduced in this season but are similar to summer.
5.2 Atmospheric conditions relevant for the occurrence of convective precipitation
5.2.1 Precipitation and convection-related indices
CLM7 exhibits maximum instability around 18:00, which is too late when compared with the simulated diurnal cycle of precipitation (Fig. 5). Thus, CLM7 shows a maximum in precipitation 6 h before the CAPE maximum. In CLM7_conv the maximum instability occurs just before its precipitation maximum, but CLM7_conv strongly misrepresents the precipitation diurnal cycle in comparison with observations. Thus, the expected relationship between the atmospheric instability maximum and consequent convective precipitation occurrence is observed only when convection is not parameterised. CLM7 resolution clearly needs a parameterisation in order to correctly represent convective processes, which occur at smaller spatial scales, however, the currently used Tiedtke scheme cannot compete with convection permitting scale.
5.2.2 Temperature and humidity
The evolution of CAPE and CIN strongly depends on the atmospheric temperature and moisture, particularly on their distribution within the boundary layer (Brooks et al. 1993; Crook 1996; Weckwerth 2000; Khodayar et al. 2010). Thus, the temporal and spatial distribution of these variables is investigated in detail for both resolutions. The diurnal evolution of these variables at ~950 and ~850 hPa is similar for both simulations (not shown), but differs in magnitude. At ~950 hPa temperature and specific humidity increase from 06:00 to 12:00 and then remain constant until 18:00 being CLM7 wetter and cooler. At ~850 hPa, temperature rises uniformly from 06:00 leading to a moistening of the atmosphere with CLM7 being drier and cooler. Maximum differences between early morning and evening are in the order of 0.4 g/kg in specific humidity and 3 °C (2 °C) in temperature at ~950 hPa (~850 hPa). CAPE increases during daytime in agreement with temperature and specific humidity variations, especially at the 850 hPa. At this level, CLM2.8 is systematically warmer and wetter.
5.2.3 Cloud cover and radiation
The variations in temperature and humidity among simulations lead to differences in the vertical distribution of: the level of base cloud formation, LCL; the level of free convection, LFC (from where the atmospheric parcels freely rise); and the equilibrium level (EL), or limit of convection (Fig. 7a, b). The wetter and cooler boundary layer of CLM7 simulation results in lower LCL and LFC, in comparison with CLM2.8. The latter conditions affecting CLM7, in addition to lower EL, could result in clouds forming more easily, probably accompanied by low intensity precipitation. The continuous formation of clouds does not allow the increase of temperature and humidity in the boundary layer, thus inhibiting deep convection and consequent heavy precipitation; this could be one of the reasons of the drizzle problem affecting CLM7 (Fig. 4). The higher LCL and LFC in CLM2.8 indicate that the triggering mechanism needs to be stronger in order to lift the atmospheric parcels to the LFC. The vertical distribution of the LFC and EL and their temporal variation, higher EL at 18:00 than 12:00, agree with the diurnal cycle of CAPE shown in Fig. 6a.
The above-described differences are reflected in the extent of cloud cover in the atmosphere. CLM differentiates between low, medium and high clouds. The higher LCL and LFC of CLM2.8, with respect to the CLM7 runs, result in a reduced cover of low level clouds with a maximum difference of circa 10 % units at 12:00 (Fig. 6b). A noticeable increase in mid-level clouds is observed in CLM2.8 at about 15:00, which could be indicative of deeper convective clouds in this simulation. Note that CAPE and precipitation maxima are found in the time period between 15:00 and 17:00. Baldauf et al. (2011) found that nocturnal boundary layer clouds are responsible for simulated drizzle at night and consequentially for an excess of precipitation. In this context, the reduced cloud cover in CLM2.8 at night could be responsible for the attenuation of the drizzle problem.
The cloud coverage could, directly or indirectly, impact on the precipitation distribution in our simulations. For example, modifications of radiation fluxes can affect the diurnal cycle of near-surface temperature (in terms of both timing and intensity). This would lead to changes in the stability of the atmosphere, which could even result in suppression of convective processes. However, an overestimation of cloud cover could be also responsible for the well-known CLM underestimation (overestimation) of shortwave (longwave) net radiation (Jaeger et al. 2008). Note that longwave radiation has negative sign; hence, an overestimation would be compensated by more negative values of longwave radiation. Figure 6c shows that in CLM2.8 the representation of both radiation net components is improved, with respect to the findings of Jaeger et al. (2008), through an increase (decrease) of shortwave (longwave) net radiation in comparison to CLM7. The findings are in good agreement with Langhans et al. (2013). The increase in shortwave net radiation is linked to a strengthening of both diffusive and direct shortwave radiation (Fig. 6d). A higher direct radiation could be related to the reduced cloudiness at 12:00 in CLM2.8 in comparison to CLM7 (Fig. 6b). Nevertheless, the presence of an additional hydrometer species (graupel) in CLM2.8, which is not taken into account by the radiation scheme, could also contribute to this effect.
5.2.4 Upward motion
6 Summary and conclusions
In the present study, we assess the effects of increasing spatial resolution on simulated precipitation and the atmospheric conditions leading to convective precipitation. Especially, we investigate the improvements at spatial scales where it is possible to switch off most convective parameterisations, so-called convection permitting scales. Added values of convection permitting model simulations have been shown by several studies in the NWP field (Mass et al. 2002; Miura et al. 2007; Richard et al. 2007; Lean et al. 2008; Weusthoff et al. 2010; Baldauf et al. 2011). Our study aims to bridge the gap between these findings in NWP mode and climate time scales. In this context, 30 years were simulated at both a 7 km (CLM7) and a 2.8 km (CLM2.8) resolution with COSMO-CLM. The simulations are evaluated over the state of Baden-Württemberg in southwestern Germany, which is a region known for the orographically induced convective precipitation. A precipitation gauge network of high temporal resolution and dense spatial density is used for the evaluation, along with the gridded daily resolution REGNIE data set.
The CLM2.8 and CLM7 simulations show similar results for mean seasonal precipitation, although with some decrease in the wet bias for CLM2.8, especially in summer, and some differences in the spatial patterns, especially in connection with steep orography. Furthermore, CLM2.8 reduces the drizzle problem, which affects CLM7 (Berg et al. 2013). In fact, CLM2.8 better represents the number of dry days in winter as well as in summer, but it is still underestimating this statistic. CLM2.8 performs very well regarding the distribution of hourly precipitation intensities in summer, while in winter it underestimates higher intensities, although an improvement respect to CLM7 is visible. However, at the daily temporal resolution, CLM2.8 severely overestimates the probability of higher intensities, especially in summer. A more detailed analysis of the problem in this season reveals that the mismatch between the results on different temporal scale is due to events lasting too long in the simulation. Our conclusion is that CLM2.8 creates events similarly to observations but it extends them with low intensity precipitation, behaviour leading to an increase of the daily intensities. It is also clear that a monthly or even daily scale normally used to evaluate CLM7 is not sufficient to appreciate the added values of CLM2.8.
The diurnal precipitation cycle of CLM2.8 is strikingly similar to observations concerning the position of the primary afternoon peak in summer. CLM7 shows severe problems for the diurnal cycle, with a strong peak at midday; several hours too early when compared to observations. We show that this behaviour is a direct consequence of the convective parameterisation used, but we also show that parameterisation is still needed at this resolution. The analysis of the diurnal cycle of temperature and specific humidity shows in general similar behaviour between CLM7 and CLM2.8. However, CLM2.8 presents higher humidity in the afternoon, which could be responsible of the more unstable atmosphere in this simulation. An investigation of the CAPE index reveals that the expected link between atmospheric instability and consequent convective precipitation occurrence is maintained only when convection is resolved. The Tiedtke (1989) parameterisation used for CLM7 is shown to largely ignore the physical connection to CAPE. This is in agreement with previous findings of Baldauf et al. (2011), who found that the parameterisation, to some extent, decouples the initiation of convection from the boundary layer conditions leading to it. On the other hand, CLM7 resolution is too coarse to properly solve convective processes. The expected relationship between CAPE and precipitation maximum is found in the additional short simulation performed at 7 km resolution, but with the main convective parameterisation switched off (CLM7_conv). Nevertheless, CLM7_conv clearly fails in representing the diurnal cycle of precipitation. It is clear that the Tiedtke scheme used for convection in CLM is not applicable for the 7 km resolution. Other schemes, such as the Kain–Fritsch scheme (Kain 2004) that better represents higher spatial resolutions (Jones et al. 2004), might be more appropriate.
Through the study of the vertical profiles of humidity and temperature, we found that the different boundary layer conditions in the CLM7 and CLM2.8 simulations lead to a lower LCL and LFC in CLM7 in comparison with CLM2.8. This could result in clouds forming more easily at low levels and thus generating drizzle; a known problem affecting 7 km resolution. At the contrary, higher LCL and LFC in CLM2.8 contribute to the moisture and temperature accumulation especially in the afternoon, causing deep convection and probably higher intensity precipitation. These conditions are likely linked to a reduced low-level cloud cover at 12:00 for CLM2.8, which could be responsible for the increase of both direct and diffusive shortwave radiation. CLM2.8 partially corrects the underestimation (overestimation) of shortwave (longwave) net radiation that according to Jaeger et al. (2008) affects coarser resolution simulations with CLM. CLM2.8 allows a representation of the spatial distribution of vertical velocity more consistent with the orographic features of the area. A more accurate representation of the areas of convergence is a crucial element for the initiation of convection over complex terrains (Barthlott et al. 2006), such as the area under investigation. Moreover, higher spatial resolution leads to substantially higher values of w in comparison with CLM7 up to the daily maximum at 15:00 in agreement with mid-level cloud coverage and convective precipitation maximum.
A problem with CLM2.8 is that the precipitation events seem to cluster into too long events compared to observations, likely due to extending the events with low intensity precipitation. This problem needs to be further analysed in shorter simulations. The large bias in mean precipitation, especially pronounced in winter is present in all three nests of the downscaling simulations. It is thus difficult to state whether the model is producing the overestimations independently at each resolution, or whether the atmospheric state (for e.g. temperature gradient, water vapour content) leading to the precipitation bias is simply carried further to the higher resolutions. The small differences between the simulations in winter are probably due to the dominance of the large-scale circulation, which is not as dependent on higher resolution, and the inactivity of the convective scheme for this season. On the other hand, also the relative small size of the CLM2.8 domain could generate a too strong dependency on the driving coarser resolution in this season.
Our results show clear improvements at convection permitting scale for higher temporal resolution of precipitation. This has great value for many impact assessment models where both high spatial and temporal resolution are necessary, e.g. in soil erosion modelling or urban drainage planning. Taking the step away from convection parameterisation could significantly improve sub-daily statistics of RCMs, and getting the diurnal cycle right for the right reasons could allow for a better insight in expected changes in precipitation extremes of short duration (Lenderink and van Meijgaard 2008).
The authors acknowledge funding, within the KLIWA-project “Bodenabtrag durch Wassererosion in Folge von Klimaveränderungen”, from Bavarian State Ministry of the Environment and Public Health, Ministry of Economics, Climate Protection, Energy and Regional Planning of the German State Rheinland-Pfalz and Ministry of the Environment, Climate Protection and the Energy Sector Baden-Württemberg. The CLM simulations were carried out at HLRS at the University of Stuttgart within the project “High resolution regional climate modelling” (HRCM). The authors are grateful to the German Weather Service (DWD) and to the State Institute for Environmental Protection Baden-Württemberg (LUBW) for data supply and cooperation. We would also extend a great thank you to the CLM-modelling community, particularly H.-J. Panitz from KIT-IMK for assistance with the RCM simulations. Finally, we would like to acknowledge the work of the R Development Core Team (2011), and the developers of CDO.
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