Joint project between
Ludwig Maximilians University (LMU) of Munich and Deutscher Wetterdienst (DWD)
LMU: Yuefei Zeng (Scientist), Florian Semrau (PhD student) and Tijana Janjic (PI)
DWD: Axel Seifert (PI)
Data assimilation (DA) on the convective scale uses high-resolution numerical models of the atmosphere that resolve highly nonlinear dynamics and physics. These non-hydrostatic, convection permitting models are in short runs very sensitive to proper initial and boundary conditions. The proper estimates of hydrometeors are crucial for prediction on convective scales. However, their estimation is hampered by assumptions made in data assimilation algorithms and in their models of the observation error and model error uncertainty. The aim of this project is to optimize the use of polarimetric radar observations to initialize numerical weather prediction (NWP) models due to the importance of this data set for the prediction of connective storms. This includes specifying the model error and the observation error for polarimetric radar data during data assimilation.
In the recent work (Zeng et al. 2020), we have compared different methods to represent subgrid-scale model error (WP 1), including small-scale noise, the physically based stochastic perturbation (PSP, Kober and Craig, 2016) scheme for turbulence, and an advanced warm bubble approach. It is found that the combination of small-scale noise and bubble performed the best for the 6-h precipitation forecasts when assimilating radar data as illustrated in Figure 1, in terms of Fractions Skill Score (FSS).
E_BASE: basic experiment using large-scale noise
E_SAN: additionally using small-scale noise
E_SANP: additionally using small-scale noise and PSP
E_SANB: additionally using small-scale noise and bubble,
Figure1: Verification of 6-h ensemble forecasts against radar-derived precipitation rate for comparison of using the FSS the for the threshold value of 5.0 mm/h as a function of forecast lead time for 14 km. The lines are marked with filled dots at the forecast lead times where the differences compared to E_SAN are statistically significant at 95% confidence intervals. In addition, the idealized setup for radar data (not polarimetric) assimilation based on the KENDA system of the DWD has been developed and tested (WP 3). See Figures 2 and 3.
Figure 2: The time evolution (from 13:00 UTC to 00:00 UTC) of reflectivity [dBZ] and horizontal wind (vector [m/s]) at the height of 5 km in the nature run of the idealized setup.
Figure 3: Sensitivity of DA results on the observation operator setting (EMVORADO, Zeng et al. 2016), observation error and observation type, shown by the vertical profiles of root-mean-square error of analysis ensemble mean for u, w, T and qr, averaged over all assimilation cycles. E_Vr: assimilation of radial wind; E_VrD: same as E_Vr but using Desroziers statistics to specify observation error; E_VrD_nzw: same as E_VrD but neglecting reflectivity weighting; E_VrD_ns: same as E_VrD but neglecting beam smoothing; E_VrD_nw: same as E_VrD but neglecting the fall speed; E_Z: assimilation of reflectivity
This work has been and will be presented at several conferences:
1) Results from idealized setup and from Zeng et al. 2020 will be presented at EGU 2020 and ISDA 2020.
2) Oral presentation: “ Representation of model error in convective scale data assimilation”, Tijana Janjic, AGU, 9-13 Dec. 2019, San Francisco, USA.
3) Invited talk: “Representation of model error in convective scale data assimilation”, Tijana Janjic, Mathematics of the weather, 14-16, Oct. 2019, Bad Orb, Germany.
Contribution of Yuefei Zeng
The problem of including the model error in data assimilation is twofold. First, the model error must be included in the data assimilation algorithm, and second, the error must be quantified through its statistics. In recent work, in order to represent the errors of unresolved scales and processes, we have produced COSMO runs with 1.4 km and 2.8 km horizontal resolution for a convective period (see Figure 3). These are used as samples in our new implementation of additive inflation that aims to mitigate small scale errors of COSMO. However, with these, we are not perturbing hydrometeors, but only horizontal wind, temperature and humidity (Zeng et al., 2019). Therefore, we are currently not examining errors in hydrometeors and in the microphysical scheme. Experiments with the second moment scheme and 1.4 km horizontal resolution will be carried out in order to obtain samples that include errors of the microphysical scheme. However, it is possible that additive inflation is not the optimal way to perturb hydrometeors. Therefore, other possibilities, such as perturbing parameters of the microphysical scheme will be investigated.
Figure 3 (adopted from Zeng et al. 2019): Samples η(i) calculated for historic case in 2014 (left); Spectrum of small-scale perturbations (level 10 = 13 km and level 30 = 3 km, right)
It has been shown that accounting for correlated observation errors leads to a more accurate analysis and to improvements in the forecast skill score (Weston et al., 2014; Bormann et al., 2016). Even the use of a crude approximation to the observation-error covariance matrix may provide significant benefits. However, the representation of spatial correlations is not straightforward. A number of approximated forms of spatial correlation matrices (or their inverses) have been proposed in the literature to increase numerical efficiency while preserving observation information content and analysis accuracy (Healy and White, 2005; Fisher, 2005; Stewart et al., 2008; Stewart, 2010). Since polarimetric radar observations have correlated observation errors, we will investigate this approach adapted to polarimetric radar data and modify LETKF accordingly.
Here we will use an idealized setup of COSMO–KENDA. Simulated observations of polarimetric radar data will be drawn from a nature run. By observing the truth, we can try to predict the location and intensity of the storms by using LETKF. Similarly, we will explore the use of retrievals, namely the drop size distribution (DSD) (Raupach and Berne, 2017; Brandes et al., 2004) which is an alternative approach to feed polarimetric information into the double-moment microphysics of the model. The benefits of including correlated observation errors will be investigated. By using different levels of microphysics schemes in the nature run and the assimilation, we will investigate the effects of model errors and how this behavior can be improved.
Contribution of Florian Semrau
During data assimilation in addition to model error statistics, observations including representation error statistics need to be specified (Janjic et. al 2018). The observation operator error is an intrinsic part of the representation error because the dynamical model dictates the discrete observation operator. Therefore, since we do not have a perfect observation operator but only its approximation, even if the sub-grid scale part of the signal is zero, there are other observation operator errors associated with the numerical discretization of the operator. One could argue that the representation error would diminish as the model’s resolution increased. However, as the model’s resolution increases, more processes are resolved. For example, Figure 4 compares the forecasts of the ICON model with 2.2 km and 1.0 km resolutions to radar measurements. As illustrated in the figure, the differences between both the 2.2 km and 1.0 km model forecasts and the observations are still very large, indicating that the representation error would make a large contribution to the observation error if these data sets were to be assimilated.
Figure 4: Simulation of radar reflectivity composite from ICON 2.2 km (left) vs 1.0 km (middle) vs radar observation (right) at 14:00 UTC, June 05 2016. No data assimilation
First, we will start with estimation of statistics of error due to unresolved scales and observation operator in idealized setups from higher resolution simulations. These will be compared with Desrozier (2005) estimates. Finally, the representation error will be parameterized . Grooms et al. (2014) suggest the use of stochastic physics for the mean and covariance of the unresolved scales. The use of the stochastic superparametrisation that is time varying improves significantly the results in their experiments. Although not design for the representation error statistics, we will explore stochastic parametrization of Sakradzija et al. (2016) for representation error of polarimetric measurements.
To include representation error in the LETKF algorithm, first the possibility of correlated observation error in LETKF need to be capacitated. The methods for including part of representation error in the Kalman filter framework, namely the error due to unresolved scales and processes, were presented in Janjic and Cohn (2006).
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