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Ensemble dispersion forecasting—Part II: application and evaluation S. Galmarinia,*, R. Bianconib, R. Addisc, S. Andronopoulosd, P. Astrupe, J.C. Bartzisd, R. Bellasiob, R. Buckleyc, H. Championf, M. Chinol, R. D’Amoursg, E. Davakisd, H. Eleveldh, H. Glaabi, A. Manningf, T. Mikkelsene, U. Pechingerj, E. Polreichj, M. Prodanovak, H. Slaperh, D. Syrakovk, H. Teradal, L. Van der Auweram a
IES/REM, Joint Research Center, European Commission, TP 441 21020 Ispra, Italy b Enviroware srl, C.Dir. Colleoni, Pzo Andromeda 1 20041 Agrate Brianza, Italy c Savannah River Technology Center, Savannah River Site, Aiken, SC 29808, USA d NCSR Demokritos, Environmental Research Laboratory, 15310 Aghia Paraskevi Attikis, Greece e / National Laboratory, Wind Energy Dep, P.O. Box 49, DK-4000, Roskilde, Denmark RISO. f Met Office, FitzRoy Road, Exeter EX1 3PB, United Kingdom g Canadian Metorological Centre, 2121 Voie de Service Nord, Rte Transcan., Dorval QC, Canada H9P 1J3 h RIVM, Laboratory of Radiation Research, P.O. Box 1, Bilthoven, Netherlands i German Weather Service (DWD), P.O. Box 10 04 65, 63004 Offenbach a.M., Germany j Zentralanstalt fuer Meteorologie und Geodynamik, A-1191 Vienna, Hohe Warte 38, Austria k NMHI, 66 Tzarigradsko shaussee, Sofia 1784, Bulgaria l JAERI, 2-4 Shirakata-shirane, Tokai, Naka, Ibaraki, 319-1195, Japan m KMI, Ringlaan 3, 1180 Brussels, Belgium Received 16 January 2004; received in revised form 16 May 2004; accepted 26 May 2004
Abstract The data collected during the long-range European tracer experiment (ETEX) conducted in 1994, are used to estimate quantitatively the ensemble dispersion concept presented in Part I. The modeling groups taking part to the ENSEMBLE activities (see, Part I) repeated model simulations of the dispersion of ETEX release 1 and the model ensemble is compared with the monitoring data. The scope of the comparison is to estimate to what extent the ensemble analysis is an improvement with respect to the single model results and represents a superior analysis of the process evolution. r 2004 Elsevier Ltd. All rights reserved. Keywords: Ensemble dispersion modeling; European tracer experiment; Model evaluation
1. Introduction Very few tracer experiments were conducted to date that cover spatial scales of the order of few thousands of *Corresponding author. E-mail address:
[email protected] (S. Galmarini).
kilometers and that can be used for the evaluation of model simulations. Among them the ANATEX (Clark et al., 1988; Draxler and Heffter, 1989; Stunder and Draxler, 1989; Heffter and Draxler, 1989), CAPTEX (Ferber et al., 1986) and the European tracer experiment (ETEX). ETEX, organized by the European Commission, the World Meteorological Organization and the
1352-2310/$ - see front matter r 2004 Elsevier Ltd. All rights reserved. doi:10.1016/j.atmosenv.2004.05.031
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International Atomic Energy Agency was conducted in 1994. It consisted of the release from a location in western France of a passive tracer (PMCH) that was detected by a network of 168 samplers distributed from Norway to Switzerland and eastward, all the way to the Polish-Ukraine border (Fig. 1). Two distinct releases were performed under different weather conditions (usually referred to as ETEX-1 and ETEX-2, Girardi et al., 1998). The ETEX-1 release took place in ‘‘wellbehaved’’ weather conditions and led to a large number of non-zero samples at ground level. So far it has been the most investigated release, often used for model evaluation (Van Dop and Nodop, 1998). With the aim of evaluating the ensemble dispersion concept presented in Galmarini et al. (2004, Part I of this paper), the ETEX-1 release has been chosen as case study. This paper will develop around the following issues: *
*
*
Simulation of the ETEX-1 release by long-range dispersion models operational at several meteorological services and environmental protection agencies in Europe and world wide and participating to the ENSEMBLE project (Bianconi et al., 2004; Galmarini et al., 2004) Use of the ETEX-1 data to evaluate the ensemble dispersion indicators presented in Part I. Comparison of the ensemble analysis with single deterministic model realizations.
The scope of this investigation is the quantitative assessment of ensemble dispersion analysis and the verification of the usefulness of ensemble dispersion prediction in the absence of experimental evidence. The results obtained will be discussed in the context of long
7000000
6500000
6000000
5500000
5000000
-500000
0
500000
1000000
1500000
Fig. 1. The ETEX sampling stations distribution and 0.1 ng m 3 contour of measured cloud at T0+12 (red),+24 (blue), +36(purple), +48 (green), +60 h (black).
range dispersion forecasting for support to decisionmaking.
2. The ETEX first release The first ETEX release took place on 23 October 1994 at 16:00 UTC (T0) from Monterfil southeast of Rennes (F). The weather conditions during the release are described in detail in Girardi et al. (1998). Briefly, a steady westerly flow of unstable air masses produced by a low-pressure system centered on Scotland was present over central Europe. Such conditions persisted for the 90 h that followed the release with frequent precipitation events over the advection area and a slow movement and deepening of the low-pressure system toward the North Sea region. We shall refer to Girardi et al. (1998) and Van Dop and Nodop (1998) for details on the sampling and analysis technique used during the experiment. The tracer dispersion detected at ground level by the sampling network is presented in Fig. 1. The figure shows 0.1 ng m 3 contour of the measured cloud every 12 h up to 60 h after the release. The shape of the cloud reveals a dominant advection in the West-East direction with a rotation of the surface portion of the cloud in the last part of the period to the North–East direction covering an area that extends from Norway to Romania. For the sake of synthesis, in Fig. 1 the clouds at the various time intervals are overlapped, the time evolution of the tracer concentration at specific times can be found in Girardi et al. (1998), Van Dop and Nodop (1998) and will also be presented later in this paper.
3. ETEX and ENSEMBLE In order to test the multi-model ensemble dispersion approach presented in Part I, 11 modeling groups participating to the ENSEMBLE (Galmarini et al., 2004) activity repeated the simulation of the ETEX-1 dispersion case. The simulations were obtained by means of 16 different long-range dispersion models which are listed in Table 1. Most of the models participated already to the ETEX modeling activities (Mosca et al., 1998a; Graziani et al., 1998a, b). Since the present study does not aim at a re-evaluation of the specific model simulations, each model will be identified hereafter by an anonymous code (m1–m16) where the code numbering does not correspond to the listing order of Table 1. The dispersion simulations of ETEX-1 were produced by means of analyzed weather data. The simulation results relate to a regular grid of 0.5 0.5 in longitude and latitude with model output every 3 h. The extension of the ENSEMBLE domain was presented in Part I. In order to compare the model results with the measured concentrations, the first were
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Table 1 Models involved in the ETEX-ENSEMBLE activity Institute
Dispersion model
Type
NWP data
Canadian Meteorological Centre Deutscher Wetterdienst
CANERM GME-LPDM LM-LPDM BPaM4D WSPEEDI (Ishikawa, 1994; Chino et al., 1995) MEDIA MEDIA-nested NAME DIPCOT
E L L L L
GEM Global DWD-GME DWD-LM ECMWF MM5
E E L L
ARPEGE ARPEGE-ALADIN UM ECMWF
DIPCOT EMAP RODOS-LSMC RODOS-MATCH NPKPUFF v.1.1.17 NPKPUFF v.2.0.7 (Eleveld, 2002) LPDM TAMOS TAMOS
P E P L-E L L
ECMWF DWD-GME DMI-HIRLAM DMI-HIRLAM HIRLAM ECMWF
L L L
RAMS3a ECMWF T319L50 ECMWF T319L50
Institut Royal Meteorologique de Belgique Japan Atomic Energy Research Institute Meteo-France Met Office (UK) National Centre for Scientific Research ‘‘Demokritos’’ (G) National Institute of Meteorology and Hydrology (BG) Risø National Laboratory (DK) RIVM, Laboratory of Radiation Research (NL)
Savannah River Westinghouse (US) Zentralanstalt fuer Meteorologie und Geodynamik (A)
L stands for Lagrangian particle model, E for Eulerian model, P for Puff model. The last table column lists the NWP model from which atmospheric circulation data originated.
integrated over a period of 3 h to reproduce the sampling time used during the tracer experiment. The measured concentrations were interpolated to the ENSEMBLE grid resolution for a direct comparison with the model results. The interpolation (Watson and Philip, 1984) consisted of a classical triangulation of the measurements at sampling stations and linear interpolation to the regular grid nodes. The minimum value is 0.001 ng m 3, which corresponds to the tracer detection limit.
4. Single deterministic model performances In order to evaluate the multi-model ensemble approach we first present the behavior of single model results when compared to the ETEX data. For the sake of synthesis, Table 2 gives the Figure of Merit in Space (FMS) of each of the model and the Median Model (Section 5.2) compared to the measurements. The FMS (Mosca et al., 1998b) is the estimate of the overlap (in percentage) at a given time between the modeled and the measured clouds at a defined concentration threshold (in this case, >0.1 ng m 3). Table 2 clearly shows a variability of the FMS as a function of time for a specific model, which in some cases can be very large (for example m5 shows a maximum overlap of 36% at 12 h after the release and a minimum of 5% 24 h later). A large variability is also present model wise for a
specific time interval like in the case of T0+6 with 82% coverage by m14 and 20% by m3 and m6. The values presented in Table 2 are also plotted in Fig. 2. The figure highlights the presence of a group of models with coherent behavior and the presence of four outliers namely m4 and m5, m8, m15. The outliers will not be discarded from the analysis since their results will serve the scope of demonstrating their effect on the ensemble analysis. All model results will therefore be considered in the ensemble treatments presented in the next sections. A more comprehensive assessment of the single model performance is given through a global analysis. It relates the statistical analysis of all couples of measuredmodeled concentration values, at all spatial locations of the domain, and at all times. The three statistical parameters FA2, FA5 and FOEX have been selected for this analysis (Mosca et al., 1998b). FA2 and FA5 give the percentage of model results within a factor of 2 and 5, respectively of the corresponding measured value, while FOEX gives in percentage of modeled concentration values that overestimate (positive) or underestimate (negative) the corresponding measurement. Table 3 shows the three parameters values calculated for all models. The values of FA2, FA5 and FOEX for m4 indicate that something went wrong in the simulation since all values are larger than a factor of 5 and they all overestimate the measured data. This shows that an error has occurred during the simulation (for example a mistake in the definition of the release rate). The results
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Table 2 FMS (in %) of single model (m1–m16) and median model against measured data. Results every 6 h from release start. Threshold value 1.0 e 10 gm 3 Model
T0+6
T0+12
T0+18
T0+24
T0+30
T0+36
T0+42
T0+48
T0+54
T0+60
m1 m2 m3 m4 m5 m6 m7 m8 m9 m10 m11 m12 m13 m14 m15 m16 Median Model
29 73 20 26 35 20 50 41 33 41 45 56 33 82 43 30 62
32 22 37 19 36 20 37 23 39 32 48 30 27 32 26 23 39
33 37 30 25 21 26 33 20 29 34 31 31 29 28 27 15 38
33 31 33 25 17 27 27 16 29 32 27 23 25 28 20 22 29
30 30 29 19 9 26 32 13 31 33 36 21 31 32 20 23 31
34 29 30 25 5 24 31 19 27 38 33 26 36 28 16 19 36
33 30 36 25 11 31 29 23 39 35 36 34 38 35 19 23 43
45 44 44 32 25 44 45 29 48 46 45 44 50 48 25 25 56
46 43 39 32 18 42 39 22 38 45 47 42 38 41 20 12 47
47 41 36 35 12 36 36 22 29 41 30 38 36 41 26 14 43
90 80 70
FMS (%)
60
m1 m3 m5 m7 m9 m11 m13 m15 mm
m2 m4 m6 m8 m10 m12
m14 m16
Table 3 Percentage of couple measured-modeled data within a factor of 2 (FA2) and 5 (FA5). Results for models m1–m16 and median model. All measured-modeled data couples at all times and points in space have been considered. The last column (FOEX) gives the percentage of over-prediction (>0) or underpredictions (o0)
50
Model
FA2[%]
FA5[%]
FOEX[%]
40
of m4 were however retained and treated together with the others since they will allow us to show the robustness of the ensemble dispersion technique.
m1 m2 m3 m4 m5 m6 m7 m8 m9 m10 m11 m12 m13 m14 m15 m16 Median Model
14.25 22.01 19.13 0 13.02 22.91 19.98 8.11 16.47 15.11 15.9 21 21.94 12.34 15.89 21.97 24.14
37.65 45.91 42.04 0 32.72 47.37 42.91 18.08 37.47 35.32 37.76 42.43 45.66 28.35 34.65 44.39 48.38
77 61 55 100 71 2 36 42 11 17 14 34 50 56 11 36 15
5. Evaluation of the multi-model ensemble dispersion indicators
5.1. Agreement in threshold level
In this section we will evaluate two ensemble indicators presented in Part I, namely the Agreement in Threshold Level and the Agreement in Percentile Level. Further to that the concept of Median Model will be introduced as part of the ensemble analysis.
The agreement in threshold level (ATL) indicator is used for the ensemble analysis of the ETEX case study. In particular we will focus on its application to timeintegrated concentration (TIC). As presented in Part I, ATL gives the spatial distribution of the models
30 20 10 0 T0+6 T0+12 T0+18 T0+24 T0+30 T0+36 T0+42 T0+48 T0+54 T0+60
Time intervals from release start T0
Fig. 2. Time evolution of FMS presented in Table 2. Data every 6 h from release start.
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agreement in simulating that a pre-defined threshold level is exceeded. Fig. 3 gives the time evolution of the ATL for TIC every 12 h and for a threshold of 0.1 nghm 3. The figure also shows the 0.1 nghm 3 contour of measured cloud (hatched surface). The distribution of models agreement shows the presence of a large region where 30–100% of the 16 models agree in simulating a threshold excedance. At the external fringes of this region for all time intervals, the presence of areas of low model-agreement (yellow colors) can be seen. This area shows that a number of models over predict the extension of the cloud where TIC is equal or larger than the pre-defined threshold. The overlap of the measured cloud shows a remarkable coincidence with the high agreement (>70%) region during all the simulated period. Apart for the case T0+24 where the composite modeled cloud appears to move faster and more to the northeast than the measured cloud, in all other case, there is no region were the measured cloud overlaps with the low agreement area. This indicates that there is not a single or few models (outliers) that perform better than the ensemble. The result points in the direction of considering the high agreement region as a reliable result bearing a considerable degree of confidence for the determination of the spatial coverage of the cloud. Such a possibility was partly anticipated in Galmarini et al. (2001) where ideal case studies were analyzed but no quantitative evaluation was provided. Another important aspect highlighted in Fig. 3 is the chance of gross error that the analysis of a single model result can produce. The last panel of Fig. 3 shows the ATL of TIC at T0+60 h for the same threshold level. This time, however, the hatched area relates to the result of model m8. As one can see, this model is responsible for the region of low agreement in the forefront of the cloud. An analysis of the dispersion based on this single model results would lead to a large overestimate of the cloud distribution. When a higher threshold value is considered the results do not change. Fig. 4 gives the time evolution of the ATL of TIC at T0+24, +36, +48, +60 h for a threshold value of 2 ng m 3. The threshold value is 20 times larger than the one selected for Fig. 4 and is used here to identify ‘‘hot spots’’. In spite of the patchiness of the measured cloud compared to the composite modeled one, the figure shows a clear overlap of the first with the high agreement region. The results of Figs. 3 and 4 are even more remarkable if one considers that the atmospheric dispersion models used to simulate the case are not strictly speaking independent systems. As a matter of fact they share several aspects, which relate to the meteorological fields used as well as approaches to modeling atmospheric dispersion processes. In spite of these aspects, the model results seem also to show a character of complementarity that allows obtaining a result closer to what was measured when a model composite is considered. This aspect will be
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discussed further on. The results presented show that the ATL is a good indicator for combining several model results in a spatial analysis and that the high agreement region gives a good indication of the cloud spatial coverage. 5.2. Agreement in percentile level and the Median Model Fig. 5 shows the results of the ETEX measurement and agreement in percentile level (APL) (50th and 75th) for surface air concentration at T0+24, +48, +60 h. As presented in Part I, for a given variable, time and a given percentile value (in this case 50th and 75th), the APL gives the variable distribution corresponding to the defined percentile of models. The comparison of the clouds relating to the 50th and 75th percentile of model results with the measured cloud shows an overestimate of both the cloud size and concentration values by the 75th percentile, while the 50th percentile agrees well with the measured cloud. This is particularly evident at T0+48 and T0+60 where the measured ‘‘hot spots’’ are also present in the APL (50th) cloud. Furthermore the spatial distribution of the low concentration values remarkably resembles the measured one. A certain degree of overestimation in the spatial distribution of the cloud is also present in the APL (50th) plot at T0+24, though much more reduced with respect to APL (75th). Fig. 6 gives the overlap of the 0.01 ng m 3 cloud at T0+24, 48, 60 h, produced by the best performing model (m2 as from the results of Tables 2 and 3), the measured cloud and the APL (50th) cloud. It clearly appears that the overlap between the last two is larger than the overlap between the single model cloud and the measured one. When other concentration levels are considered, the horizontal concentration gradient obtained with APL is much closer to the one of the measure cloud when compared to the result of the single model. The results of Figs. 5 and 6 indicate that the 50th percentile of model results may be more representative of the actual cloud evolution than the 75th percentile and the single models. In order to prove it we have calculated the FMS of what will be called the Median Model. The Median Model results are obtained by calculating the median of all model results at all time steps and in all grid nodes. The FMS of the Median Model calculated every 6 h are presented in Table 2. As one can see the FMS is indeed higher than the single model results at almost all time intervals, as also depicted in Fig. 2. In order to generalize the analysis of the Median Model results, the global analysis was also conducted as given in Table 3. FA2 and FA5 are systematically higher that the single model values. FOEX is not the minimum value (obtained from m15 results) though the fourth smallest.
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Fig. 3. ATL of time-integrated concentration at T0+12 (a), +24 (b), +36 (c), +48 (d), +60 h (e) Threshold level 0.1 nghm 3. Colors distribution of ATL obtained from all model results. Hatched surface in the first five panels from upper left: measured cloud at threshold level. (f) Hatched surface cloud modeled by m8 at threshold level.
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Fig. 4. ATL of time-integrated concentration at T0+24 (a), T0+36 (b), T0+48 (c), T0+60 h (d) for a threshold value of 2 ng hm 3. Hatched surface: measured cloud at threshold level.
The choice of the 50th percentile, and consequently of the Median Model, is not casual but based on the results shown in Fig. 7. The figure shows FA2, FA5 and FOEX obtained from a global analysis of a series of percentile values (from 15th to 80th) of the models’ distribution. The model percentiles that give the maximum FA2 and FA5 and the minimum FOEX are between the 40th and the 50th with small differences in the three parameters values within the percentile range. For smaller or larger percentiles than the ones included in this range, FA2 and FA5 decrease rapidly and FOEX shows very large values of under or over-estimates of the measured data. An argument that can be raised against the multimodel ensemble dispersion modeling (EDM) and the use of the Median Model may relate to the selection of the model that define the ensemble, the presence of erroneous results in ensemble distribution and their effect on analysis. In order to demonstrate that,
although such a situation may occur, the ensemble analysis identifies the wrong model results and the Median Model filters them out. The case of the results of m4 is an example of such a circumstance. Since m4 systematically overestimates the concentration values through out the simulation, its results define the upper tail of the model result distribution and do not affect the median values. The same would occur in case of a systematic underestimate. The results obtained by means of the APL indicator and the construction of the Median Model results show that the multi-model ensemble dispersion analysis provides additional information compared to single model results. In spite of the of the use of different meteorological data and the intrinsic model diversity, but at the same time in spite of the fact that the models are not totally independent systems, the Median Model produces the best results and its use seems to increase
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Fig. 5. Comparison of APL and measured surface concentration at T0+24, +48, +60 h. APL values at 50th percentile and 75th percentile of model results.
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50 FOEX 40 FA5 30 20 FA2
%
10 0 0
10
20
30
40
50
60
70
80
90
100
-10 -20 -30 -40 -50 Percentiles
Fig. 7. FA2, FA5 and FOEX obtained from global analysis of various percentile models.
Fig. 6. Comparison of Median Model, best single model results and measurements. Variable: surface concentration; Red best single model result; yellow Median Model; orange ETEX measurements.
the reliability of the single model realization. As one can see the use of the Median Model does not penalize the user of a very good model and it is very convenient for the user of a poor performing one. One should bare in mind that model performance can be a case-dependent property of the model, therefore in the absence of measurements for model validation nobody can say apriori whether a model forecast will be reliable or not. In general the results obtained with the Median Model seem to be more conservative than those produced by single models. Once again the ensemble analysis tends to indicate a complementarity of the various model simulations in producing the Median Model results. When combined in the Median Model, the single model results provide an estimate that is superior to the single deterministic model simulation. The concept of complementarity of model results needs however to be demonstrated. In a set of 16 model simulations, the presence of two sets of constantly good model results in the ensemble may bias the analysis and the whole concept, since they would always contribute to the definition of the Median Model. In order to show that no specific model result dominates, we have determined the relative contribution of all the models to the median. Having selected a representative range of concentration values defining the ETEX measured data (0.1–1.0 ng m 3), the number of times a specific model contributes to the median definition was calculated, regardless of the point in space or the instant in time in which this happens. The results are presented in the histogram of Fig. 8 where the contributions are normalized by the maximum value obtained. Apart from m4 that never contributes to the median as expected, all the other models do with varying
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evolution of the measured and the Median Model concentrations at the same locations presented in Figs. 9a and b. The results have dramatically improved with respect to the single model results for both the concentration maximum, trend, TOA and TOD.
Normalised contribution to the median
1.2 1 0.8 0.6 0.4
6. Discussion
0.2 0 m1 m2 m3 m4 m5 m6 m7 m8 m9 m10 m11 m12 m13 m14 m15 m16 Model code
Fig. 8. Contribution of various models (m1–m16) to the determination of the 50th percentile. Values calculate for concentrations range [0.1–1.0 ng m 3]. Values normalized to the maximum contribution.
proportions. Therefore at various instants of the dispersion simulation and at various points in space, all model results alternatively contribute to define the Median Model simulation. The results of Fig. 8 were obtained also for other ranges of concentration values. However, no dominant sub-set of models was determined. 5.3. Time analysis: Median Model against single model After the space and global analysis presented in the previous sections, the time analysis at fixed locations is presented here. Again if dispersion model results are used for support to decision-making, the accuracy of the prediction at single location is very important. The aim of this section is to show that once more the analysis of single deterministic model results could be deceiving while the ensemble treatment could produce more reliable results. When analyzing time series at specific locations, other than the evolution in time of the concentration value, two more aspects are relevant in evaluating a model performance, namely time of arrival, TOA (departure, TOD) of the cloud to (from) the sampling location. Figs. 9a and b compare the time series of ETEX measurements at eight locations of the domain with the results produced by the single models. The locations have been chosen through out the domain in order to show various stages of the cloud evolution from very close to the source point to large distances. As Figs. 9a and b show, the various models give a variety of time evolutions of the cloud ranging from very poor to good performances when compared to the measured time series. While the maximum concentration values at the various locations are rather well reproduced by the majority of the models except of m4, the time evolution of the concentration shows a variety of trends, TOA and TOD values. In particular the last two are over or underestimated by several hours. Fig. 10 gives the time
The results obtained in this study show that use of the various indicators presented in Part I provide a wider and better perspective on the process evolution than the ones obtained by analyzing a single deterministic case. The deterministic simulation is in general assumed to be correct but unfortunately it still includes a level of uncertainty that is too high for the scope for which the model results are used. The statistical treatment proposed with EDM seems however to reduce this uncertainty. EDM and the use of the indicators presented can also be considered a valuable approach to the reduction of the risk for gross errors (the case of m4 serves as an example in this respect). As shown earlier the Median Model provides better results than the single models but at the same time, if modeling is finalized at decision making or regulatory purposes, the use of APL at larger percentile values provides a more conservative identification of the cloud extension that can better serve the scope of civil protection and countermeasure adoption. At present we are not in the position of providing a rigorous explanation on why the Median Model should perform better then the single models. However, we may try to propose a hypothesis that still needs to be verified by future research. The results of a dispersion model depend on the model concept and the meteorological data used to simulate the dispersion. Although a certain degree of uncertainty is present in both elements, atmospheric circulation models and dispersion models are based on atmospheric physics laws and principles that bound the solutions. One could therefore think of the various model simulations as a family of realizations that take into account, with different emphasis, the various physical aspects of the actual dispersion process. Therefore, the analysis of the ensemble of model results in terms of composite of the various model simulations at the various points in space and time is more conservative, filters the single model differences and it is finally more consistent with the actual evolution of the process. By definition, the median is less sensitive to extreme scores and it is a better measure for highly skewed distributions. The Median Model thus filters extreme results and when performed at each point in space and time, reduces the deterministic character of the single realization. Given the present population of model results it is also clear that the use of the mean value would lead to a large overestimate of the
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Fig. 9. Time evolution of atmospheric concentration produced by single model at some locations of the modeling domain (colored lines). Measure concentration (blue line with stars).
concentration levels and it would result inappropriate. In our view the median is more representative indicator of the ensemble results and adequate when no a priori
indication is available on the representativeness of the statistical sample and its distribution. Eventually, provided a larger population of model results, the
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Fig. 10. Time evolution of Median Model results and measured concentrations at locations of Fig. 9.
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skewness of the distribution would reduce, thus making the median tend to the mean.
generalized and placed in a more rigorous theoretical framework.
7. Conclusions
References
The ensemble dispersion modeling technique, presented in Part I, has been evaluated. The European Tracer Experiment case study was simulated by a number of modeling groups participating to the ENSEMBLE activities. A total number of 16 longrange atmospheric dispersion models where used, those are based on different approaches to atmospheric dispersion modeling and make use of different atmospheric circulation data. All model used are operational modeling system used for the prediction of the evolution of accidental releases of harmful materials to the atmosphere. The evaluation of the EDM technique mainly focused on the global analyses and the indicators for the spatial analysis introduced in Part I, namely ATL and APL. In the case of ATL the measured cloud appears to compare very well with the regions of high agreement of models thus showing that the use of this indicator allows the identification of the region where the dispersing cloud is most likely to be. The use of the APL indicator has outlined that the cloud corresponding to the 50th percentile value of model results agrees well with the measured cloud. A more detailed analysis has confirmed that percentile values between the 40th and 50th are the ones that produced at best the evolution of the measured cloud. The Median Model results (obtained using the 50th percentile of all model results at all time and points in space) have been shown to be superior to all single model ones in reproducing the measured cloud. The analysis of the contribution of the single models in defining the 50th percentile has shown that no dominant sub set of models exists but that all models contribute, with different proportion, to the definition of the Median Model results. This showing that a clear character of complementarity exists among the model results. An analysis of the model results at specific locations as a function of time (time analysis) shows that while the single models produce a wide spectrum of time evolution of the concentration, the Median Model, on the contrary, provides a more accurate reproduction of the concentration trend and estimate of the cloud persistence at the sampling location. While in Part I and in this paper the methodology has been presented and evaluated with the ETEX case only, future investigation should relate to the application to other case studies for which measurements are available, for example ETEX-2 (Girardi et al., 1998) and the accidental release of Algesiras (E) (Voght et al., 1998; Baklanov and Sorensen, 2001; Galmarini et al., 2001). Furthermore the conclusions presented in this paper should be
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