Multi-Model Ensemble Wake Vortex Prediction
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1 Multi-Model Ensemble Wake Vortex Prediction Stephan Körner *, Frank Holzäpfel *, Nash'at Ahmad+ * German Aerospace Center (DLR) Institute of Atmospheric Physics + NASA Langley Research Center WakeNet 2015, Amsterdam
2 DLR.de Chart 2
3 DLR.de Chart 3 Revision of P2P - Motivation wake vortex descent 1 88 landings 2 Γ*=Γ/Γ0, z*=z/b0, y*=y/b0, t*=t/t0 b0 = initial vortex spacing w0 = initial vortex descent speed 70 landings
4 DLR.de Chart 4 Revision of P2P wake vortex descent prim. vortices b0 - secondary vortices weakened by 30 % after first orbit (0.28 * Γ0) - tertiary vortices weakened by 30 % from the beginning (0.28 * Γ0) sec. vortices ground 2 image vortices - vortex-ground interaction above b0: not yet further investigated - vortex ground interaction not only distance but also time dependent?
5 DLR.de Chart 5 Revision of P2P bias= model - observation
6 DLR.de Chart 6 Revision of P2P
7 DLR.de Chart 7 Multi Model Ensemble Sugar How to mix several good ingredients? Water Lemon Juice Lemonade
8 DLR.de Chart 8 Why not use the best ensemble member exclusively? Why not use the best ensemble member exclusively? which is the best member? in average best performing member can sometimes be the worst one y y t y t t Can an ensemble outperform its best member? success of ensemble appr.: any model can be the best sometimes consistently low performing models no increase of skill Yes! Hagedorn et al., 2005
9 DLR.de Chart 9 Ensemble Members NASA-DLR cooperation D2P deterministic output of P2P based on decaying potential vortex, adapted to LES results (DLR) TDP 2.1 considers effect of crosswind shear on vortex descent (NASA) APA 3.2 decay and transport model according to Sarpkaya (NASA) APA 3.4 reduced effect of stratification (NASA) Probability that one of the models delivers the best forecast (in ground-effect, on the basis of rmse for 99 example cases)
10 DLR.de Chart 10 Multi-Model Ensemble Reliability Ensemble Averaging (REA) model performance (a-priori) model convergence iteration loop Giorgi and Mearns, 2002
11 DLR.de Chart 11 Multi-Model Ensemble Reliability Ensemble Averaging natural variability RD,i depends on distance to ensemble mean: z z ensemble mean if bias or distance to ensemble mean < nv model reliable (RB,i or RD,i = 1) natural variability t t nv = model resolution limit
12 DLR.de Chart 12 Multi-Model Ensemble Reliability Ensemble Averaging uncertainty bounds: reliable less reliable uncertainty bounds depend on ensemble spread weighted ensemble average fi according to Giorgi and Mearns, 2002
13 DLR.de Chart 13 Application to Wake Vortex Models Reliability Ensemble Averaging Training RB,i and RD,i mixture of landings from WakeFRA, RB,z,i(t), RB,y,i(t), RB,Γ,i(t), RD,z,i(t), RD,y,i(t), RD,Γ,i(t) Δt*=2 t0 separately for luff and lee vortices weights for reliability factors: RB,z,i : m=1.0, RD,z,i : n=0.3 WakeMUC and WakeOP 95 selected cases Uncertainty envelope initial condition uncertainty added (not considered in original approach): variable variable unit unit σ (standard (standard deviation) deviation) variable true airspeed air density weight z0 y0 [m/s] [kg/m³] [kg] [m] [m] if initial conditions derived from lidar: z0 y0 Г0 unit [m] [m] [m²/s] σ (standard deviation)
14 DLR.de Chart 14 Application to Wake Vortex Models REA natural variability, Γ* N* ε* v* = N*t0 = (ε *b0)1/3/w0 = v/w0
15 DLR.de Chart 15 Application to Wake Vortex Models REA natural variability, z*
16 DLR.de Chart 16 Results REA forecast (one single landing) 89.1 % 89.1 % 69.7 % 75.6 % enhancement: rmse z*,tdp=0.158 rmse z*,rea=0.148 rmse Γ*,D2P=0.085 rmse Γ*,REA=0.072 probability levels according to - 99 testcases - WakeFRA & WakeOP 62.9 % 62.6 %
17 DLR.de Chart 17 Results REA reliability factors (one single landing) no correlation between RD and RB can be found!
18 DLR.de Chart 18 Results REA scoring 99 randomly chosen cases skill factor s: median 2nd best best
19 DLR.de Chart 19 Results REA scoring 99 randomly chosen cases skill factor s: 2nd best best median advanced MME approach outperforms Direct Ensemble Average (DEA)
20 DLR.de Chart 20 PDD of models and ensemble overconfident ensemble: ensemble spread too low well-dispersed ensemble: coverage of full spectrum of possible solutions Weigel et al., 2008, Hagedorn et al.,2004 overconfident ensemble small or no rmse improvement well-dispersed model forecasts rmse improvement
21 DLR.de Chart 21 Conclusion ensemble can improve quality of wake vortex forecasts on average however only 1.6 % improvement compared to best model reasons: - ensemble is overconfident for z* and y* - uncertainties from env. and natural variability dominate model uncertainty but: models might behave differently in particular ambient weather conditions and out-of-ground investigation with pdds
22 DLR.de Chart 22 Further Development How does a good training data set look like? Can the results be further improved by distinguishing various weather conditions? How does the Bayesian Model Averaging (BMA) perform? source: Raftery et al., 2005
23 DLR.de Chart 23 Backup
24 DLR.de Chart 24 Results REA forecast reliability (one single landing) low reliability for y - forecast high reliability for z - forecast medium reliability for Γ - forecast
25 DLR.de Chart 25 Wake Vortex Predictions Motivation - optimization of tactical separation at airports 1 - hazard warning system Wake v traject ortex ory - Wake Encounter Avoidance & Advisory System (WEAA) 2 - Free Flight
26 DLR.de Chart 26 Ensemble Methoden Bayesian Model Averaging P(B) = Wahrscheinlichkeit des Eintretens von B P(B A) = Wahrscheinlichkeit für B, unter Vorraussetzung A PDF = Probability Density Function (Wahrscheinlichkeitsdichtefunktion) Law of total probability: Beispiel: Wir befinden uns auf einem Schiff: - wir wollen die Position B bestimmen - 3 Crew-Mitglieder (A1,A2,A3) wissen wie es geht, haben aber unterschiedliche Methoden according to Grimmett and Welsh.,
27 DLR.de Chart 27 Ensemble Methoden Bayesian Model Averaging Law of total probability: A1 A2 A3 Methode s= vn*tn individuelle Wahrscheinlichkeit, dass die Methode Erfolg hat: P(B An) Wahrscheinlichkeit, dass wir A1, A2 or A3 fragen: P(An) P(B)=
28 DLR.de Chart 28 Ensemble Methoden Bayesian Model Averaging Law of total probability: A1 A3 A2 Methode s= vn*tn PDF der Methode (Modell-Unsicherheiten): P(B An) Wahrscheinlichkeit, dass wir A1, A2 or A3 fragen: P(An)
29 DLR.de Chart 29 Ensemble Methoden Bayesian Model Averaging Law of total probability: angewandt auf Vorhersage-Modelle: Annahme: es gibt immer ein bestes Ensemble-Glied An = Modell n B = vorherzusagende Größe BT = Trainings-Daten P(An) = Wahrscheinlichkeit, dass An das beste Modell ist (Gewichtungsfaktor, basierend auf BT) P(B An) = PDF of An alone (Gaussian distribution, given that An is the best forecast) gewichtete Summe von Wahrscheinlichkeitsdichtefunktionen (PDFs) according to Raftery et al.,
30 DLR.de Chart 30 Ensemble Methoden Bayesian Model Averaging BMA applied on 48-h surface temperature forecast (bias corrected) ensemble forecast individual model PDF individual model forecast 90% interval verification source: Raftery et al.,
31 DLR.de Chart 31 Multi-Model Ensemble benefit increase deterministic skill predict forecast skill provide probabilistic forecast
32 DLR.de Chart 32 Multi-Model Ensemble
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