Assimilation of Wind Power Data to Improve Numerical Weather Prediction and Wind Power Prediction

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1 Assimilation of Wind Power Data to Improve Numerical Weather Prediction and Wind Power Prediction Erstellung innovativer Wetter- und Leistungsprognosemodelle für die Netzintegration wetterabhängiger Energieträger - Eine Kooperation von Meteorologie und Energiewirtschaft - Stefan Declair EWEA Technology Workshop Wind Power Forecasting Rotterdam, December 3 rd 2013

2 Energiewende in Gemany: Haves and Wants 2

3 3

4 Who is EWeLiNE? 4

5 Agenda 1. Data Assimilation 2. Data Situation 3. Impact-Study 5

6 Agenda 1. Data Assimilation 2. Data Situation 3. Impact-Study 6

7 Forecast: Can i cross the street without getting hit? Information used: Observations Knowledge about cars, street, etc Experience statistics Forecast errors due to: Observation (estimation) errors Model errors (icy street) Case does not match statistics 7

8 8 LETKF Goal: compute a best-fit initial state for the next model integration step Method: Local Ensemble Transform Kalman Filter Local: localizes spatially around observations Ensemble Transform: works in ensemble space Kalman Filter: tracks means and covariances ) ( ) ( ~ 1 b o b o b a a y y K y y R Y P w T 1 1 1) ( ~ b b T a Y R Y k P ) ( ) ( i a b b i a w X x x b T a b a X P X P ~ )] ( [ )] ( [ ) ( 1 1 x H y R x H y X P X x J o T o b T b b minimize in S transform to observation space ~ Cost function to minimize

9 KENDA Kilometer-scale Ensemble Data Assimilation Priority program within COSMO consortium LETKF for the nonhydrostatic COSMO-DE model of DWD Implementation following Hunt et al., 2007 Basic Idea: perform the analysis in the space of the ensemble pertubations computationally efficient, but also restricted to do corrections to space spanned by the ensemble explicit localization analysis ensemble members are local linear combinations of the first guess ensemble members 9

10 10 KENDA R o-fg o-fg LETKF LETKF LETKF < o-fg o-fg P b K

11 Forward Operator Process chain 11

12 Forward Operator Powercurve Fit 12

13 Forward Operator - Example Input Wind speed/direction from COSMO-DE Analysis Power observations Cost function Depending on orthogonal distance between data points and objective function Results Wind direction sector RMSE=10.1% 13

14 Agenda 1. Data Assimilation 2. Data Situation 3. Impact-Study 14

15 Data - Haves 68 wind farms, node-sharp 15min resolution/10min delay Average hub heights, farm point of mass Installed farm nominal power 15

16 Data - Comparison Wind observations University of Hamburg Height m Available from 2005/01/01 10min temporal resolution Power observations Reference wind farm Average hub height 67m Available from 2012/01/01 15min temporal resolution Reference wind farm Tower Hamburg approx. 47km 16

17 Data - Comparison 17

18 Data - Comparison Jahrespeak (mit viel Phantasie) 6h-Peak 24h-Peak 12h-Peak 18

19 Data - Wants Additional information needed Average hub distance Average blade radius Hub alignment Information content outside of partial power Hub activity Losses between farm (hubs) and nodes account wake effects increase information density because all the uncertainties enter the LETKF via the observation error covariance matrix reduce uncertainties 19

20 Agenda 1. Data Assimilation 2. Data Situation 3. Impact-Study 20

21 OSSE Observation System Simulation Experiment Goal: Test the impact of newly available observations in the data assimilation Method: assimilate artificial observations in slightly perturbed truth Advantages: Truth is known exactly All generated fields can be used as observations Observation system can be altered easily Observation errors Observation densities Temporal resolution/delay 21

22 OSSE Observation System Simulation Experiment Current state artificial wind obs* from model run nature run disturbed run w/ obs* * obs: wind observations at average wind farm hub height control run w/o obs* 25

23 Conclusion Data assimilation KENDA: LETKF data assimilation scheme in COSMO-DE Forward operator: lookup table approach in progress Data situation Available data are of good quality More detailed information necessary to reduce uncertainty for LETKF OSSE Determine the impact of a new observation system Work in progress Thank you for your attention! 26

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