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Storm-Scale Ensemble Forecast Experiment - Fort Worth Tornadic Storm Case

Storm-Scale Ensemble Forecast Experiment - Fort Worth Tornadic Storm Case. Fanyou Kong 1 and Kelvin Droegemeier 1,2 1 Center for Analysis and Prediction of Storms, 2 School of Meteorology, The University of Oklahoma. Domain Setting. 24km (238x150). 6km (180x180). 3km (180x180).

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Storm-Scale Ensemble Forecast Experiment - Fort Worth Tornadic Storm Case

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  1. Storm-Scale Ensemble Forecast Experiment - Fort Worth Tornadic Storm Case Fanyou Kong1 and Kelvin Droegemeier1,2 1Center for Analysis and Prediction of Storms, 2School of Meteorology, The University of Oklahoma

  2. Domain Setting 24km (238x150) 6km (180x180) 3km (180x180)

  3. Ensemble perturbation method • Four SLAF (scaled-lagged average forecast) members: s1, s2; s3, s4 perturbations between previous ARPS forecasts (P1,P2) and current analysis are ± to the analysis • One control member (regular ARPS run): cntl

  4. 3/28/2000 3/29/2000 00Z 06Z 12Z 18Z 00Z 06Z 24 km ensemble 18-hr cntl 24-hr P1 s1 s2 30-hr P2 s3 s4 6 km ensemble 12-hr rad, sat (P1 – cntl) (P2 – cntl) 3 km ensemble 22Z 8-hr rad, sat

  5. 12hr accumulate rainfall ARPS ETA

  6. 3-hr rainfall from 24 km ensemble cntl mean spread

  7. Domain average spread from 24 km ensemble

  8. Domain average spread from 24 km ensemble

  9. 3-hr rainfall from 24 km ensemble cntl s1 s2 s4 s3

  10. 3-hr rainfall probability from 24 km ensemble ≥ 0.1 in ≥ 0.25 in ≥ 0.50 in

  11. 500 hPa Height from 24 km ensemble mean spread

  12. Sea Level Pressure from 24 km ensemble mean spread

  13. Surface Temperature from 24 km ensemble mean spread

  14. 6 km ensemble

  15. 3/28/2000 3/29/2000 00Z 06Z 12Z 18Z 00Z 06Z 24 km ensemble 18-hr 24-hr P1 30-hr P2 6 km ensemble 12-hr cntl rad, sat s1 (P1 – cntl) s2 s3 (P2 – cntl) s4

  16. 1-hr rainfall from 6 km ensemble cntl mean spread

  17. Domain average spread from 6 km ensemble

  18. Domain average spread from 6 km ensemble

  19. 1-hr rainfall from 6 km ARPS ensemble s1 s2 cntl s3 s4 mean

  20. 1-hr rainfall probability from 6 km ensemble ≥ 0.25 in ≥ 0.1 in

  21. 1-hr rainfall probability from 6 km ensemble ≥ 1.0 in ≥ 0.5 in

  22. Hourly accumulate rainfall (mean vs obs) mean

  23. Hourly accumulate rainfall (probability vs obs) Prob ≥ 0.1 in

  24. 3 km ensembles • Test different ways to form IC/BC for individual members • Evaluate ensemble analyses and products suitable for storm-scale EF • Assess value of storm-scale EF

  25. 3/28/2000 3/29/2000 00Z 06Z 12Z 18Z 00Z 06Z 24 km ensemble 18-hr 24-hr P1 30-hr P2 6 km ensemble 12-hr 3 km ensemble 8-hr cntl (method one & two) rad, sat 22Z s1 (P1 – cntl) s2 s3 (P2 – cntl) s4

  26. 3 km Ensembles – Method One • Initiate at 22Z March 28 • Control run from 6km cntl • s1/s2 using perturbation between 24km P1 and control, s3/s4 using perturbation between 24km P2 and control • Run ADAS only once (control run), with NIDS and sat data • Explicit microphysics

  27. Composite reflectivity from 3km cntl(initiate at 22Z)

  28. radar cntl

  29. Method One s1 s3 s2 s4

  30. Method One s1 s3 s2 s4

  31. 3 km Ensembles – Method Two • Initiate at 22Z March 28 • Control run from 6km cntl • s1/s2 using perturbation between 24km P1 and control, s3/s4 using perturbation between 24km P2 and control • Run ADAS for each member, with NIDS and sat data • Explicit microphysics

  32. Method Two s1 s3 s2 s4

  33. Method Two s1 s3 s2 s4

  34. Surface reflectivity (method two) mean spread

  35. Surface reflectivity probability (method two) ≥ 35 dBZ ≥ 45 dBZ

  36. Hourly rainfall (method two) s1 s3 obs s2 s4

  37. Hourly rainfall probability from 3km ensemble(method two) ≥ 0.1 in ≥ 0.25 in ≥ 0.5 in ≥ 1 in

  38. 3 km Ensembles – Method Three • Initiate at 23Z March 28 • Control run from 6km cntl • s1/s2 using perturbation between 24km P1 and control, s3/s4 using perturbation between 24km P2 and control • Run ADAS for each member, with NIDS and sat data • Explicit microphysics

  39. Composite reflectivity from 3km cntl(method three)

  40. Model reflectivity vs radar cntl radar

  41. Model reflectivity vs radar s1 radar

  42. Model reflectivity vs radar s2 radar

  43. Model reflectivity vs radar s3 radar

  44. Model reflectivity vs radar s4 radar

  45. Model reflectivity vs radar mean radar

  46. Surface reflectivity from 3km ensemble (method three) s1 s2 cntl s3 s4 mean

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