melting of tungsten by elm heat loads in the jet divertor
play

Melting of Tungsten by ELM Heat Loads in the JET Divertor Guy - PowerPoint PPT Presentation

Melting of Tungsten by ELM Heat Loads in the JET Divertor Guy Matthews, Gilles Arnoux, Boris Basylev, Jan Coenen,. and JET Contributors G.F.Matthews a , G.Arnoux a , B.Bazylev g , J.W.Coenen b , A.Autrique f , I.Balboa a , M.Clever b ,


  1. Melting of Tungsten by ELM Heat Loads in the JET Divertor Guy Matthews, Gilles Arnoux, Boris Basylev, Jan Coenen,…. …and JET Contributors G.F.Matthews a , G.Arnoux a , B.Bazylev g , J.W.Coenen b , A.Autrique f , I.Balboa a , M.Clever b , Ph.Mertens b , R.Dejarnac i , I.Coffey a , Y.Corre i , S.Devaux c , L.Frassinetti j , E.Gauthier i , J.Horacek d , S.Jachmich h , M.Knaup b , M.Komm d , K.Krieger c , S.Marsen e , A.Meigs a , R.A.Pitts k , T.Puetterich c , M.Rack b , G.Sergienko b , M. Stamp a , P. Tamain i , V. Thompson a and JET Contributors l JET EFDA, Culham Science Centre, Abingdon, OX14 3DB, UK a CCFE, Culham Science Centre, Abingdon, OX14 3DB, UK b Forschungszentrum Jülich, Jülich, Germany c Max-Planck-Institut für Plasmaphysik, 85748 Garching, Germany d Association EURATOM-IPP.CR, AS CR, Za Slovankou 3, 18221 Praha 8, Czech Republic e Max-Planck-Institut für Plasmaphysik, D-17491 Greifswald, Germany f Ecole Central Lyon, Lyon, France g Karlsruhe Institute of Technology, P.O.Box 3640, D-76021 Karlsruhe, Germany h Laboratory for Plasma Physics, Ecole Royale Militaire/Koninklijke Militaire School i CEA, IRFM, F-13108 Saint-Paul-lez-Durance, France j Division of Fusion Plasma Physics, KTH, SE-10044 Stockholm, Sweden k ITER Organisation, Route de Vinon sur Verdon, 13115 Sain-Paul-lez Durance, France l See the Appendix of Romanelli F et al 2014, Proceedings of the 25 th IAEA Fusion Energy Conference, St. Petersburg, Russia EX/4-1, Fusion Energy Conference 2014, St. Petersburg 1

  2. Outline 1. Background 2. The JET melt experiment 3. Simulation of the results 4. Conclusions and future plans

  3. Decision on material for ITER first divertor Risks for tungsten melting in early ITER operation had to be reviewed by IO 3

  4. Bulk W melting well studied in medium sized tokamaks Bulk melting can cause disruptions = dangerous for ITER Bulk melting risk was considered low for ITER divertor due to tile shaping & protection systems ASDEX-Upgrade divertor manipulator

  5. Looking down into the tungsten divertor - after The JET tungsten divertor 2011 Tungsten lamella shaping and As installed divertor protection systems in JET at ITER relevant 2012 inter-ELM heat fluxes After ~3500 pulses ~20Hrs plasma 5

  6. W melting by ELMs QSPA ELM simulations looked worrying for ITER N. Klimov et al., JNM 390-391 (2009) QSPA-T …but plasma pressure lower and B 721 W target higher in ITER (and JET) Plasma  stabilises surface waves flow direction Extrapolation to ITER requires a benchmark for the MEMOS code q  > 2.2 MJm -2 , t ~0.5 ms  3.8 MJm -2 for a 1.5 ms pulse JET is capable of achieving a (ITER minimum t TQ ) similar transient heat-flux at normal incidence 6

  7. Typical temperature rise due to ELMs in JET Geometric factor for a vertical edge ~ × 20 Temperature rise (  C) Surface  T depends Existing data – normal lamellas  T during ELMs mainly on pedestal pressure not ELM size! So increase heating power or I p to raise  T [T.Eich] ITER ~10 5 Pa Pedestal pressure (Pa) 7 7

  8. Outline 1. Background 2. The JET melt experiment 3. Simulation of the results 4. Conclusions and future plans

  9. Exposing a tungsten edge in JET A JET pulse 84779 B q || A B 9

  10. Typical JET W melt pulse 3MA/2.9T 23MW 300kJ ELMs q || ~3GWm -2 ~0.5GWm -2

  11. Limitations of the top IR viewing

  12. Melt pulses are reproducible and no disruptions Special lamella Temperature from IR (  C) Standard (Ref.) lamella Time (s)

  13. 84686 – Before melting q || q || Special lamella 5.5mm Special lamella 5.5mm Special lamella 5.5mm Special lamella 5.5mm LFS LFS LFS HFS HFS 13

  14. After 84724 Special lamella LFS HFS 14

  15. After 84778 Special lamella LFS HFS 15

  16. After 84779 Special lamella LFS HFS 16

  17. After 84781 Special lamella LFS HFS 17

  18. After 84782 Special lamella LFS HFS 18

  19. After 84783 J x B B  J thermionic 5.5mm LFS HFS Erosion: 150-300  m per pulse, 5-10  m per ELM (frequency 30Hz) Total volume moved: ~6mm 3 19

  20. Erosion centres on the ELM footprint T ref (  C) 20

  21. Indirect evidence for W droplet expulsion W droplet event during melt pulse Laser blow off with W target A few droplets reach the main plasma with diameters ~ 100  m - Small perturbations only and no disruptions 21

  22. Outline 1. Background 2. The JET melt experiment 3. Simulation of the results MEMOS = key tool used for ITER predictions Stefan problem in 3D geometry accounting surface evaporation, melting and re-solidification solved by implicit method - Surface power density vs time from IR is the input - Vapour shielding - Temperature dependent thermophysical data applied - Moving boundaries are attached to melt layers - All forces: Gradient of plasma pressure, gradient of surface tension, J x B, tangential friction force [Bazylev TH/P3-40] 22

  23. Power density q || from reference lamellas IR camera T(t) MEMOS 3D Theodor 2D inverse code q n (MWm -2 ) q || = q n / sin  B  Reference lamellas 23

  24. Power density on the special lamella PIC model says: MEMOS input = q n from IR (Theodor) f s >0.6 during ELMs f s iterated to match: evaporation rate, f s ~1 inter-ELM and L-mode synthetic IR image and Planck radiation q || from reference lamellas q n = q || sin   q s Special q s = f s  q || cos  lamella q s = f s  q || cos  24

  25. f s chosen to fit evaporation rate and Planck radiation Temperature #84779 – IR (unresolved) and peak (MEMOS) Melting IR MEMOS f s =1 W evaporation rate from WI (400.88nm) MEMOS f s =0.4 Best fit to all data with f s =0.4 25

  26. W melt evolution #84779 – MEMOS [Bazylev TH/P3-40] f s =0.4 26

  27. Hierarchy of forces – MEMOS [Bazylev TH/P3-40] JET pulse #84779 - MEMOS Surface: -40 to +10  m Surface: -200 to +400  m  m B  m Shadow Melt depth and motion JxB match JET data HFS J 60mm 2.5mm LFS Plasma pressure (6kPa) + Plasma pressure (6kPa) + surface tension gradients + surface tension gradients thermionic emission (JxB) 27

  28. Conclusions W melting by ELMs in JET provided important inputs to ITER: • Shallow melts with a few small droplets ejected but no disruptions • JET melt results are consistent with MEMOS assuming J × B dominant • Unexpectedly large power mitigation factor found for exposed W edge Future JET plans New lamella at 15  : • Fully resolved IR temperature • Grazing field angle / more ITER-like • Simpler geometry 28

  29. Thermionic emission during ELM - MEMOS JET pulse #84779 - MEMOS [Bazylev TH/P3-40] Unlike JET experiment, suppression of thermo electron emission is predicted in ITER due to grazing field angles 29

  30. Larmor radius smoothing - PIC code [Dejarnac NF] Equivalent to f s ~0.8 - Calculated for ELMs only - insufficient to explain f s =0.4 in H-mode - No effect expected in L-mode where we find f s =0.2 30

  31. MEMOS suggests significant vapour shielding …..but we are not able to prove it experimentally due to lack of a consistent physics model for f s =0.4 in H-mode and f s =0.2 in L-mode #84779 31

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend