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MICE CM53

21–22 Feb 2019
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Europe/London timezone

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Contribution List

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  1. 1. Analysis Workshop
    20/02/2019, 10:00
  2. 22. Analysis Workshop
    20/02/2019, 13:30
  3. 23. Welcome and introduction
    Kenneth Richard Long (Imperial College (GB))
    21/02/2019, 09:00
  4. 24. Analysis status and plans
    Chris Rogers (STFC)
    21/02/2019, 09:25
  5. 19. Computing Status
    Paul Kyberd (Departm.of Physics(QMW-Coll.))
    21/02/2019, 09:50
  6. 7. System Performance Paper
    Paolo Franchini (University of Warwick - MICE)
    21/02/2019, 11:00
  7. 8. Tracker Performance
    Christopher Hunt (Imperial College)
    21/02/2019, 11:45
  8. 9. Global Tracks and Optical Alignment
    Mr Joe Langlands (University of Sheffield)
    21/02/2019, 12:15
  9. 20. Discussion
    21/02/2019, 12:45
  10. 10. 4D Amplitude Evolution - Rapid Communication
    Chris Rogers (STFC)
    21/02/2019, 14:00
  11. 11. 4D emittance evolution - detailed paper
    Christopher Hunt (Imperial College)
    21/02/2019, 14:45
  12. 12. Discussion
    21/02/2019, 15:15
  13. 14. Optics evolution in the cooling channel
    Mr Paul Jurj (Imperial College)
    21/02/2019, 16:00
  14. 13. Wedge and 6D Emittance Evolution
    Mr Craig Brown (Brunel)
    21/02/2019, 16:30
  15. 15. LiH Scattering Analysis
    John Nugent (University of Glasgow)
    22/02/2019, 09:00
  16. 16. LH2 scattering analysis
    Gavriil Chatzitheodoridis (University of Glasgow)
    22/02/2019, 09:45
  17. 21. Discussion
    22/02/2019, 10:15
  18. 17. Field on scattering analysis
    Dr Alan Young (University of Strathclyde)
    22/02/2019, 11:00
  19. 18. Energy loss analysis
    Scott Wilbur (University of Sheffield)
    22/02/2019, 11:20
  20. 25. Collaboration Board summary
    Paul Kyberd (Departm.of Physics(QMW-Coll.))
    22/02/2019, 11:40
  21. 26. Closing remarks
    Kenneth Richard Long (Imperial College (GB))
    22/02/2019, 12:00
  22. 2. Detailed Emittance Evolution
  23. 5. Global tracks and magnets
  24. 6. Optics evolution in the cooling channel
  25. 3. Tracker update
  26. 4. Wedge and 6D Emittance