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33rd European Synchrotron Light Source Workshop (ESLS)

29–31 Oct 2025
Synchrotron SOLEIL
Europe/Paris timezone

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Contribution List

22 out of 22 displayed
  1. 20. Registration
    30/10/2025, 08:00
  2. 22. Workshop general information
    Dr Laurent NADOLSKI (SOLEIL)
    30/10/2025, 08:15
  3. 4. SOLEIL report
    Alexandre MOUTARDIER (SOLEIL), Dr Laurent NADOLSKI (SOLEIL)
    30/10/2025, 08:40
  4. 1. ESRF report
    Nicola Carmignani (ESRF), jean-luc Revol (ESRF)
    30/10/2025, 09:10
  5. 11. ALBA report
    Ferran Fernandez (ALBA Synchrotron), Ubaldo Iriso (ALBA-CELLS)
    30/10/2025, 09:40
  6. 3. PETRA report
    Michaela Schaumann (DESY)
    30/10/2025, 10:10
  7. 5. KIT report
    Johannes Steinmann (Karlsruhe Institute of Technology), Patrick Schreiber
    30/10/2025, 11:10
  8. 6. DIAMOND report
    Richard Fielder (Diamond Light Source)
    30/10/2025, 11:40
  9. 7. SESAME report
    Maher Attal
    30/10/2025, 12:10
  10. 21. Workshop group photo
    30/10/2025, 12:40
  11. 8. MLS report
    Arnold Kruschinski, Carsten Mai (Helmholtz-Zentrum Berlin)
    30/10/2025, 13:40
  12. 14. MAX IV report
    Stephen Molloy (MAXIV)
    30/10/2025, 14:10
  13. 10. ASTRID2 report
    Jørgen S. Nielsen (Aarhus University, Department of Physics and Astronomy, ISA)
    30/10/2025, 14:40
  14. 12. SOLARIS report
    Adriana Wawrzyniak, Dr Roman Panas (NSRC SOLARIS)
    30/10/2025, 15:10
  15. 13. BESSY report
    Meghan McAteer (HZB)
    30/10/2025, 16:10
  16. 2. SLS2.0 Report (Remote/TEAMS)
    Masamitsu Aiba
    30/10/2025, 16:40
  17. 9. ELETTRA report (REMOTE/TEAMS)
    Emanuel Karantzoulis, Stefano Krecic
    30/10/2025, 17:10
  18. 15. Discussion
    30/10/2025, 17:40
  19. 17. Non-Redundant Aperture Interferometry for Full 2D Beam Characterization
    Ubaldo Iriso (ALBA-CELLS)
    31/10/2025, 09:15

    The talk is about a novel way to measure small beam sizes (emittances) by using multiple hole interferometry, based on a Non-Redundant Aperture mask.

    The technique comes originally from the radio-astronomy, and with small variations, has proved to work well at ALBA in the field of accelerators. Furthermore, the technique allows other benefits that can potentially be applied in other...

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  20. 18. ThomX light source: commisioning and operation
    Nicolas Delerue
    31/10/2025, 09:45
  21. 16. Quadrupole variation (QV) beta function measurement at SLS2.0
    Jesus Avila Pulido (Paul Scherrer Institut PSI)
    31/10/2025, 10:15
  22. 19. Closeout
    Dr Laurent NADOLSKI (SOLEIL)
    31/10/2025, 10:45