ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

21
ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

description

ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA. Workshop home page: http://www-conf.slac.stanford.edu/icfa2010 / Plenarvorträge – anklicken Programm der working groups – working group anklicken. Plenarvorträge:. *. Montag: Statusberichte FELs - PowerPoint PPT Presentation

Transcript of ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

Page 1: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

ICFA Future Light Sources workshop1.– 5. 3. 2010SLAC, Menlo Park, CA, USA

Page 2: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

2

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Workshop home page:http://www-conf.slac.stanford.edu/icfa2010/

Plenarvorträge – anklickenProgramm der working groups –

working group anklicken

Working Group 1: Scientific Needs for Future X-Ray SourcesWorking Group 2: Storage Ring-based SourcesWorking Group 3: ERL-based Sources Ati, BettinaWorking Group 4: FEL-based SourcesWorking Group 5: High Brightness Electron GunsWorking Group 6: High-resolution Diagnostics, Timing, and StabilizationWorking Group 7: Undulators, Beamlines, X-ray Optics, and Detectors JohannesWorking Group 8: Novel Source Concepts

Page 3: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

3

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Plenarvorträge:

Montag: Statusberichte FELsFuture performance of the LCLS – J. Welch (SLAC) Progress at the XFELs in Europe and Japan – H. Braun (PSI)Progress in soft X-ray FELs – R. Bartolini (Diamond)Lessons from FLASH - S. Schreiber (DESY)Performance Metrics of Future Light Sources – R. Hettel (SLAC)

Dienstag: Zukünfitge QuellenScience with next-generation soft X-ray sources – S. Wakatsuki (KEK)Science with next-generation soft X-ray sources – F. Parmigiani (ST)X-Ray Detectors for Next-Generation X-Ray Sources-The Fine Art of High-Speed X-Ray

Imaging--Daniel Rolles, CFELRing-based sources overview – M. Borland (ANL)R&D towards an ERL – G. Hoffstaetter (Cornell U.)

*

*

*

Page 4: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

4

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Donnerstag: Diverses

Report from the high brightness electron beams workshop – J. Rosenzweig (UCLA)  Concepts for smaller, cheaper, better – C. Pellegrini (UCLA)Advances in laser/plasma-based sources – W. Leemans (LBNL)Advanced insertion devices; practices and concepts – R. Schlueter (LBNL)Room temperature high rep-rate RF structures for light sources – S. Tantawi (SLAC)

Freitag:

Working Group Summaries

Page 5: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

5

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

James Welsh: LCLS / LCLS 2

First lasing @ 1.5Ǻ, April 2009, first user run Oct.- Dec. 2009

–Availability: 92.9%, 7.1% linac down time and tuning

–70-300fs changing time 1min

–single bunch ,10Hz, 30 Hz,

–0-40GW FEL-power dep. on bunch length

–800-8000eV photon power, changing time 5-30min

–ultrashort pulses, <10fs, changing time 1-2h, 20pC

–pos. jitter < 10% of spot size

–energy fluctuations 3.6% rms / 24h

–Wavelength jitter 0.1-0.2% (2x energy jitter)

Page 6: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

6

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Neue Projekte: second harmonic afterburner8 freie Undulatoren => 0.75Å

Page 7: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

7

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Page 8: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

8

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Page 9: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

9

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

FEL: polarised light echo, self seedingbeam doubler

Page 10: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

10

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Page 11: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

11

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Hans Braun: Progress at the X-FELs in Europe and Japan

Soft-x ray FELS: Max-Lab, Shanghai

Page 12: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

12

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Dominierendes Thema: Welcher Quelle gehört die Zukunft?

Speicherring FEL ERL

Robert Hettel – „Flux und Brightness reichen nicht aus, „neue Kriterien nötig“Mike Borland – APS setzt zunächst auf APS-Upgrate, danach eher auf USR als ERLFulvio Parmigiani – Welche wiss. Fragestellung – welche exp. Technik – welche QuelleGeorg Hoffstaetter – pro ERL Zusammenfassung WG 1…

Page 13: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

13

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Robert Hettel: Performance metrics of FLS

Page 14: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

14

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Page 15: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

15

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Mike Borland: Overview of Ring-Based X-ray SourcesScaling of ring performance – development of ultimate storage rings – symmetry?

Page 16: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

16

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Mike Borland: Overview of Ring-Based X-ray Sources

Page 17: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

17

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Page 18: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

18

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Mathias Fuchs: Laser Plasma Sources - MPQ

Page 19: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

19

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Mathias Fuchs: Laser Plasma Sources - MPQ

Page 20: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

20

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Page 21: ICFA Future Light Sources workshop 1.– 5. 3. 2010 SLAC, Menlo Park, CA, USA

21

Beschleuniger Physik Seminar, 23.3.2010, B. Kuske

ICFA Future Light Sources workshop, 1.-5. 3. 2010

Anton Bartey: Summary Wg I: Science Drivers

8 science drivers: rep. rates pulse lengthChemical reactions < 10kHz 1-50fsMolecular movies < 10kHz 1-50fsAtoms to materials 10Hz-1MHz as-psMaterials at mesoscale sing. shot-kHz psMatter in extreme conditions fs / ps-nsCorrelated materials kHz-10MHz as-fsHirarchical biology quasi CW, CW fs / ps pulsesMulti componant materials Folie fehlt

Strong need for choppers for photons at 1.3GHz – R&D