Title Experiences at FLASH and plans for SPARC

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Title Experiences at FLASH and plans for SPARC Patrick O’Keeffe WUTA 2008, 8 th-10

Title Experiences at FLASH and plans for SPARC Patrick O’Keeffe WUTA 2008, 8 th-10 th October

What I am going to talk about… ØCharacteristics of FLASH and Optical Laser ØMotivations

What I am going to talk about… ØCharacteristics of FLASH and Optical Laser ØMotivations and Scheme for Synchronisation ØMeasurement of synchronisation by Cross-correlation ØPossible experiments at SPARC Patrick O’Keeffe WUTA 2008, 8 th-10 th October

Who am I … EU RTD project “X-Ray FEL Pump-Probe” Grant No. HPRI-CT-1999 -50009

Who am I … EU RTD project “X-Ray FEL Pump-Probe” Grant No. HPRI-CT-1999 -50009 o HASYLAB/DESY (Coordinator) o Dublin City University o CNRS / LURE Host (FEL) Synchronisation Measurements Michael Meyer Funded by the 5 th Framework Programme of the European Commission Presently: Postdoc at CNR/IMIP in group of Lorenzo Avaldi Patrick O’Keeffe WUTA 2008, 8 th-10 th October

Layout at FLASH 250 m RF-gun Final energy Cs 2 Te - photocathode Nd:

Layout at FLASH 250 m RF-gun Final energy Cs 2 Te - photocathode Nd: YLF pulse laser (2 -20 ps; 262 nm) 1010 electrons (1 -3 n. C) Up to 1 Ge. V SASE undulator FLASH 6 modules (each 4. 5 m) 0 = 27. 3 mm; B 0 = 0. 497 T SASE FEL Wavelength of VUV radiation 15 -50 nm, 150 m. J Patrick O’Keeffe Experimental Hall WUTA 2008, 8 th-10 th October

Time Structure of the FEL Patrick O’Keeffe WUTA 2008, 8 th-10 th October

Time Structure of the FEL Patrick O’Keeffe WUTA 2008, 8 th-10 th October

Optical Laser parameters Wavelength: Pulse duration: pulse energy for single laser pulse: 790 nm.

Optical Laser parameters Wavelength: Pulse duration: pulse energy for single laser pulse: 790 nm. . . 830 nm 100 -120 fs ~ 50 µJ (for 800 pulses in macropulse) up to 1 m. J (10 Hz pulse rep. rate) Courtesy: Ingo Will MBI (Berlin) Patrick O’Keeffe WUTA 2008, 8 th-10 th October

Motivations for Synchronisation Motivation: Pump-probe experiments Atomic / Molecular Physics (e. g. dynamics /nonlin.

Motivations for Synchronisation Motivation: Pump-probe experiments Atomic / Molecular Physics (e. g. dynamics /nonlin. processes in VUV/X-ray) Solid state dynamics (e. g. magnetization dynamics, non-thermal melting) Plasma physics (probing high electron densities) Patrick O’Keeffe WUTA 2008, 8 th-10 th October

Synchronisation Scheme. . . hours. . . 100 ms. . . systematic drifts within

Synchronisation Scheme. . . hours. . . 100 ms. . . systematic drifts within the pulse changes from macropulse longterm drifts ~100 fs to macropulse > ps ~ 300 fs 1. 3 GHz and 108 MHz main oscillator Temperature stabilised Cables (300 m) pump - probe laser Klystron Injector laser experiment undulator linac electron pulse compression Patrick O’Keeffe WUTA 2008, 8 th-10 th October

Cross Correlation in ATI of rare gases hwir =1. 55 e. V hwxuv =

Cross Correlation in ATI of rare gases hwir =1. 55 e. V hwxuv = 26 e. V Sidebands (intensity prop. to intensity of IR) Ar(IP) 15. 76 e. V Ar(1 S 0) Patrick O’Keeffe WUTA 2008, 8 th-10 th October

Set-up used in the Hamburg Experiments Patrick O’Keeffe WUTA 2008, 8 th-10 th October

Set-up used in the Hamburg Experiments Patrick O’Keeffe WUTA 2008, 8 th-10 th October

First Experiment - 2005 Cross correlation: FEL 32. 2 nm (50 fs – 40

First Experiment - 2005 Cross correlation: FEL 32. 2 nm (50 fs – 40 m. J) Laser 523 nm (12 ps – 250 m. J) Sideband Intensity = 2% of Main He line Tcross = 12. 0 +/- 0. 4 ps M. Meyer, D. Cubaynes, P. O’Keeffe, H. Luna, P. Yeates, E. T. Kennedy, J. T. Costello, P. Orr, R. Taïeb, A. Maquet, S. Düsterer, P. Radcliffe, H. Redlin, A. Azima, E. Plönjes, and J. Feldhaus PHYSICAL REVIEW A 74, 011401 R 2006 Patrick O’Keeffe WUTA 2008, 8 th-10 th October

Second Iteration! Cross correlation: FEL 13. 8 and 25. 5 nm (15 -20 fs

Second Iteration! Cross correlation: FEL 13. 8 and 25. 5 nm (15 -20 fs – 50 m. J) Laser 800 nm (120 fs – 20 m. J) Integrated Intensity of Sidebands = 20 % Tcross = 600 +/- 50 fs (FWHM) Jitter = 590 fs (FWHM) 250 fs (r. m. s. ) P. Radcliffe, et al. , Appl. Phys. Lett. 90, 131108 (2007). Patrick O’Keeffe WUTA 2008, 8 th-10 th October

SPARC vs FLASH SPARC FLASH 500 nm 15 - 45 nm Visible EUV Power

SPARC vs FLASH SPARC FLASH 500 nm 15 - 45 nm Visible EUV Power 400 m. J 150 m. J Temporal Width 2 ps 10 s fs Wavelength Visible : temporal structure via autocorrelation Characteristics of SPARC similar to commercial ps YAG Patrick O’Keeffe WUTA 2008, 8 th-10 th October

Above Threshold Ionisation with SPARC 1015 photons/pulse @ 500 nm 2 ps focussed to

Above Threshold Ionisation with SPARC 1015 photons/pulse @ 500 nm 2 ps focussed to 50 mm 1013 W/cm 2 Mc. Ilrath et al. Phys. Rev. A 35 (1987) 4611 Patrick O’Keeffe WUTA 2008, 8 th-10 th October

IMIP Group experience SPARC Project CNR–IMIP, Poli MI, Uni. Na, Uni. Pd Science 314(2006)443

IMIP Group experience SPARC Project CNR–IMIP, Poli MI, Uni. Na, Uni. Pd Science 314(2006)443 Patrick O’Keeffe WUTA 2008, 8 th-10 th October

Seeding of SPARC Two seeding schemes mentioned in TDR produce: 53. 2 nm =

Seeding of SPARC Two seeding schemes mentioned in TDR produce: 53. 2 nm = 23. 3 e. V 32 nm = 38. 7 e. V Optically based autocorrelation methods become difficult Pulses on the 10 s fs – 100 fs scale Could use cross-correlation methods for characterisation of the temporal structure of the FEL Patrick O’Keeffe WUTA 2008, 8 th-10 th October

Dynamics of Excited Ionic States State of the art of gas phase pump-probe: Soft

Dynamics of Excited Ionic States State of the art of gas phase pump-probe: Soft X-ray–Driven Femtosecond Molecular Dynamics Murnane and Kapteyn and coworkers: Science 317, 1374 (2007); Photons /pulse Patrick O’Keeffe HHG Seeded SPARC ~106 - 107 WUTA 2008, 8 th-10 th October

Acknowledgements Michael Meyer Members of the “X-Ray FEL Pump-Probe” EU RTD project Lorenzo Avaldi,

Acknowledgements Michael Meyer Members of the “X-Ray FEL Pump-Probe” EU RTD project Lorenzo Avaldi, Paola Bolognesi, Roberto Flammini Patrick O’Keeffe WUTA 2008, 8 th-10 th October