Installation of the Optical Replica Synthesizer (ORS) at FLASH

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Installation of the Optical Replica Synthesizer (ORS) at FLASH

Who and What? G. Angelova, V. Ziemann- Task: Modulator and radiator undulators, participating in the Theoretical simulations with Genesis P. van der Meulen, N. Javahiraly, M. Larsson, Task: The Seed laser, and the Diagnostic devices in the tunnel downstream of the modulator undulator H. Schlarb, M. Yurkov, E. Schneidmiller, E. Saldin, Task: Responsible for the dipole magnets of the chicane, Support structures for all magnets and general construction work such as the building of the laser laboratory where the seed laser will be placed as well as. Theoretical simulations S. Khan, Joern Bodewadt, Task: Design and construction of the laser transport line from the seed laser to the injection of the seed pulse the accelerator vacuum vessel at the vacuum window at the dog leg of FLASH Atoosa Meseck, Task: Theoretical simulations with MAD and Genesis

Cause coherent emission of light pulse in radiator that mimics the longitudinal shape of the electron bunch (optical replica). Why? Measure the longitudinal bunch profile of the femtosecond long electron bunches (Saldin, Schneidmiller, Yurkov: NIM A 539 (2005) 499.) Energy modulation via (v.e) coupling Longitudinal density modulation in chicane

174800 168919 171500 168919 168919 168919 168919 166727 166114 1.5m 1.5m Radiator Steer magnets to Modulator form a Chicane OTR 2 OTR 1 175300 172900 179100 167265

Component List Two undulators and power supplies Chicane Optical stations I and II Laser Transfer Line Seed Laser, Hutch Person-power Good-will Out of the Tunnel In the Tunnel

Undulators Delivery first week of March 2007

HILDA

VERONICA

Mechanical Support In progress- ready middle of March 2007

Water cooling of the Undulators The coil will be cooled with demineralised water The maximum available pressure drop in the magnet is 3.7 bar. The inlet temperature of the cooling water is 30 C The temperature increase in the undulator should be at least 10 C. The maximum flow velocity of the water must be below 2 m/s.

Power supply connections for the undulators +1/4-3/4 +1-1 +1-1 +1-1 +1-1 +1-1 +3/4-1/4 25A (HB available at DESY) 98 A for the ten coils in the middle (KR 120- available at DESY) 74A for last two inner cooils (KR 120- available at DESY) 25A(HB available at DESY)

Chicane Purpose : Transform energy- into density modulation at the laser wavelength Hardware: Steerer magnets at 171.5, 172.9, 174.8, 175.3m Girders for 4 steerer (to form a chicane) 1.5 m between dipoles Power supplies

2 OTR station To analyze the beam profile and the OTR distribution we will have: OTR chambers + window: CF63, CF16 OTR mover,cabling, interlock OTR frame Silicon wafers + Ag coating (extra pair with Al coating)

Optical Station I and II Hardware: Optical table (one per station) Mechanical support for the optical table Optical components on the optical table OTR chamber (one per station) + window, frame, screens, interlock Laser shielding

Optics Station I ORS Chicane @ 173.43m Seed Laser and OTR e - Laser shielding Mirror, motorized Mirror, motorized Beamsplitter Radiation shielding Lens Filter CCD or Quadrant Photodiode Lens Filter Fast Photodiode

Optics Station II ORS analysis @ 182.41m ORS and coherent OTR e - Laser shielding Mirror, motorized Mirror, motorized Telescope, beamshaper Beamdump GL Polariser, adjustable Radiation shielding Filter, adjustable Iris, adjustable Shutter Light shielding Grenouille 8-50USB/8-500USB

Laser Hutch- To be or not to be November 2006 23 February 2007 End of work scheduled for March 2007!!!

Seed laser Peter van der Meulen, N. Javahiraly (SU) and Axel Winter (DESY). The Seed laser will be based on 1550nm Er-fiber oscillator with frequency doubler from DESY As an amplifier we will use CPA2001 Ti: Sapph amplifier from Stockholm University. - Wavelength : 800 nm - Pulse duration : 150 fs - Pump:YAG Laser operating at 10W of 532 nm Seed Laser with: Length = 2 ps (for stable overlap between the el bunch and laser pulse) Energy/pulse=0.25 mj, Peak field = 1.8 108 V/m Width = 0.75 mm (FWHM) Schedule: 1) Building seed laser and oscillator, shipping the oscillator and testing it- Ready 13/03/07 2) Interfacing the Oscillator- Ready 13/04/07, Transportation of the Seed laser- 20/04.07 3) Work in Laser hutch including Laser tests (optical tables, water connections etc.) Ready 04/05/07

Laser Transfer Line 1. Ordering of mirror, lenses, cameras, laser spot position control and virtual beam waist 2. Design, ordering parts, assembly and cabling of motorized mirror holders 3. Design, assembly and installation of the telescope Additional tunnel into the beam tunnel will be drilled near the dogleg 4. Design and installation of tables and transport tubes

The influence of the el. beam properties on the ORS- output Simulation: Comparison between ideal bunch (constant parameter along the bunch) and the more realistic bunch (variation of the beam properties along the bunch). What are the tolerance limits (which betaamplitude, energy chirp and so on, breaks the process? Can we implement an additional angle in the dispersive section to separate the seeding radiation. Electron beam properties Additional info: Atoosa Meseck- BESSY

Conclusions 1. Undulators- Arrive at DESY 06/03/07, Installation- Ready 19/06/07 2. Mechanical support Ready 15/04/07, 3. OTR station elements- Ready 30/03/07, Installation- Ready 25/04/07 4. Optical Stations elements - Ready 09/04/07, Installation- Ready 30/04/07 5. Stereer magnets for Chicane- Prepared, Installation- Ready 23/05/07 6. Laser Building- Ready 30/03/07 7. Seed laser, oscilloscope, tests- Ready 04/05/07 8. Laser Transfer line- Ready 30/05/07 9. Theoretical simulations- In progress 10. Commissioning - July-August 2007

Position of interest, approximately Vacuum window 158.2 Modulator start 167.0 Chicane 171.5, 172.9, 174.8, 175.3 Radiator start 178.2 Existing OTR screens 7match 165.8 (overlap) 3sund1 168.9 (overlap) 2sund3 177.9 (CTR) 5seed 186.9 (extract) 14seed 195.8 Existing BPM 2match 161.2 6match 164.7 (modulator) Q4sund2 175.7 Q3seed 184.7 Q12seed 193. Q20seed 201.7 Existing steering magnets 3match 161.5 (modulator) 6match 165.0 (into modulator) 5sund2 176.3 (into radiator) 3seed 185.3 (out radiator) 12seed 194.3 19seed 200.6

Sketch of the seed laser beamline (length in mm) total length: ~ 24,8 m modulator undulator ~10000 ~2000 laser system vacuum window electron beam Sheet piling tunnel wall??? ~1530 1920 location for telescope ~1200 ~1000 5400 3670

Separating the (strong, mj) seed laser from the (weak, tens of μj) replica pulse Orthogonal polarization from crossed undulators. Modulator vertically polarized. (Separation of the spontaneous radiation from dog-leg dipole with horizontal polarization) Radiator horizontally polarized. Absorb the seed laser in the chicane. Higher harmonics problematic: The TiSa 800 nm has 2nd harmonic 400 nm, which cannot be phasematched in the BBO.