Lasing and Saturation of the LCLS at 1.5 Å Paul Emma, for the LCLS Commissioning Team SLAC National Accelerator Laboratory Aug. 23-28, 2009 UCLA April 10, 2009 The Vision… John Madey, 1971 “…possibility of partially coherent radiation sources in the … x-ray regions to beyond 10 keV.” Linac Coherent Light Source at SLAC X-FEL based on last 1-km of existing 3-km linac 1.5-15 Å (14-4.3 GeV) See J. Galayda Talk Injector (35º) at 2-km point Existing 1/3 Linac (1 km) (with modifications) New e- Transfer Line (340 m) X-ray Transport Line (200 m) Undulator (130 m) Near Experiment Hall UCLA Far Experiment Hall Commissioning Status of LCLS Laser, gun, & injector commissioned: 2007 Linac & bunch compressors commissioned: 2008 First beam through undulator beamline: Dec. 13, 2008 21 undulator magnets installed & ready: April 7, 2009 First lasing at 1.5 Å: April 10, 2009 (first try!) 1.5 Å FEL saturation observed: April 14, 2009 (after BBA) X-ray diagnostics commissioned July 1 – now (not done) Soft x-rays transported into hutch #1 (AMO) Aug. 18, 2009 User operations start Oct. 1, 2009 (commission in Sep.) 132 meters of FEL Undulator Installed All 33 undulators now installed ! H.-D. Nuhn, THOA02 July 22, 2009 First Attempts at FEL Lasing – April 10, 2009… 21 undulator magnets installed (slots 13-33) Reduce peak current to 500 A (normally 3000 A) Observe screen 50 meters past undulator (FEE diagnostics not ready until late June) Insert one undulator magnet at a time. Correct orbit, check field integrals, & spontaneous radiation pattern J. Welch, THOA05 After 10 undulators inserted, we begin to see a smaller spot at center of screen (still 500 A) So we insert 12 undulators and then slowly raise the peak current back to 3 kA… 1.5 Å FEL light! Undulator Gain Length Measurement at 1.5 Å: 3.3 m gex,y 0.4 mm (slice) Ipk 3.0 kA sE/E 0.01% (slice) (25 of 33 undulators installed) D. Ratner, TUOA03 FEL e- Energy-Loss Shows >2 mJ per X-ray Pulse 1.5 Å Also monitor and calibrate gas detector readings 10 MeV/e- (2.4 mJ) initial DEi Dumpline BPMs ~100 meters Horizontal DE = DEf - DEi Dog-Leg BPMs vary FEL power with oscillations & record e- energy loss Vertical Bend final DEf FEL Intensity Jitter 9.6% rms at 1.5 Å over >1 hr > 1 hr klystron trips 1.87 ± 0.18 mJ 30 Hz beam rate, 5 Hz sample rate, 10000 data points, SASE saturation Injector Transverse Projected Emittance ~0.5 mm Exceptional beam quality from S-band Cu-cath. RF gun… Time-sliced x-emittance: 0.4 mm gex 0.43 mm 135 MeV 0.25 nC 35 A gey 0.46 mm D. Dowell, et al. J. Wu, TUPC56 LCLS Machine Layout L0 TCAV0 heater 3 wires 3 OTR L1X 3 wires 2 OTR 3 OTR L1S sz1 L2-linac DL1 BC1 stopper 135 MeV 250 MeV sz2 4 wire old scanners screen + 8 coll’s 4 wire scanners + 6 coll’s m wall gun BC2 TCAV3 L3-linac BSY DL2 4.3 GeV 5.0 GeV 14 GeV 14 GeV vert. stopper dump undulator 14 GeV Accelerator is last 1-km of SLAC linac (14 GeV) RF photocathode gun and off-axis injector Two bunch compressors + ‘laser heater’ Two transverse RF deflectors for time-resolved beam measurements X-band (12 GHz) compression linearizer 4 emittance diagnostic stations + 4 spectrometers Primary and secondary collimation sections Fixed gap, planar, 132-m undulator at 14 GeV + 1-mm res. RF BPMs Near and Far Experimental Halls + 500 m of x-ray transport YAGS2 RF deflector ON energy time Laser OFF σE/E < 12 keV YAGS2 adds Landau damping Laser Heater Working Well Z. Huang, WEOA01 Laser: 40 µJ σE/E 45 keV YAGS2 Laser: 230 µJ σE/E 120 keV Laser Heater Improves FEL Power & Gain Length nominal (6 mJ) D. Ratner, TUOA03 33 undulators & some YAG saturation? Laser heater OFF Heater OFF 0.01% at 14 GeV with compression factor 90 1.5 Å 0.4-mm emit 0.5-mm emit Heater OFF Heater ON Undulator Girder with 5-DOF Motion Control + IN/OUT Beam Finder Wire (BFW) Cavity BPM (<0.5 mm) Quadrupole magnet 3.4-m undulator magnet sand-filled, thermally isolated supports J. Welch, TUPC53 X-translation (in/out) Wire Position Monitor H.-D. Nuhn, THOA02 Hydraulic Level System CAM-based 5-DOF motion control Beam-Based Undulator Alignment H. Loos Measure undulator trajectory at 4 energies (4.3, 7.0, 9.2, & 13.6 GeV) Scale all linac & upstream transport line magnets each time Do not change anything in the undulator Calculate… (Matlab GUI) Move quads and adjust BPM offsets for dispersion free trajectory Iterate… H.-D. Nuhn, THOA02 RESULT: vary energy by factor of 3 trajectory changes by <10 mm Undulator Quadrupole Alignment after BBA Vary each quadrupole magnet gradient by 30% sequentially Record kick angle using both upstream & downstream BPMs, adjusting for incoming jitter Calculate quadrupole magnet transverse offsets Earth’s field effect (0.4 G) 8 mm rms undulators installed (with m-metal) Z (m) <1 mm Undulator Quadrupole Remote Position Control 3-parameter fit to 20 BPMs along undulator (y0, y0, and Dy) Dy = 30 nrad kick due to quad ±4 mm (y0, y0) 0.7 mm backlash <0.5 µm res. Thanks ANL! Undulator Alignment Diagnostics (Stretched Wires & Hydraulic Levels) Measured und. & quad moves H.-D. Nuhn, THOA02 6 x [microns] 4 undulator alignment drift over 3 days Calculated orbit change 2 0 -2 -4 -6 0 5 10 15 20 Girder Numbers 25 30 35 Undulator Taper more than Doubles Power 1.5 Å measured range (|x| 5 mm) Wake (3 kA) 40 MeV Spont. (13.6 GeV) 20 MeV Post Sat. Taper 70 MeV 1% 5-mrad pole cant angle unmeasured range (>5 mm) H.-D. Nuhn, THOA02 Electron Energy Loss & Spread Induced by FEL Gain FEL OFF FEL FELOFF ON Undulator, Dump-Line, and Screen 4.3 GeV, lr = 15 Å, Ipk = 500 A 0.05% allow FEL FEL with with straight orbit suppress oscillation 2.6 mJ @ 830 eV 50 MeV FEL ON 10 MeV loss/e- Longitudinal Wakefields in the LCLS Undulator ±4 MeV 3.0±0.3 kA Sasha Novokhatski, WEPC22; and J. Wu, WEPC24 Measured 1.5-Å FEL Attenuation of Be Solid Attenuators 9 Be Attenuators (0.01-32 mm) Be Attenuator Gas Detector (1 Torr) Log-e (gas-detector) Attenuation length = 3.73 ± 0.08 mm (8.3 keV) Measurements and Simulations for 20-pC Bunch at 14 GeV MEASURED SLICE EMITTANCE 20 pC 135 MeV gex = 0.14 µm 20 pC tested J. Frisch, WEOD01 time-slicing at 20 pC Y. Ding PRL 102 854801 SIMULATED FEL PULSES 1.5 Å, 3.61011 photons Ipk = 4.8 kA ge 0.4 µm Y. Ding Z. Huang Simulation at 1.5 Å based on measured injector & linac beam & Elegant tracking, with CSR, at 20 pC. 15 Å, 2.41011 photons, Ipk = 2.6 kA, ge 0.4 µm Y. Ding Z. Huang 1.2 fs Simulation at 15 Å based on measured injector & linac beam & Elegant tracking, with CSR & 20 pC. First Experiment Has Started Commissioning (AMO) Soft X-Ray Mirror Transport Done Atomic, Molecular, and Optical Science (AMO) Atomic, Molecular, and Optical Science (AMO) This instrument, designed for photons in the 0.8-2.0 keV range, will investigate the effects of the x-ray beam on atoms and molecules: absorption, ionization and subsequent evolution of the electronic structure on femtosecond time scales, and also to investigate the behavior of atoms in excitation states previously impossible to study (e.g., stripped of all K-shell electrons). Problems & Issues X-ray diagnostics installation & commissioning fell behind schedule (1.5 months) X-ray spot size is a bit large for the present mirrors (mis-calculation + technical limits) 120-Hz operation still requires much work (spring or summer of 2010) OTR screens beyond BC1 still unuseable (COTR) Controls commissioning takes time Many smaller issues that need attention: Cavity BPM gain drift >20% over 1-2 weeks No short-bunch (<10 fs) diagnostics Energy change still requires up to 1 hr Comments Hard X-ray SASE FEL works, and works well No blind tuning or unexpected settings required, with lower charge preferred (0.25 nC) FEL starts up quickly after 8-hr mainenance day and is, in fact, difficult to suppress (up to 3.8 mJ observed at 1.5 Å) These results are of course quite welcome, but are somewhat surprising… Many of us were expecting a more difficult struggle, as was the case at the SLC, but this is just the start. Acknowledgements Thanks to… The extraordinary commissioning team at SLAC ! The operations, metrology, engineering, controls, installation, and RF groups at SLAC The tremendous undulator and cavity-BPM team at ANL The x-ray diagnostics team at LLNL John Galayda (project director) for his leadership and confidence in the team And many of you, who have contributed your ideas, comments, and many years of experience toward this revolutionary new light source, 17 yrs after it was first proposed