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HXRSS operation experiences at LCLS
Shan Liu, Torsten Wohlenberg How to edit the title slide Upper area: Title of your talk, max. 2 rows of the defined size (55 pt) Lower area (subtitle): Conference/meeting/workshop, location, date, your name and affiliation, max. 4 rows of the defined size (32 pt) Change the partner logos or add others in the last row. Self-seeding Project Meeting, Shan Liu,
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HXRSS set-up procedure and operation schemes
Outlines HXRSS set-up procedure and operation schemes Undulator radiation damage Tunnel visit and technical discussions (see Torsten’s talk) Summary and future plan Host at LCLS: Jim Welch; Discussions with Juhao Wu, Kun Fang, Jim Turner, Franz-Josef Decker, Alberto Lutman, Heinz-Dieter Nuhn, Yuantao Ding, Yiping Feng, John Amman, Patrick Krejcik, Mario Santana Marc Guetg, et al.; Slides mainly from Alberto Lutman and Heinz-Dieter Nuhn.
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HXRSS GUI Bragg reflected x-ray beam (1.49 Å) Zoomed (40 mm rms)
Courtesy of Paul Emma Bragg reflected x-ray beam (1.49 Å) Zoomed (40 mm rms) Bragg angle calculation tool (taken into account crystal calibration) Any way to increase the image resolution? 500 hours to develop this GUI
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HXRSS crystal calibration
9.1 keV – 7 lines crossing,Yaw = 0.8 deg, Pitch Scan Experiment Theory Courtesy of Alberto Lutman In the analytical formula have been introduced : An initial rotation of the diamond in the crystal holder A tilt of the rotation axis of the yaw and pitch stages Offsets between readouts and actual machine angles Roll = 4.25°, Yaw = 0.014°; Pitch_y = 1.05°, Pitch_z = -0.95°, Yaw_x = -2.5°, Yaw_z = °; offset_pitch= 0.12°, offset_yaw= 0.59°.
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HXRSS Crystal GUI HXRSS Crystal gui allows to:
- select the desired reflections Calculate pitch and yaw angles to have the desired reflections (one or two) at the desired photon energies Sets angles in the machine - Change the crystal calibration parameters Calibration was measured once in January 2013 and never changed. Gives any seeded photon energy within 2 eV. Courtesy of Alberto Lutman
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HXRSS set-up procedures
Standard SASE tuning with taper without crystal Tune on electron beam phase space by looking at XTCAV with wakefield backtracking to U16 Flat phase space distribution at U16 after undulator tuning
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HXRSS set-up procedures
Turn on chicane, steer to reference orbit, check undulator pointing for bent crystal spectrometer. Insert crystal, set crystal angle and find seeding on spectrometer Kick at U16 and use energy vernier to adjust e- energy to get SASE at the desired photon energy Take crystal out and maximize intensity before U16 Insert crystal again tune the signal after U16 Optimize delay (scan with 5 fs/step) Tune on taper + standard tuning (OCELOT/Quad…) minimum 20 min. setup time Spectrum vs energy bpm Spectrum vs energy bpm Energy BPM Energy BPM SASE Crystal in (seeding on 1 color)
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Chicane Residual Field
In phase-shift mode the effect from residual field is corrected by orbit steering (using x and y correctors upstream )
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Undulator Tapering Quadratic taper is normally used in operation
On-line taper optimization program for self-seeding with measured energy distribution under development by Juhao Wu and Kun Fang. Figure shows a regular quadratic taper for seeding starts around und #26
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Different Schemes for Operation
Single bunch self-seeding Single bunch two-color self-seeding (separation within amplification bandwidth) Twin bunch two-color self-seeding (increases achievable separation) Two bunch two-color SASE/self-seeding Single bunch fresh slice two/three-color (self-seeding) FEL with dechirper
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Single-Crystal Two-Color HXRSS Manipulating the yaw angle
pitch First undulator section Second undulator section e - Diamond crystal ψ θ Courtesy of Alberto Lutman pitch angle θ range [45°,90°] * yaw angle ψ range [-2.5°,2.5°] Beam propagation The yaw angle controls the energy separation for the double lines -> important! Larger yaw angle can increase the separation of the two lines! (004) (-1,1,3) (1,-1,3) *Lutman, A. A., et al. "Demonstration of single-crystal self-seeded two-color X-ray free-electron lasers." Physical review letters (2014):
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Twin-bunch HXRSS increases achievable separation
L1S L1X DL1 BLM1 BLM2 L0 Gun Undulator E-BPMs 2-color spectrum Pulse Stacker Few ps delay Tens of fs delay after compression Cathode laser *A. Marinelli, et al. ”Twin-bunch two-color FEL at LCLS." Proceedings of IPAC 2016, TUZA02.
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(unpublished material)
Single bunch fresh slice two/three-color (self-seeding) FEL with dechirper Courtesy of Alberto Lutman (unpublished material) Vertical wakefield kicker Horizontal wakefield kicker Head-tail kick on x Head-tail kick on y FEL Statistics: 746 +/- 125 mJ (250 on tail) 1.03 mJ @710eV Tail Head Tail Lasing Pulse on tail ~ 4 fs ; Pulse on head ~ 17 fs Head Lasing Demonstrated: Pulse duration control Nov (A. Lutman unpublished) Fresh-slice two-color Jan 2016 (A. Lutman unpublished) Fresh-slice self-seeding March 2016 Fresh-slice three colors (6 and 12 May 2016) (A. Lutman unpublished) *C. Emma, et al. “High efficiency, high brightness X-ray free electron lasers via fresch bunch self-seeding." Proceedings of IPAC 2016, MOPOW040.
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HXRSS Scraping Test at LCLS
Courtesy of Heinz-Dieter Nuhn Observation: HXRSS chicane delays greater than 30 fs (3.14 mm offset) trips down stream Beam Loss Monitors (BLMs).
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HXRSS Scraping Test at LCLS
40 fs 10 fs Girder rotation used to “re-center” beams in the bellow thus extending the accessible delay range Problem mitigated at LCLS by bellows replacement: from 9 mm diameter to 11 mm diameter Center of chicane (dipole magnets, BPM and Monochromator) Center of undulator system (beam w/o seeding) Max. offset of 15 mm Our case at E-XFEL: no bellows -> minimum distance to vacuum chamber is 4.5 mm (with 15 mm offset) Minimum distance to the diamond crystal needs to be studied by simulation (important for delay scan)
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LCLS undulator dose Beam halo losses are main source of radiation
Integrated dose by thermoluminescent dosimiters Slope of averages: -4.7×10-5 / Gy Averaged over 1 Gy Intervals Due to mono-chamber misalignment and small bellow aperture Note: LCLS-II collimation is being designed to be orders of magnitude better than LCLS-I * Nuhn, Heinz-Dieter, et al. Undulator Radiation Damage Experience at LCLS. No. SLAC-PUB System beam rate pulse charge beam power E-time <DK/KE> ±(DK/K)tol E-time × (DK/K)tol / <DK/K E> Times better than LCLS-I [] [Hz] [pC] [kW] [GJ/d] [d/GJ] [10-4/GJ] [10-4] [days within tolerance] LCLS 120 150 0.180 0.015 64.3 -0.16 1.5 586 1.0 SXR 300 0.144 0.012 80 3.0 1466 1,000 100 0.40 0.035 29 -0.091 1000 1.9 4,000 1.60 0.14 7.2 -0.023 7.6 1,000,000 30 10 0.10 569 HXR 322 -1.41 956 0.400 116 3.8 -0.435 15 0.39 1137 Beam halo losses are main source of radiation LCLS-I collimation system is too short ( 3 radiation length) and their locations are not optimized-> remove and create halo at the same time Significant particle losses from out-of-time electrons are (dark current) generated in the gun
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Other discussions: radiation safety and aperture limit
Fluka simulation performed including whole undulator sections for miss-steered beam at LCLS. Magnet damage experiment performed at LCLS -> scaling factor of 70 kGy/% obtained -> 700 Gy is the upper limit of radiation dose (with 0.01% tolerance for undulator) -> taken for collimation system design of LCLS-II. Minimum gap of dechirper at LCLS-I: 1 mm -> plan for LCLS-II: dechirper with minimum gap of 2 mm? Beam halo study is important to define the minimum aperture -> beam halo measurements may be performed at LCLS.
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Summary and future plan
GUI and tools for HXRSS operation at E-XFEL may be developed in advance (based on the experience from LCLS); Different operation schemes of HXRSS demonstrated at LCLS -> can be applied in the future at E-XFEL; Undulator radiation damage measured at LCLS-I and estimated for LCLS-II can be taken as a reference for GEANT4 simulation.
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Thank You!
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