The FLASH objective: SASE between 60 and 13 nm

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Injector beam control studies winter 2006/07 talk from E. Vogel on work performed by W. Cichalewski, C. Gerth, W. Jalmuzna,W. Koprek, F. Löhl, D. Noelle, P. Pucyk, H. Schlarb, T. Traber, E. Vogel, FLASH Seminar at June 19 th 2007

The FLASH objective: SASE between 60 and 13 nm 4MeV 130 MeV 380 MeV BC3 BC2 ACC1 ACC2/3 700 MeV bypass 13 nm photon beam-line rf gun laser rf gun accelerating module vertical deflecting rf 1.3 GHz klystron bending magnet undulator bunch compressors beam dump collimator Major prerequisites for SASE 100 fs short bunches obtained by bunch compression for 2 ka peak current small beam energy variations

Short bunches are created by the FLASH injector 4 MeV 130 MeV 380 MeV BC3 BC2 ACC1 ACC2/3 700 MeV bypass 13 nm photon beam-line rf gun laser rf gun accelerating module toroid monitor camera OTR screen 1.3 GHz klystron bending magnet bunch compressors beam dump Bunch compression is sensitive to beam energy variations caused by rf gun laser pulse arrival time variations gun rf phase variations ACC1 rf amplitude and phase variations ACC2/3 rf amplitude variations

The source of the bunches: rf gun laser and rf gun 4MeV 130 MeV 380 MeV BC3 BC2 ACC1 ACC2/3 700 MeV bypass 13 nm photon beam-line rf gun laser rf gun accelerating module toroid monitor camera OTR screen 1.3 GHz klystron bending magnet bunch compressors beam dump laser pulses shoot onto the cathode determine the bunch (timing) structure a stable gun rf phase is required for minimal arrival time jitter at ACC1 emission phase measurement with off crest accelerated beam

Emission phase stability measured with beam Emission phase = phasing between rf gun laser pulses and gun rf indirect rf phase measurement bunch charge depends on rf phase at edge present resolution about ± 0.01 (20 fs) The laser pulse arrival time AND the gun rf phase affect the emission phase!

Creating the laser pulses Diode-pumped Nd:YLF Oscillator Modulators (AOM EOM AOM) 108 Piezo tuning of MHz 1.3 GHz 13.5 MHz cavity length In cooperation of DESY and Max-Born- Institute, Berlin, I. Will et al., NIM A541 (2005) 467, S. Schreiber et al., NIM A445 (2000) f round trip = 27 MHz Faraday isolator Pulse picker Pockels cell Stabilized by quartz tubes E pulse = 0.3 µj Fiber-coupled pump diodes E pulse = 6 µj Diode pumped Nd:YLF amplifiers Fast current Pulse control picker Flashlamp pumped Nd:YLF amplifiers Faraday isolator Relay imaging telescopes Fast current control LBO BBO E pulse < 0.3 mj E pulse < 50 µj Conversion to UV picture from S. Schreiber

Pulse Train Oscillator (PTO) The electro optic modulator (EOM) composed of 1.3 GHz amplifier and cavity potential candidate creating laser pulse arrival time variations (slope) well-aimed phase variations of 1.3 GHz master oscillator (MO) signal can correct the arrival time Modulators (AOM EOM AOM) 108 MHz 1.3 GHz 13.5 MHz Piezo tuning of cavity length f round trip = 27 MHz Stabilized by quartz tubes picture from S. Schreiber Fiber-coupled pump diodes picture from S. Schreiber

Emission phase variation by EOM MO signal manipulation we assume no influence of laser amplifier on slope we measured the step response of the laser on 1.3 GHz phase changes and adapted phase slope onto 1.3GHz of laser: see adjacent picture (not knowing better!) What s about the gun rf?

FLASH rf gun filling time: typical 55 μs flat top time: up to 800 μs pulse repetition: up to 5 Hz high RF field: 40 MV/m Perfect rf field symmetry, no sparks and easier cooling by no rf probe no mechanical tuner via the temperature the frequency is controlled (0.1 deg Celsius corresponds to 2.1 deg in RF phase)

Rf control by SimCon 3.1 and sophisticated algorithms Implications of missing probe: calculation of probe form forward and reflected rf calibration and linearization is an issue Algorithms: P(I) control with recursive 20 khz low-pass (IIR) for stability at high gain (>5) Adaptive feed forward (AFF) from rf pulse to rf pulse set point table 50 MHz 1MHz DAC AFF table t 0 FIR gate gun klystron pre-amp proportional gain integral gain 1 2 AFF gain track back IIR low-pass 1MHz ADC virtual rf probe 3 50 MHz 4 reset

Calibration of virtual probe signal & phase determination non zero (loop) phase leads to an unwanted mixture of I and Q applying a step function (I only) and recording the response (example for f = 200 Hz) excitation & response in time domain response plotted in IQ plane

Spiral like cavity response the initial angle gives the loop phase final IQ values for different tuning describe a circle Alexander Brandts loop phase calibration method is based on circle fitting cavity response for loop phase zero cavity response for (loop) phase 30º Plots for the sc 1.3 GHz TESLA cavities, the RF gun behaves similar!

Virtual probe signal calibration (method established at FLASH by A. Brandt) circle fitting after frequency variation DOOCS panel for calibration parameters Plots taken at PITZ the plots and panels look similar at FLASH!

Nonlinearity compensation of virtual probe signal Problem: IQ detectors are not perfect rf phase changes lead to amplitude changes amplitude changes lead to heat load changes within gun and as a consequence within the circulator this causes reflected power interlocks at the klystron time consuming restart for getting gun temperature equilibrium RF phase scan amplitude response before and after the linearization : Countermeasure: linearization of virtual probe signal by an algorithm

No longer heat load changes caused by rf phase changes RF gun temperature changes while scanning the rf phase: before the compensation after some iterations to obtain the compensation parameters

Action of control loops - the case without control gun Beam based emission phase measurement: set point table 50 MHz 1MHz DAC AFF table reset klystron pre-amp proportional gain integral gain t 0 FIR gate 1 2 AFF gain track back IIR low-pass 1MHz ADC virtual rf probe 3 50 MHz 4 gun heats up within rf pulse gun resonance frequency changes the emission phase changes by 8.5

The case with P control only gun Beam based emission phase measurement: set point table 50 MHz 1MHz DAC klystron pre-amp proportional gain integral gain AFF table reset t 0 FIR gate AFF gain ADC IIR low-pass virtual rf probe 1 4 2 track back 1MHz 3 50 MHz proportional control with gain 4 emission phase change suppressed the emission phase changes by 1.7

Case with P control and adaptive feed forward (AFF) gun Beam based emission phase measurement: set point table 50 MHz 1MHz DAC AFF table reset klystron pre-amp proportional gain integral gain t 0 FIR gate 1 2 AFF gain track back IIR low-pass 1MHz ADC virtual rf probe 3 50 MHz AFF corrects systematic errors AFF gain of 0.4 the emission phase changes by 0.14

Long term stability (2) (1) Observed emission phase stability: (3) (1) RF drive only: peak-to-peak 1.3 (2) P control only: peak-to-peak 0.4 (3) P and AFF control: peak-to-peak 0.4

The gun rf phase slope feature Potential sources of emission phase slopes: uncertainties in probe calibration gun laser pulse arrival time changes drifts due to wave guide heating (distance between directional coupler and gun) and so on Countermeasures: slope at gun laser arrival time changing 1.3 GHz MO EOM phase phase slope at gun rf:

Which slope to use at the gun? According to measurements at BC2, applying a combination of both slopes (gun laser arrival time and gun rf phase) results in the most stable beam! Let s go to ACC1 and beam stability measurements at BC2

Accelerating the bunches up to 130 MeV 4MeV 130 MeV 380 MeV BC3 BC2 ACC1 ACC2/3 700 MeV bypass 13 nm photon beam-line rf gun laser rf gun accelerating module toroid monitor camera OTR screen 1.3 GHz klystron bending magnet bunch compressors beam dump beam stability measurement via synchrotron light monitor in BC2 beam energy in BC2 dominated by ACC1 energy gain (only 3% from gun) beam energy stability measured in BC2 yields upper limit for ACC1 rf stability

To make the material less monotonous: picture of ACC1 and BC2

Beam energy determined by synchrotron light spot at BC2 Fitting methods: Fit 1: slope at head gives information on rf amplitude Fit 2: Gaussian fit to profile information on rf amplitude and rf phase Resolution: E/E = 10-4

ACC1 rf control: P control with beam based beam loading compensation Problem: Scheme implemented for ACC1 at FLASH: cavity with fast proportional (P) RF control corrects after 20 μs first 20 bunches suffer R/Q, beam klystron correction within 2 bunches required Countermeasures: prediction of beam current and derivation of compensation feed forward table DAC proportional gain ADC set point table measurement of beam current in real time and applying appropriate compensation

Ideal gain for proportional rf control at ACC1 relative energy stability 1E-3 1E-4 0 10 20 30 40 Gain limitations: noise at pick up signal: G = 15 theory w/o paying attention to the 8/9 π mode: G = 40 theory with paying attention to the 8/9 π mode: G > 100 gain of proportional control Plus points: Gain resulting in most stable beam: error suppression for small gain values noise amplification for large gain values ideal gain between both cases best single bunch stability: E/E = 2x10-4 XFEL requirement: E/E = 10-4 we controlled only 7 cavities (one pick up makes trouble) XFEL injector has four instead of only one module

If we accelerate multiple instead of one bunch all bunches shall show similar relative energy stability E/E ok with the proportional control all bunches shall show similar absolute energies E beam loading compensation required

Charge proportional signal from toroid monitor taking several samples (5) per bunch from analogue monitor signal sum of samples offset correction using samples at times without beam

Calibration of compensation signal with phase scan Method: rf feedback off identical signal without beam and with beam and compensation for correct amplitude I and Q cross zero at same phase value (-10 ) Calibration problem: rf power from klystron output fluctuates from rf pulse to pulse theoretical residual beam loading in arb. units measured residual beam loading in arb. units 3 2 1 0-1 -2-3 15 10 5 0-5 -10 compensation 20% to high compensation 20% to low -15-40 -30-20 -10 0 10 20 30 phase of compensation factor in degrees

Actual status of the beam loading compensation Operation with P control only (G = 15) Beam loading compensation switched on Next steps: Improvement of the calibration and further qualification of method by measuring energy stability of beam in BC2.

Accelerating the bunches up to 380 MeV 4 MeV 130 MeV 380 MeV BC3 BC2 ACC1 ACC2/3 700 MeV bypass 13 nm photon beam-line rf gun laser rf gun accelerating module toroid monitor camera OTR screen 1.3 GHz klystron bending magnet bunch compressors beam dump beam stability measurement via OTR screen in BC3 beam energy in BC3 is a results from the ACC1 and ACC2/3 rf stability nevertheless, the beam energy stability measured in BC3 yields an upper limit for the ACC2/3 rf stability

Beam energy determined by OTR screen in BC3 The beam position measured with an OTR screen in a dispersive section Gaussian fit to profile for beam position: yields beam energy information. Resolution: E/E = 3x10-5

ACC2/3 rf control: proportional control for 16 cavities Key features for this control: Control scheme used at ACC2/3: connection of two SimCon 3.1 boards as master and slave to control the vector sum of 13 cavities (3 cavities have been excluded form the control) klystron linearization was switched on feed forward table DAC klystron proportional gain 16x ADC set point table no beam loading compensation applied as only two bunches has been accelerated within this studies

Beam energy stability observed at BC3 P control with gain = 0 P control with gain = 10 P control with gain = 40 E/E = 1.6x10-4 E/E = 1.6x10-4 E/E = 2x10-4 No beam energy stability improvement due to rf control? sensor noise (down converters) the klystron it selves seems to be well stabilized due to the gain = 0 result!

Summary and outlook RF gun: emission phase can be manipulated via the gun laser and the rf control which one to manipulate for optimal FLASH performance? systematic way for virtual probe calibration nonlinearities compensated: no longer problems with reflected power interlocks rf control with P control and adaptive feed forward well established beam based emission phase measurement established measured with beam: reasonable and sufficient performance of gun rf control First accelerating module ACC1: energy and rf amplitude stability measurement established at BC2 ideal P control gain determined single bunch energy stability E/E = 2x10-4 (XFEL specs E/E = 10-4 ) beam based beam loading compensation works calibration of beam based beam loading compensation remains to be improved

Summary and outlook (continued) Second and third accelerating modules ACC2/3: beam stability measurement available at BC3 using an OTR screen two SimCon 3.1 are able to control vector sum of 16 cavities no improvement by proportional rf control observed rf sensor noise (from down converters?) remains to be reduced drastically rf drive from klystron at ACC2/3 well stabilized: compare E/E = 1.6x10-4 @ ACC2/3 to E/E = 1.7x10-3 @ ACC1 for gain = 0 multi bunch beam stability remains to be measured Within the accelerator studies in winter 2006/2007, we carried out quite some amount of work!