A   B   C   D   E   F   G   H   I   J   K   L   M   N   O   P   Q   R   S   T   U   V   W   X   Y   Z  

Schlarb, H.

Paper Title Page
WEPC05 Technical Design of the XUV Seeding Experiment at FLASH 503
 
  • V. Miltchev, A. Azima, J. Bödewadt, F. Curbis, H. Delsim-Hashemi, M. Drescher, Th. Maltezopoulos, M. Mittenzwey, J. Roßbach, R. Tarkeshian, M. Wieland
    Uni HH, Hamburg
  • S. Düsterer, J. Feldhaus, T. Laarmann, H. Schlarb
    DESY, Hamburg
  • R. Ischebeck
    PSI, Villigen
  • S. Khan
    DELTA, Dortmund
  • A. Meseck
    Helmholtz-Zentrum Berlin für Materialien und Energie GmbH, Berlin
 
 

The Free-electron-laser at Hamburg (FLASH) operates in the Self-Amplified Spontaneous Emission (SASE) mode, delivering to users photons in the XUV wavelength range. The FEL seeding schemes promise to improve the properties of the generated radiation in terms of stability in intensity and time. Such an experiment using higher harmonics of an optical laser as a seed is currently under construction at FLASH. The installation of the XUV seeding experiment (sFLASH) is going to take place in fall 2009. This includes mounting of new variable-gap undulators upstream of the existing SASE-undulators, building the XUV-seed source as well as installation of additional photon diagnostics and electron beam instrumentation. In this contribution the layout of sFLASH will be discussed together with the technical design of its major components.

 
WEPC52 Using an Ytterbium Fiber Laser Based Electro-Optic Experiment For Electron Bunch Diagnostic at FLASH 627
 
  • L.-G. Wißmann, S. Schulz
    Uni HH, Hamburg
  • V. R. Arsov
    PSI, Villigen
  • M.K. Bock, M. Felber, P. Gessler, K.E. Hacker, F. Löhl, F. Ludwig, H. Schlarb, B. Schmidt, S. Wesch, A. Winter, J. Zemella
    DESY, Hamburg
 
 

FLASH (The Free-Electron Laser At Hamburg) is a High-Gain SASE-FEL providing ultrashort pulses with a central wavelength of 6 to 40 nm. Measuring and controling the longitudinal shape of the electron bunches can dramatically improve the stability of the lasing process. Non-destructive electro-optical bunch profile diagnostics have proved to work with resolutions down to 100 fs. The electro-optical (EO) setup at FLASH relies on a standard Ti:sapphire laser delivering 80 fs pulses with 4 nJ pulse energy. For practical and physical reasons (i.e., space, costs, maintenance, performance) a new, ytterbium fiber laser system has been developed. This laser system supports pulse energies of 4.5 nJ and a bandwidth of 100 nm at a center wavelength of 1030 nm. Active repetition rate control allows to lock the laser to the RF based synchronisation system. A better EO signal-to-noise ratio is expected due to the improved group velocity matching in the EO crystal. First results from the prototype Yb laser system and comparison with the Ti:Sa based data will be presented. Furthermore, a structurally engineered version, promising enhanced stability and reliability will be introduced.

 
WEPC66 Beam Arrival Time Monitors Used in a Time-Of-Flight Beam Energy Measurement 659
 
  • M.K. Bock, V. R. Arsov, M. Felber, P. Gessler, K.E. Hacker, F. Löhl, F. Ludwig, H. Schlarb, B. Schmidt, A. Winter, L.-G. Wißmann
    DESY, Hamburg
  • S. Schulz, J. Zemella
    Uni HH, Hamburg
 
 

At FLASH an optical synchronisation system with femtosecond stability is now being installed and commissioned. The pulses from an erbium-doped fibre laser being distributed in length-stabilised fibres to various endstations are used to detect the electron bunch arrival time using electro-optical modulators. To determine variations of the arrival time caused by phase changes of the RF gun or by timing changes of the photo-injector laser a beam arrival time monitor has been installed after the first acceleration section, prior to the bunch compressor BC2. A second bunch arrival time monitor installed after the bunch compressor allows for measuring the beam energy with high precision through a time-of-flight detection. Both monitors provide futher insight into the accelerator subsystem stability and opens up the opportunity for a robust fast feedback stabilisation.

 
WEPC69 Design and Drift Performance of the FLASH Master Laser Oscillator RF-Lock 663
 
  • K.E. Hacker, V. R. Arsov, M.K. Bock, M. Felber, P. Gessler, F. Löhl, F. Ludwig, H. Schlarb, B. Schmidt, S. Schulz, A. Winter, L.-G. Wißmann, J. Zemella
    DESY, Hamburg
 
 

The master laser oscillator (MLO) at FLASH is locked to the master RF oscillator (MO) by mixing a 1.3 GHz signal from an MLO-based photodetector and a 1.3 GHz signal from the MO. The baseband output of the mixer is sent to an ADC-DSP-DAC regulation system that feeds back on a piezo controlled mirror position in the laser. The rms jitter and long term drift stability of the RF-lock circuit alone can be less than 5 fs in the temperature controlled chassis, but it can jump 10 to 15 fs when the temperature regulation of the room is disturbed by people working inside. Out-of-loop and in-loop measurements were also conducted under various environmental conditions.

 
WEPC70 Demonstration of a BPM with 5 Micron Resolution over a 10cm Range 667
 
  • K.E. Hacker, V. R. Arsov, M.K. Bock, M. Felber, P. Gessler, F. Löhl, F. Ludwig, H. Schlarb, B. Schmidt, S. Schulz, A. Winter, L.-G. Wißmann, J. Zemella
    DESY, Hamburg
 
 

A unique, perpendicularly-mounted stripline BPM pickup is installed in the dispersive sections of the FLASH bunch compressors. For 4-5 um resolution, it requires a front-end that can measure the difference between the phases of the beam transient pulses with a resolution that is better than 10-15 fs. Two front-ends have been tested with the pickup: a 10.4 GHz down-mixing scheme and an electro-optical modulator (EOM) based scheme that uses the optical synchronization system. The EOM scheme typically produces 6 to 12 fs resolution. It is, however, expensive, complex, and dependent on an optical infrastructure that is still in a development phase. It was not anticipated that an RF-mixing scheme could deliver the required, sub-15 fs resolution and drift stability, but with a temperature stabilized chassis in a climatized room and sufficiently high frequencies, an RF mixing scheme can deliver resolution that is comparable to that of the EOM scheme for this particular application, the measurement of the relative arrival-times of two ~ps pulses. A direct comparison of beam arrival time measurements with 10.4 GHz down-mixing and EOM sampling is also presented.

 
WEPC72 Progress Towards a Permanent Optical Synchronization Infrastructure at FLASH 671
 
  • S. Schulz, L.-G. Wißmann
    Uni HH, Hamburg
  • V. R. Arsov, M.K. Bock, M. Felber, P. Gessler, K.E. Hacker, F. Löhl, F. Ludwig, H. Schlarb, B. Schmidt, A. Winter, J. Zemella
    DESY, Hamburg
 
 

Free-electron lasers like FLASH and the planned European XFEL generate X-ray light pulses with durations in the order of a few ten femtoseconds. For these next-generation light sources, an optical synchronization system has been proposed to enable time-resolved measurements with sub-10 fs resolution and the laser-driven seeded operation mode of the FEL. The system is based on the timing-stabilized distribution of an optical pulse train, from which RF signals can be generated or to which other laser systems can be synchronized. Furthermore, it facilitates several special diagnostic measurements on the sub-10 fs time-scale.

The optical synchronization system at FLASH has recently progressed from a bread-board/test-bench implementation to a more permanent engineered infrastructure. We report on the master laser oscillator, the lock to the master RF oscillator, the free-space distribution unit, four installed fiber links, three bunch arrival-time monitors, one optical cross-correlator and the controls development. We also identified a couple of design issues during the commissioning of the devices.

 
THOB02 Results from the Optical Replica Synthesizer at FLASH 739
 
  • P.M. Salén, M. Hamberg, M. Larsson, P. van der Meulen
    FYSIKUM, AlbaNova, Stockholm University, Stockholm
  • G. Angelova Hamberg, V.G. Ziemann
    Uppsala University, Uppsala
  • J. Bödewadt, A. Winter
    Uni HH, Hamburg
  • S. Khan
    DELTA, Dortmund
  • F. Löhl, E. Saldin, H. Schlarb, E. Schneidmiller, M.V. Yurkov
    DESY, Hamburg
  • A. Meseck
    Helmholtz-Zentrum Berlin für Materialien und Energie GmbH, Berlin
 
 

We present results from the new electron bunch diagnostic tool, Optical Replica Synthesizer [1] (ORS), installed at FLASH. The ORS produces an optical replica of the electron bunch profile, which is analyzed with a Grenouille, a device based on the Frequency Resolved Optical Gating (FROG) technique. This optical replica is generated by inducing a microbunching in the electron bunch and letting it pass through an undulator, called a radiator. The radiator emits coherently at the wavelength of microbunching, 772 nm. In order to create the microbunching a laser pulse is spatially and temporally overlapped with the electron bunch in another undulator, placed before the radiator. This introduces an electron energy modulation which is transformed into a density modulation in a chicane before the microbunched electron bunch is sent into the radiator. We observed an optical replica pulse of approximately 5 microJ corresponding to an electron bunch-spike of about 150 fs FWHM when the accelerators were set at optimal FEL conditions. We also showed that the ORS can run parasitically while maintaining SASE by steering the electron beam around the outcoupling mirror for the radiation.


[1] E. Saldin, E. Schneidmiller, M. Yurkov, “A simple method for the determination of the structure of ultrashort relativistic electron bunches,” Nucl. Inst. and Methods A 539 (2005) 499.

 

slides icon

Slides

 
FROA05 RF-based Detector for Measuring Fiber Length Changes with Sub-5 Femtosecond Long-Term Stability 780
 
  • J. Zemella, V. R. Arsov, M.K. Bock, M. Felber, P. Gessler, K.E. Hacker, F. Löhl, F. Ludwig, H. Schlarb, B. Schmidt, A. Winter
    DESY, Hamburg
  • S. Schulz, L.-G. Wißmann
    Uni HH, Hamburg
 
 

At the Free-Electron Laser in Hamburg (FLASH), an optical synchronization system is being installed with a projected point-to-point stability of 10 fs. The system is based on the distribution of reference laser pulses over actively stabilized fiber links using optical cross-correlators. As an alternative to the complex cross-correlation scheme, which can achieve sub fs long-term stability and works well over several 100 m long fiber links, an RF-based technique which is much less complex and expensive could be used. It is based on the power detection of high harmonic frequencies in a balanced arrangement to reduce amplitude noise. For a 20 m long fiber link, it was demonstrated that a sub-5 fs rms long-term stability over 30 hours can be achieved. The system and the most recent measurements are presented here.

 

slides icon

Slides

 
THOB05 Photon DIiagnostics for the Seeding Experiment at FLASH 754
 
  • F. Curbis, A. Azima, J. Bödewadt, H. Delsim-Hashemi, M. Drescher, Th. Maltezopoulos, V. Miltchev, M. Mittenzwey, J. Roßbach, R. Tarkeshian, M. Wieland
    Uni HH, Hamburg
  • S. Düsterer, J. Feldhaus, T. Laarmann, H. Schlarb
    DESY, Hamburg
  • R. Ischebeck
    PSI, Villigen
  • S. Khan
    DELTA, Dortmund
  • A. Meseck
    Helmholtz-Zentrum Berlin für Materialien und Energie GmbH, Berlin
 
 

Starting from next year, the technical feasibility of a direct seeding scheme at 30 and 13nm will be studied at the free-electron laser FLASH at DESY. During a major shutdown in order to upgrade the SASE-FEL facility, it is planned to install a HHG source, a new chain of 10 m variable gap undulators and a dedicated commissioning beamline for photon diagnostics and pilot time-resolved pump-probe experiments. Besides demonstrating successful seeding at short wavelength, the project aims for time resolution in the 10 fs range to study ultrafast processes by combining the naturally synchronized FEL and seed laser pulses. After the extraction of the radiation in a magnetic chicane, a short branch will accommodate intensity and beam monitors and a spectrometer. The intensity monitor detects scattered photons from a gold mesh on a shot-to-shot basis using micro-channel plates and XUV diodes. It is designed to detect photons several orders of magnitude apart in flux, i.e. spanning the wide range from the spontaneous emission up to the seeded FEL radiation at gigawatt power level. Simulations of this device are presented as well as test and calibration measurements carried out at FLASH.

 

slides icon

Slides