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The ORS at FLASH and sFLASH Peter van der Meulen Stockholm University Div. Molecular Physics FLS2010, March 1-5, 2010, 48 th ICFA Advanced Beam Dynamics Workshop on Future Light Sources ew diagnostic tool for characterizing electron bunc
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The ORS at FLASH and sFLASH

Jan 12, 2016

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The ORS at FLASH and sFLASH. a new diagnostic tool for characterizing electron bunches. Peter van der Meulen Stockholm University Div. Molecular Physics. FLS2010, March 1-5, 2010, 48 th ICFA Advanced Beam Dynamics Workshop on Future Light Sources. - PowerPoint PPT Presentation
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Page 1: The ORS at FLASH and sFLASH

The ORS at FLASH and sFLASH

Peter van der Meulen

Stockholm UniversityDiv. Molecular Physics

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

a new diagnostic tool for characterizing electron bunches

Page 2: The ORS at FLASH and sFLASH

ORS: Optical Replica Synthesizer

FLASH, XFEL, JFEL, LCLS: SASE

electron bunch properties: longitudinal density profileslice emittanceslice energy spread

SASE is very sensitive to the properties of the electron bunch

need to control and measure these properties!

electron bunch: moving at v ≈ cca. 20 m longca. 100 m wide

hard to measure directly measure an optical copy instead

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 3: The ORS at FLASH and sFLASH

ORS: Optical Replica Synthesizer

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 4: The ORS at FLASH and sFLASH

ORS: Optical Replica Synthesizer

Erbium fiber oscillator:• 1550 nm• ca. 54 MHz• amplified• frequency doubled, 1 mm PPLN• 1 – 5 mW

Clark-MXR CPA2001• Ti:Sapph CPA system • 5 Hz (1 kHz)• ca. 700 J/pulse• 0.2 – 3.0 ps

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 5: The ORS at FLASH and sFLASH

ORS: temporal overlap

Er:fiberoscillator

stretcher compressorTi:Sapphamplifier

to tunnel

ca.54 MHzpulse train

FLASH 5 Hz trigger

ca.19 ns

Fourier Transform 24th harmonic

ca. 1.3 GHz

diff. freq.mixing

FLASH RF1.3 GHz

vectormodulator

Matlab progam

piezo +delay

…+ cos[(.t + ] = 0

delay

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 6: The ORS at FLASH and sFLASH

ORS: Magnet structures

Undulators:• electromagnets• 1450 mm• 40 mm gap, 0.5 T max.• 14 poles (1/4,-3/4,1,-1…)• 4 power supplies• modulator vertical• radiator horizontal

Chicanes:• 4 dipole magnets• 1300 mm

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 7: The ORS at FLASH and sFLASH

ORS: spatial overlap

calibration and OTR screens on7Match and 3SUND1

Joern Boedewadt

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 8: The ORS at FLASH and sFLASH

ORS: temporal overlap

0 1 2 3 4 5 6

0

0.2

0.4

0.6

0.8

1

Time (ps)

Coh

eren

t O

TR

int

ensi

ty (

arb.

uni

ts)

CoherentOTR

@ 385 nm

PRSTAB 11, 070702, 2008FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 9: The ORS at FLASH and sFLASH

GRENOUILLE*

based on SH FROG technique (autocorrelator + spectrometer)

single shot measurement

2D phase retrieval algorithm => fully characterized pulse

Electric field profile electron bunch profile (I4)

femtosecond optical pulse characterization

* Swamp Optics

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 10: The ORS at FLASH and sFLASH

ORS: FROG trace

seed laser pulse: ca. 400 fs FWHMFROG trace: ca. 150 fs FWHM FLASH’s electron bunch spike?

Compatible with SASE!!!FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 11: The ORS at FLASH and sFLASH

ORS: FROG trace

• ca. 1-5 J/pulse

• ca. 150 fs FWHM

• no direct comparison with TDC (LOLA) FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

-800 -600 -400 -200 0 200 400 600 8000

0.2

0.4

0.6

0.8

1

E-f

ield

(ar

b. u

nits

)

Time (fs)-800 -600 -400 -200 0 200 400 600 800

-5

-3

-1

1

3

5

Pha

se (

rad)

Page 12: The ORS at FLASH and sFLASH

ORS at FLASH

Some remaining issues:

• cross check with TDC (LOLA) and/or EO measurement

• laser power: 1 mJ/ pulse 30 mJ/pulse

• better digital data collection: 8 bit 12/16 bit

• what happens under further bunch compression? CSR?

• what is the future of the ORS?

The ORS seems to work, but…

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 13: The ORS at FLASH and sFLASH

ORS: FROG trace

A FROG trace obtained upon further compressing the electron bunch:

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 14: The ORS at FLASH and sFLASH

ORS at sFLASH

temporary shutdown September 2009

rebuild ORS in new position

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 15: The ORS at FLASH and sFLASH

ORS at FLASH

Other applications of the ORS:

• phase of optical replica pulse energy chirp of electron bunch

• slice energy spread

• slice emittance

• 3D spatial electron bunch characterization via coherent OTR

• ‘echo’ test experiments (G. Stupakov, SLAC-PUB-13445, Oct. 2008)

• ORFIR

• general study laser – electron interactions

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 16: The ORS at FLASH and sFLASH

conclusions

• first ORS results obtained in 2009!!!

• the ORS seems a very useful addition to (s)FLASH, as a diagnostic device. Some issues deserve further study.

• more (parasitic) beam time is required to make the ORS a standard and routine diagnostic technique.

• ‘alternative’ applications of the ORS appear very promising.

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 17: The ORS at FLASH and sFLASH

DESY, 27 January 2009

Collaborators

Stockholm University: Peter Salen Mathias Hamberg Mats Larsson

Uppsala University: Volker Ziemann Gergana Angelova-Hamberg

DESY: Holger Schlarb Florian Löhl

Hamburg University: Joern Boedewadt Axel Winter Shaukat Khan

BESSY: Atoosa Meseck

DESY: E. Saldin, E. Schneidmiller & M. Yurkov

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 18: The ORS at FLASH and sFLASH

THANK YOU!

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 19: The ORS at FLASH and sFLASH

ORS: temporal overlap

Holger SchlarbFlorian Löhl

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 20: The ORS at FLASH and sFLASH

ORS @ sFLASH

What to do:

• move undulators, dipoles and optical stations (+ cables)

• re-build OS1 chicane in vertical plane; re-design OS2 chicane

• change to HHG laser; 10% beamsplitter, ca. 4 mJ/pulse + compression

• improve laser beam diagnostics

• insert new OTR screens: diffuse scattering screen doped YAG screen for e-beam and laser? better optical quality: surface and flatness

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 21: The ORS at FLASH and sFLASH

DESY, 27 January 2009

BOA pulse compressorBother-free Optimized Arrangement

Swamp Optics

fused silicatransmission

grating,ca. 1000 l/mm

• no angular dispersion• no pulse front tilt• no spatial chirp

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 22: The ORS at FLASH and sFLASH

• imaging using coherent OTR/ODR: longitudinal bunch profile high k – small wavelength compared to THz measurements high intensity

I(r) N d2r’ dz (r’,z) Eone-electr(r-r’) 2

+

N2 d2r’ dz exp(-ikz) (r’,z) Eone-electr(r-r’) 2

Icoh(r) N2 d2 (,k) ( exp(ir))/( 2 + 2) 2 = k/

if (,k) = f() . g(k) X

but….

ORS contributions to sFLASH

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources

Page 23: The ORS at FLASH and sFLASH

The ORS as a routine diagnostic?PR

STA

B 1

1, 0

7070

2, 2

008

what about the possibility to do an image reconstructionusing algorithms similar to those applied in single-particle

X-ray diffraction?

multiple k’s and modulation using chirped seed pulses

FLS2010, March 1-5, 2010, 48th ICFA Advanced Beam Dynamics Workshop on Future Light Sources