Notes from the Workshop on: Realizing the Potential of Seeded FELs in the Soft X-Ray Regime. Kirsten Hacker Nov
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1 Notes from the Workshop on: Realizing the Potential of Seeded FELs in the Soft X-Ray Regime Kirsten Hacker Nov
2 Highlights -User expectations -New theory and simulations -New experiment designs -Recent experimental results
3 Users want CONTROL Slide from Schoenlein
4 Users want NGLS (FLASH clone with 2.4 GeV, CW upgrade)
5 Users want NGLS
6 NGLS wants to be like FLASH John Byrd (BNL): fs-synchronization THz diagnostics Alan Fry (SLAC): seeding scheme
7 Destination: seeded 1 nm Self-seeding Advantage : No seed laser problems Disadvantage: Less control External seeding Advantage: sensitivity to seed laser properties Disadvantage: sensitivity to seed laser properties
8 Destination: seeded 1 nm? EEHG or HHG
9 Destination: seeded 1 nm EEHG or HHG
10 Best of both worlds Two-color Experiments, anyone? EEHG or HHG 1 st radiator 2 nd radiator HGHG fresh bunch chicane
11 Self-seeding: sounds easier SASE radiator (linear) monochromator seeded radiator (steady-state)
12 Theory and simulations Reversible heater Intra-bunch scattering Seed laser phase errors Seed laser wavefront errors
13 Huang: reversible heater
14 Huang: reversible heater
15 Comment: Since a low slice energy spread is so important for seeding, why are we moving the seeding experiments into FLASH II and FLASH III where the energy spread is worse than in FLASH I?
16 Stupakov: IBS Concern: coulomb collisions and EEHG Theory: derive diffusion coefficient in beam frame and then transform to lab frame Conclusion: becomes a problem around 200 th harmonic of 200 nm (~1nm). Distance between exit of last chicane and entrance to radiator must be short for seeding at 1 nm
17 Comment: I think other effects will cause problems for EEHG loooong before IBS
18 Ratner et al.: seed phase error Concern: seed phase error harmonic number Theory: short laser pulse, longer e-beam Conclusion: hard limit at ~1 nm in best-case scenario Shortens usable portion of seed
19 Comments: It is nice to see an expression for how the usable portion of a chirped seed is shortened at higher harmonics, BUT If one has an excess of seed power, one may not want to fully compress the seed pulse. A chirped pulse leaves more flexibility to find the correct frequency for the radiator (eases tolerances) Note that one loses seed bandwidth everywhere. There are methods to measure and correct these errors. The scarier problem comes from uncorrelated phase errors!
20 Hacker et al.: seed wavefront Concern: wavefront harmonic number Theory: analytic and numerical predictions of reduction of EEHG bunching factor Conclusion: difficulties arise below 40 nm Analytic expression for wavefront tolerance Optics errors -> adaptive mirrors and/or spatial filter B-integral considerations Compressor mis-alignments -> wave-front rotation & pulse-front tilt
21 Hacker et al.: seed wavefront
22 Numerical simulations: 1 nm EEHG schemes presented by Xiang (SLAC), Penn (BNL), and Reiche (PSI) did not investigate the wavefront error tolerance, although Xiang and Penn did recently attempt to understand the tolerance of their schemes to phase error FLASH nm has studied the tolerances of these errors since early 2011
23 Geloni: self-seeding
24 Geloni: self-seeding
25 Geloni: self-seeding
26 Geloni: self-seeding
27 Experimental results HHG: Lambert (LOA) & Giannessi (SPARC) EEHG: Xiang (SLAC-NLCTA) HGHG: Allaria (ELETTRA)
28 Lambert Giannessi
29 Lambert, LOA: HHG
30 Giannessi:
31 Giannessi:
32 Giannessi:
33 Giannessi:
34 Giannessi:
35 Werin,
36 Xiang
37 Xiang:
38 Xiang:
39 Allaria
40 Allaria: ELETTRA HGHG
41 Allaria: Transverse Coherence
42 Allaria: Phase Shifters
43 Allaria: Transverse Coherence
44 Allaria: Theory & Measurements
45 Allaria: HGHG->stability
46 Conclusions Seeding at ~1 nm will be attempted in 2 ways Self-seeding HGHG cascade with saturation in first stage using either EEHG or HHG FLASH is set to lead in EEHG Trieste leads in HGHG (SLAC has a seriously huge laser team)
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