Free-Electron Laser Challenges 1997
DOI: 10.1117/12.274372
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Output characteristics of SASE-driven short-wavelength FELs

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Cited by 9 publications
(4 citation statements)
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“…The typical design under consideration for these systems is the SASE FEL to avoid the requirements for an external source or good X-ray mirrors. Here, shot noise [93] in the initial electron bunch provides the initial photons, typically having an equivalent power of 10 to 1000 watts due to the large electron charges involved [94]. However, the short wavelength required demand relatively high electron energies, and most designs involve beam energies of 1 GeV or more.…”
Section: A Sase For Short Wavelengthsmentioning
confidence: 99%
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“…The typical design under consideration for these systems is the SASE FEL to avoid the requirements for an external source or good X-ray mirrors. Here, shot noise [93] in the initial electron bunch provides the initial photons, typically having an equivalent power of 10 to 1000 watts due to the large electron charges involved [94]. However, the short wavelength required demand relatively high electron energies, and most designs involve beam energies of 1 GeV or more.…”
Section: A Sase For Short Wavelengthsmentioning
confidence: 99%
“…Theoretical efforts [93] predict the production of short, intense spikes within the micropulse separated by the effective cooperation length. This is similar to effects seen in oscillators at high gain [103,104].…”
Section: A Sase For Short Wavelengthsmentioning
confidence: 99%
“…Our basic perspective will be to view the pulse parameter space of the SASE XRFEL as a limiting case of the pulse parameters typically found on synchrotron storage rings. To initiate our discussion, we first recall the basic phase space properties predicted for the 1.5 Å SLAC LCLS [20,21]. In practical terms, the pulse is about as long as it is wide and has a temporal fine structure consisting of regions longitudinally on the order of 1 fs in length and transversely fully coherent (viz., with diameters equal to the full pulse diameter).…”
Section: Introductionmentioning
confidence: 99%
“…To initiate our discussion, we first recall the basic phase space properties predicted for the 1.5 Å SLAC LCLS [20,21]. In practical terms, the pulse is about as long as it is wide and has a temporal fine structure consisting of regions longitudinally on the order of 1 fs in length and transversely fully coherent (viz., with diameters equal to the full pulse diameter).…”
Section: Introductionmentioning
confidence: 99%