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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC Simulations of LSC in the LCLS Injector Cécile Limborg-Déprey, P. Emma, Z. Huang, Juhao Wu March 1st, 2003 LSC in drifts Simulations for Injector Case of 100 m modulation Other wavelengths [ 50,150,200, 300] m Conclusion LSC in drifts Simulations for Injector Case of 100 m modulation Other wavelengths [ 50,150,200, 300] m Conclusion
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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC Simulations of LSC in drifts Simulations description 40k/200k particles Distribution generated using the Halton sequence of numbers Longitudinal distribution 2.65 m of drift With 3 cases studied 6MeV, 1nC 6 MeV, 2nC 12 MeV, 1nC Simulations description 40k/200k particles Distribution generated using the Halton sequence of numbers Longitudinal distribution 2.65 m of drift With 3 cases studied 6MeV, 1nC 6 MeV, 2nC 12 MeV, 1nC +/- 5%
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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC
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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC
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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC Summary 100 m Comparison with theory Transverse beam size evolution along beamline taken into account (Radial variation of green’s function for 2D ) Evolution of peak current NOT taken into account yet Absence of dip in 6MeV curve : “Coasting beam “ against “bunched beam” with edge effects Intrinsic energy spread
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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC Nominal Tuning 10 ps pulse (rise/fall time 1ps ) 1 nC Nominal Tuning 10 ps pulse (rise/fall time 1ps ) 1 nC Laser + Gun Linac0-1 Linac0-2 6MeV0MeV60MeV150MeV ASTRA Simulations of LSC along Injector Beamline
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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC ASTRA Simulations for modulation of 100 m Modulation Wavelength = 100 m, with 8% amplitude peak-to-peak “Noise of 8% amplitude around flat top is likely to be present “ P.Bolton FWHM = 3mm Longitudinal bining = 200 points (~ more than 6 bins per period) 1 Million particles Modulation Wavelength = 100 m, with 8% amplitude peak-to-peak “Noise of 8% amplitude around flat top is likely to be present “ P.Bolton FWHM = 3mm Longitudinal bining = 200 points (~ more than 6 bins per period) 1 Million particles Current density with modulation = 100 m Region of interest Fourier Analysis Position (mm) Cycles per mm
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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC Longitudinal Phase Space After removal of correlation up to order 5 Energy Current Fourier transform Fit up to 3 rd order Substract and Fit Amplitude + rms w.r.t reference level z = 0.15 m E = 6MeV Gun Exit E = 0 → 0.35 keV Current modulation = 5.65% → 3%
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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC Energy Current Fourier transform z = 1.4 m E = 6MeV Entrance L01 E = 0.35 keV → 1 keV Current modulation = 3% → 1.5%
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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC Exit L01 Energy Current Fourier transform z = 4.4 m E = 60MeV Exit L01 E = 1 keV → 3 keV Current modulation = 1.5 % → 1.5%
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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC Exit L02 Energy Current Fourier transform z = 8.4 m E = 150MeV Exit L02 E = 3 keV → 3.9 keV Current modulation = 1.5 % → 1.6%
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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC Summary 100 m
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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC Summary 50,100,150,300 m Attenuation by factor More than 5 for <100 m ~ 5 for >100 m
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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC At end LCLS injector beamline: Current density modulation strongly attenuated residual energy oscillation has amplitude between 2 keV and 4 keV for wavelengths [50 m, 500 m] Impedance defined by At end LCLS injector beamline: Current density modulation strongly attenuated residual energy oscillation has amplitude between 2 keV and 4 keV for wavelengths [50 m, 500 m] Impedance defined by Same results with PARMELA
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Injector Requirements Limborg@slac.stanford.edu Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile Limborg-Déprey, SLAC Conclusion Good agreement Simulations / Theory for drift and Acceleration Solutions to handle Numerical Problems Noise Problem ( high number of particles) Shorter wavelengths (new option in ASTRA) Clear “Attenuation” in gun makes situation less critical than first thought But not enough attenuation : for wavelengths >100 m : attenuation line density modulation by factor of~5 for wavelengths <100 m : attenuation line density modulation by factor of more than 5 To reach less than 0.1% at end of beamline requires less than 0.4% rms on laser so +/- 0.56% = far beyond what is achievable by laser Also large energy modulation in all cases (“large” = of the order or more than intrinsic energy spread) Heater is required as microstructure present in all wavelengths cases and in particular those < 100 m Good agreement Simulations / Theory for drift and Acceleration Solutions to handle Numerical Problems Noise Problem ( high number of particles) Shorter wavelengths (new option in ASTRA) Clear “Attenuation” in gun makes situation less critical than first thought But not enough attenuation : for wavelengths >100 m : attenuation line density modulation by factor of~5 for wavelengths <100 m : attenuation line density modulation by factor of more than 5 To reach less than 0.1% at end of beamline requires less than 0.4% rms on laser so +/- 0.56% = far beyond what is achievable by laser Also large energy modulation in all cases (“large” = of the order or more than intrinsic energy spread) Heater is required as microstructure present in all wavelengths cases and in particular those < 100 m
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