diagnostics (wbs 1.5) yiping feng
DESCRIPTION
Diagnostics (WBS 1.5) Yiping Feng. Motivations System Specifications System Description WBS Schedule and Costs Summary. Motivations. X-ray Free-Electron Laser (FEL) is fundamentally different from storage-ring based synchrotron sources Linac-based, single-pass, 120 Hz at LCLS - PowerPoint PPT PresentationTRANSCRIPT
Yiping [email protected]
LUSI DOE Review July 23, 2007Diagnostics (WBS 1.5) 1
Diagnostics(WBS 1.5)Yiping Feng
Diagnostics(WBS 1.5)Yiping Feng
MotivationsSystem SpecificationsSystem DescriptionWBSSchedule and CostsSummary
MotivationsSystem SpecificationsSystem DescriptionWBSSchedule and CostsSummary
Yiping [email protected]
LUSI DOE Review July 23, 2007Diagnostics (WBS 1.5) 2
MotivationsMotivations
X-ray Free-Electron Laser (FEL) is fundamentally different from storage-ring based synchrotron sources
Linac-based, single-pass, 120 Hz at LCLSFeedback is limited by low repetition rateEach macro electron bunch is different in timing, length, density, energy (velocity), orbit, etc.
X-ray amplification process based on self-seeding SASE*Lasing starts from a random electron density distributionEach X-ray pulse consists of a random time sequence of spikes of varying degrees of saturation
X-ray FEL exhibits inherent Intensity, spatial, temporal, and spectral fluctuations on pulse by pulse basis
X-ray Free-Electron Laser (FEL) is fundamentally different from storage-ring based synchrotron sources
Linac-based, single-pass, 120 Hz at LCLSFeedback is limited by low repetition rateEach macro electron bunch is different in timing, length, density, energy (velocity), orbit, etc.
X-ray amplification process based on self-seeding SASE*Lasing starts from a random electron density distributionEach X-ray pulse consists of a random time sequence of spikes of varying degrees of saturation
X-ray FEL exhibits inherent Intensity, spatial, temporal, and spectral fluctuations on pulse by pulse basis
*Self Amplification of Spontaneous Emission
Yiping [email protected]
LUSI DOE Review July 23, 2007Diagnostics (WBS 1.5) 3
GoalsGoals
X-ray diagnostics are required to measure these fluctuations since they can’t be eliminated
Integral parts of InstrumentsTiming & intensity measurements for XPP experimentsWave-front characterization for CXI experiments
Measurements made on pulse-by-pulse basisRequiring real-time processing by controls and data system
Commonalities in needs & specsStandardized and used for all applicable instrumentsModularized for greater flexibility of deployment and placement
Critical diagnostics must be performed and data made available on pulse-by-pulse basis
X-ray diagnostics are required to measure these fluctuations since they can’t be eliminated
Integral parts of InstrumentsTiming & intensity measurements for XPP experimentsWave-front characterization for CXI experiments
Measurements made on pulse-by-pulse basisRequiring real-time processing by controls and data system
Commonalities in needs & specsStandardized and used for all applicable instrumentsModularized for greater flexibility of deployment and placement
Critical diagnostics must be performed and data made available on pulse-by-pulse basis
Yiping [email protected]
LUSI DOE Review July 23, 2007Diagnostics (WBS 1.5) 4
Expected Fluctuations of LCLS FEL pulsesExpected Fluctuations of LCLS FEL pulses
Parameter Value Origin*
Pulse intensity fluctuation
~ 30 %Varying # of FEL producing SASE spikes; 100% intensity fluctuation/per-spike; etc.
Position & pointing jitter (x, y, , )
~ 25 % of beam diameter
~ 25 % of beam divergence
Varying trajectory per pulse; Saturation at different locations of -tron curvature
Source point jitter (z) ~ 5 m SASE process reaching saturation at different z-points in undulator
X-ray pulse timing (arrival time) jitter
~ 1 ps FWHMTiming jitter btw injection laser and RF; Varying e-energy per-pulse
X-ray pulse width variation
~ 15 %Varying e-energy leading to varying path (compression) in bunch compressors
Center wavelength variation
~ 0.2 % (comparable to FEL bandwidth)
Varying e-energy leading to varying FEL fundamental wavelength and higher order
*To be discussed in details in breakout session
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LUSI DOE Review July 23, 2007Diagnostics (WBS 1.5) 5
X-ray Diagnostics SuiteX-ray Diagnostics Suite
Fluctuation Type Diagnostic Device
Pulse intensity fluctuationa) Pop-In Intensity Monitorb) In-Situ BPM/Intensity Monitor
Position & pointing jitterc) Pop-In Position/Profile MonitorIn-Situ BPM/Intensity Monitor- Pointing determination from multiple BMP’s
Source point jitter Focal point jitter w/ focusing optics
d) Wave-front Sensor- Back-propagating from radius of curvature measurement
X-ray pulse timing jittere) Electro-Optic Sampling (EOS) Device- Relative timing btw e-bunch & ref. probe laser
X-ray pulse width variation EOS Device- Establishes upper limit
Center wavelength variation LCLS e-energy calibration- X-ray wavelength cross-calibration is needed
Yiping [email protected]
LUSI DOE Review July 23, 2007Diagnostics (WBS 1.5) 6
System SpecificationsSystem Specifications
Diagnostic Item Purposes Specifications*
Pop-inintensity monitor(moderate-resolution)
Coarse beam alignment/monitoring;
Destructive; Retractable;Dynamic range 104;Per-pulse operation at 120 Hz;Relative accuracy < 10-2
Pop-inposition/profile monitor
Coarse beam alignment/monitoring
Destructive; Retractable;At 50 m resolution - 25x25 mm2 field of view;At 10 m resolution - 5x5 mm2 field of view
In-situIntensity monitor/BPM(high-resolution)
Per-pulse normalization of experimental signals;High-resolution beam position monitoring
Transmissive (< 5% loss); Dynamic range 106;Per-pulse operation at 120 Hz;Relative accuracy < 10-3
In-situ Electro-optic sampling (EOS) device
Measure relative timing between electron bunch (thus co-propagating x-ray pulse) and a probe optical laser pulse
Non-intrusive to e-beam;Non-destructive; Per-pulse operation at 120 Hz;20 fs resolution;
In-situWave-front sensor
Characterization of wave-front;Locating focal point of focused beam
Destructive; Per-pulse operation at 120 Hz;0.15 nm < < 0.3 nm
* Must have high damage threshold
Tech
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Pop-In Intensity Monitor (WBS 1.5.3)Pop-In Intensity Monitor (WBS 1.5.3)
Coarse alignment of X-ray opticsmonochromators, mirrors, lens, etc.strategically placed in close proximity to optic
Detection techniquePulse operation not photon countingSensor type
Si Diode (used successfully at SPPS)CVD Diamond
Coarse alignment of X-ray opticsmonochromators, mirrors, lens, etc.strategically placed in close proximity to optic
Detection techniquePulse operation not photon countingSensor type
Si Diode (used successfully at SPPS)CVD Diamond
Destructive; Retractable;Moderate dynamic range 104; Relative accuracy < 10-2;Per-pulse operation at 120 Hz;
Si Diode
stages
FEL
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Pop-In Position/Profile Monitor (WBS 1.5.2)Pop-In Position/Profile Monitor (WBS 1.5.2)
Destructive; Retractable;At 50 m resolution 25x25 mm2 field of view;At 10 m resolution 5x5 mm2 field of view;
Coarse alignment of X-ray optics (beam finder)
Optical imaging of fluorescence from a scintillating screen
Positions in x, y2D intensity profile
Attenuation of beam may be required to avoid saturation
Two modes of operation: low and high resolutions
Coarse alignment of X-ray optics (beam finder)
Optical imaging of fluorescence from a scintillating screen
Positions in x, y2D intensity profile
Attenuation of beam may be required to avoid saturation
Two modes of operation: low and high resolutions
CCD Camera
YAG Screen
Mirror
FEL
stages
Yiping [email protected]
LUSI DOE Review July 23, 2007Diagnostics (WBS 1.5) 9
In-Situ Intensity/Position Monitor (WBS 1.5.4)In-Situ Intensity/Position Monitor (WBS 1.5.4)
Transmissive (> 98% w/ 100 m Be @ 8 keV);High dynamic range 106;Relative accuracy < 10-3
Position resolution < 5 m;Per-pulse operation at 120 Hz;
Precise normalization of incident intensity to 0.1%
Critical to XPP experiments where small change in diffraction intensity need to be resolved, i.e. Bi coherent phonon decay after photo-excitation
Detection techniqueCompton back scattering from Be thin foil (up to 108 photons w/ 1012 in incident beam)
Precise beam position calibration w/ use of array of sensors to < 5 m
Commercial fluorescence monitor using similar design provides equal resolution but not viable due to damage considerationsCVD diamond design more complex in fabrication
Precise normalization of incident intensity to 0.1%
Critical to XPP experiments where small change in diffraction intensity need to be resolved, i.e. Bi coherent phonon decay after photo-excitation
Detection techniqueCompton back scattering from Be thin foil (up to 108 photons w/ 1012 in incident beam)
Precise beam position calibration w/ use of array of sensors to < 5 m
Commercial fluorescence monitor using similar design provides equal resolution but not viable due to damage considerationsCVD diamond design more complex in fabrication
Be thin foil
FEL
Quad-sensor
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Electro-Optic Sampling Device (WBS 1.5.6)Electro-Optic Sampling Device (WBS 1.5.6)
Non-intrusive to e-beam;Non-destructive; Per-pulse operation at 120 Hz;
Relative timing btw e-bunch & EOS-probe laser pulse Inferring timing btw X-ray pulse &
experimental probe laser
Based on (linear) Pockels effectbirefringence in strong E-field exerted by relativistic e-bunch in proximity1-D Spatial encoding of timing for detection using CCD
Single shot measurement
EOS technique proven at SPPS20 fs timing determination200 fs resolution for e-bunch length
ChallengesLong distance btw EOS location (LTU) & experiments (NEH)120 Hz operation requires real-time processing of EOS data
Relative timing btw e-bunch & EOS-probe laser pulse Inferring timing btw X-ray pulse &
experimental probe laser
Based on (linear) Pockels effectbirefringence in strong E-field exerted by relativistic e-bunch in proximity1-D Spatial encoding of timing for detection using CCD
Single shot measurement
EOS technique proven at SPPS20 fs timing determination200 fs resolution for e-bunch length
ChallengesLong distance btw EOS location (LTU) & experiments (NEH)120 Hz operation requires real-time processing of EOS data
EOScrystal
Probe-laser footprint
Yiping [email protected]
LUSI DOE Review July 23, 2007Diagnostics (WBS 1.5) 11
Hartmann Wave-front Sensor (WBS 1.5.5)Hartmann Wave-front Sensor (WBS 1.5.5)
Characterization of wave-front of focused X-ray FEL is a challenge
Critical to CXI experiments if atomic resolution is ultimately to be achievedCommon scanning or direct imaging techniques made at focus not viable due to FEL high peak power
Hartmann Wave-front Sensor technique is viableMeasurement made far from focusFocal point determination calculated from radius of curvature measurementWave-front distortion obtained by back-propagation of diffracted wave-front determined at mask plane
Commercial Hartmann wave-front for long wavelengthSuccessful in optical applications (adaptive optics, etc.)For X-ray applications, X-EUV sensor for energy up to 4 keVNeeds modification for higher energies and 120 Hz operation
Characterization of wave-front of focused X-ray FEL is a challenge
Critical to CXI experiments if atomic resolution is ultimately to be achievedCommon scanning or direct imaging techniques made at focus not viable due to FEL high peak power
Hartmann Wave-front Sensor technique is viableMeasurement made far from focusFocal point determination calculated from radius of curvature measurementWave-front distortion obtained by back-propagation of diffracted wave-front determined at mask plane
Commercial Hartmann wave-front for long wavelengthSuccessful in optical applications (adaptive optics, etc.)For X-ray applications, X-EUV sensor for energy up to 4 keVNeeds modification for higher energies and 120 Hz operation
Yiping [email protected]
LUSI DOE Review July 23, 2007Diagnostics (WBS 1.5) 12
Hartmann Wave-front Sensor (con’t)Hartmann Wave-front Sensor (con’t)
Image obtained from
Imagine Optics, Ltd
ChallengesWorking at 8 keV
Tighter technical specs at shorter wavelengthMask must allow ray-optics approximationNew 8 keV version being developed & tested nowMask materials must be compatible with FEL application
120 Hz operation will require customizationImaging sensor readout rate not sufficient
Use pixelated detector capable of 120 Hz operationIntegrate with Controls/Data systems
ChallengesWorking at 8 keV
Tighter technical specs at shorter wavelengthMask must allow ray-optics approximationNew 8 keV version being developed & tested nowMask materials must be compatible with FEL application
120 Hz operation will require customizationImaging sensor readout rate not sufficient
Use pixelated detector capable of 120 Hz operationIntegrate with Controls/Data systems
Algorithm
Divergent
wavefront
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LUSI DOE Review July 23, 2007Diagnostics (WBS 1.5) 13
1.5 WBS1.5 WBS
1.5Diagnostics
1.5.1Physics SupportEng. Integration
1.5.2Pop-in Position
Monitor
1.5.3Pop-in Intensity
Monitor
1.5.4In-situ Intensity
Monitor
1.5.5In-situ Wave-front
Sensor
1.5.2.1Engineering &
1st article const.
1.5.2.2XPP
1.5.2.3CXI
1.5.2.4XCS
1.5.3.1Engineering &
1st article const.
1.5.3.2XPP
1.5.3.3CXI
1.5.3.4XCS
1.5.4.1Engineering &
1st article const.
1.5. 4.2XPP
1.5.4.3CXI
1.5.4.4XCS
1.5.5.1Engineering
1.5.5.2CXI
1.5.6In-situ EOS
Device
1.5.6.1Engineering
1.5.6.2XPP
Yiping [email protected]
LUSI DOE Review July 23, 2007Diagnostics (WBS 1.5) 14
Diagnostics Schedule in Primavera 3.1Diagnostics Schedule in Primavera 3.1
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LUSI DOE Review July 23, 2007Diagnostics (WBS 1.5) 15
Diagnostics MilestonesDiagnostics Milestones
CD-1 Aug 01, 07Conceptual Design Complete Oct 24, 07CD-2a Dec 03, 07CD-3a Jul 21, 08Phase I Final Design Complete Oct 24, 07EOS monitor complete Oct 20, 08Pop-in position/profiler 1st article Nov 25, 08In-situ intensity/position 1st article Jan 21, 09Pop-in intensity 1st article Apr 15, 09Phase I Installation Complete Aug 21, 09CD-4a Feb 08, 10
CD-1 Aug 01, 07Conceptual Design Complete Oct 24, 07CD-2a Dec 03, 07CD-3a Jul 21, 08Phase I Final Design Complete Oct 24, 07EOS monitor complete Oct 20, 08Pop-in position/profiler 1st article Nov 25, 08In-situ intensity/position 1st article Jan 21, 09Pop-in intensity 1st article Apr 15, 09Phase I Installation Complete Aug 21, 09CD-4a Feb 08, 10
Yiping [email protected]
LUSI DOE Review July 23, 2007Diagnostics (WBS 1.5) 16
Diagnostics Cost Estimate Diagnostics Cost Estimate
Direct Cost $2,326.2PED $700.0MS&T $1,376.2ASSY $250.0
Indirect Cost $630.0Escalation $210.0Total Cost $3,166.2
Associated Contingency 35.1%
IndirectCosts
Escalation
PED
MS&T
ASSY
DirectCosts
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LUSI DOE Review July 23, 2007Diagnostics (WBS 1.5) 17
SummarySummary
Concepts of all diagnostic devices are well developed
Frequent design discussions amongst LUSI and LCLS scientistsEOS device was successfully deployed at SPPS
1st articles will help LCLS commissioning/operation and early sciences on LUSI instruments
LUSI EOS will aid LCLS e-beam diagnosticsLUSI BPM could aid LCLS e-beam fast feedback system
Ready to proceed with baseline cost and schedule development
Concepts of all diagnostic devices are well developed
Frequent design discussions amongst LUSI and LCLS scientistsEOS device was successfully deployed at SPPS
1st articles will help LCLS commissioning/operation and early sciences on LUSI instruments
LUSI EOS will aid LCLS e-beam diagnosticsLUSI BPM could aid LCLS e-beam fast feedback system
Ready to proceed with baseline cost and schedule development