Title: Future UCLA Work in High Brightness Beams and FEL at BNL ATF: Compression and VISA II
1Future UCLA Work in High Brightness Beams and FEL
at BNL ATF Compression and VISA II
James Rosenzweig UCLA Department of Physics and
Astronomy
- ICFA Sardinia
- July 4, 2002
2VISA I
- VISA completed last year, measuring a large range
of phenomena - Exponential gain and saturation
- Statistics
- Angular, wavelength spectrum
- Microbunching with CTR
- Operating point was pathological
- Strong compression due to nonlinear properties of
beamline 3 - Extremely sensitive system to rf phase jitter
- Information on initial longitudinal phase space
lost - Needed brave effort on experiment and
start-to-end simulation to unfold - Can we do a more linear experiment, with
desired longitudinal phase space? - Can we compress the beam in a more standard way?
3UCLA Compressor _at_ ATF
- Compressor project begun 2.5 years ago to provide
ATF with chicane - ONR funding (C. Roberson)
- Extrapolation of Neptune/FTF experience to higher
energies - Brought need to model systems with CSR (VISA
start-to-end!) - CSR, longitudinal and transverse phase effects
- Status
- Magnets shipped 5/02
- Vacuum vessel ships now
- New funding!
4Physics Goals of Compressor/VISA II
- Compress beam to 20 micron bunch length level
- Study CSR production directly in chicane
- Longitudinal phase space after chicane
- Transverse phase space diagnosis (a la Neptune?)
- Mitigate severe nonlinearity of bend beamline
- Diagnose beam completely at end of transport
- FEL studies with compressed beams
- Use FEL as diagnostic of compressor
- FEL studies with chirped, but uncompressed beams
- Impact LCLS schemes using chirping
- Study gain v. chirp
- Direct diagnosis of FEL longitudinal pulse
characteristics
5Compression experiments
- New funding from Roberson
- Very interested in CSR problems
- Personnel involved (JBR)
- Ron Agusstson
- Alex Murokh
- Sven Reiche
- Compression effects
- Tokyo polychromator
- Remove SDL ambiguities
- Energy spectrum measurements
- CSR instability
- What kind of beam do we expect?
- Can we take send this beam to the VISA undulator
in useful form?
6VISA I Review Beamline
(Beamline 3)
Insert compressor here
- Gun and Linac Section (1.6 cell photo-emission
gun and 2 SLAC type linac structures operating at
S-Band, generate 71 MeV beam) - 20 double-bend dispersive transport section
- Beamline III, with VISA matching optics and 4-m
strong focusing undulator (K1.26)
7Transport to Beamline 3
- Initially an FEL radiation pulse energy was
measured 1-10 nJ, in agreement with the
measured beam brightness.
- In the attempt to compensate for the dispersion,
a new tune was developed
- With the new tune the FEL radiation intensity
went up to 10 µJ. Why?
8Saturation Measurements and Physical Model
- With the high gain an FEL saturation in 3.6 m was
observed
Lg 18.7 cm
- How does the gain length measurement agree with
the high gain SASE-FEL theory? Not that well if
we believed beam parameters at linac exit
9More inconsistencies in the data
- Highest gain observed after changing rf phase of
linac - Change of the tune significantly altered all SASE
radiation properties, indicating changes of basic
electron beam properties
many spikes spike width 0.1 centered at 830 nm
single spike spike width 1 centered at 845 nm
(old tune)
(new tune)
10 Bunch compression in beamline 3
- High gain observed for running 4 degrees forward
of crest horizontal beam size expands inside of
undulator (dispersion error) - Strong bunch compression in the dispersive
section was suggested, due to mistuning of linac
energy from the nominal value. Effective R56 can
change sign, order of magnitude due to T566, off
energy operation.
-10
- Increase in peak current reduces FEL gain length,
explains the observed spectral behavior (watch
for e?growth due to dispersion mismatch) - Longitudinal transformation highly nonlinear
horizontal/long. coupling - Measure compression in final VISA runs!
11PARMELA/ELEGANT Analysis
- PARMELA reproduced the beam properties measured
after the linac, and ELEGANT simulated bunch
compression in the double-bend line. - ELEGANT is input off-design energy, with
appropriate chirp for high gain case
PARMELA output after linac
ELEGANT output after dispersive section (no
collimation). Note width, mainly due to T512
12Emittance Growth in Dispersive Section
- CSR effect on emittance is insignificant
- De?CSRgt 0.3 mm-mrad
Residual dispersion, nonlinearities dominate
e?Dp/pgt 7 mm-mrad
Slice emittance of the lasing beam core stays
below e?slicegt lt 4 mm-mrad
Now we have a detailed, benchmarked model of the
beam sent into the undulator
13Single Golay Cell Measurements
- Initial test indicated strong CTR signal
dependence on linac RF phase.
Peaked SASE Signal
- Low pass filter in/out comparison (R0.68)
indicated short (sub-40 µm) bunch length.
- Ratio measurement at the operating point
established a benchmark for the PARMELA/ELEGANT
numerical model of the system.
14Comparison with CTR Measurements
- Manipulating the beam energy and chirp
(equivalent to linac RF phase detuning) allowed
reproduction of the bunch compression measured
experimentally.
Simulated current
Simulated CTR from the ELEGANT beam current
output good agreement with measurement.
15Start-to-end GENESIS simulations
- GENESIS output is in excellent agreement with FEL
gain, angular profile
- Statistics of saturation also benchmarked with
start-to-end mode - Details count!!! Must know as much about phase
space as possible.
16Example effect of CSR on compressed beam
- Beam bunch length is T516/T526/emittance limited
(emittance must be 2 mm-mrad) - CSR provides energy loss mechanism during bends
- This can interact with the T516/T526 terms to
produce longer beam - No-CSR case has 300 A, not 250 A - GENESIS gain
is far too large.
No CSR
CSR
Correlated cut due to collimator, T516/T526
Width set by T516/T526
17Compression experiments
- New funding from Roberson
- Very interested in CSR problems
- Personnel involved (JBR)
- Ron Agusstson
- Alex Murokh
- Sven Reiche
- F. Chou (Cline group)
- INFN-SPARC invited to join experiments
- What kind of beam do we expect?
- What are the interesting measurements?
- What can we do with this beam?
18Note compressor and BL3 bends are orthogonal
ELEGANT study of compression/transport
19Coherent radiation experiments
- Study CSR and CTR
- Coherent synchrotron radiation from bend 3/4
edges - Dedicated port
- Beam is shortest there!
- Enhanced radiation
- CTR after final dipole
- Wavelengths too short for interferometry? (SDL
meas.) - Spectrum of direct interest
- Tokyo polychromator
- Poor-mans version w/filters
CSR port, aimed at Dipole 4 entrance
20Phase space measurements
- Momentum spectrum from horizontal bend
- Transverse phase space tomography
- Does the phase space bifurcate (S. Schreiber says
yes)? - Momentum (not time) resolved tomography
-
21VISA-II prospects
- LCLS demands path to shorter (few fs!) pulse
lengths - Chirped beam/slicing
- Chirped beam/compression
- Proposed experiments using
- Chirped, compressed beam
- Chirped, uncompressed beam
- Compress FEL output. Use FROG to diagnose?
- ONR funding on the way for compressor/VISA-b this
summer - First job for FEL fix transport in BL3 to allow
chirping - Offset linear negative R56 (compressor setting)
- Correct T566
Saturation in 3 m with compressed beam (GENESIS)
22Mitigation of Nonlinearity Originally Studied for
S-Bahn at Neptune
Simulation results after S-Bahn from Elegant
Without Sextupoles (T566 -1.9 m)
RAMPED BEAM
WITH Sextupoles (T566 0)
23Sextupole correction of BL3 dynamics
Initial Phase Space
Final Phase Space (NO Sextupoles)
T566 -10 m
Final Phase Space (WITH Sextupoles)
T566 1.1 m
24Sextupoles for Neptune and ATF
- Length 5cm Gap 4cm
- B0-0.000074 T
- K10.836m-2(Nept), 0.138m-2 (ATF)
- B0.034 T/m
- K2914 m-3(Nept), 152 m-3 (ATF)
- B 36.9 T/m2
- Op Current 100 Amps
25Issues for VISA II
- What kind of energy spreads can be transported
- Better transport in BL3
- Need to develop methods to confirm linearity of
longitudinal transport - CTR
- Uncompressed beam can use streak camera
- Photon measurement really demands ways of
measuring time structure - Nonlinear harmonic crystal (crude measurement)
- SS autocorrelation with crystal
- FROG
26People and time
- UCLA people
- Pellegrini, Rosenzweig
- Murokh, Reiche
- Agusstson, Andonian
- Collaborators
- BNL
- SLAC
- INFN-SPARC
- A. Tremaine (LLNL)
- Schedule
- Compressor begins now
- VISA inspection soon
- Sextupoles in queue