Title: Summary from TTF2 Working Group
1Summary from TTF2 Working Group Jean-Paul
Carneiro, Markus Koerfer DESY, Hamburg TESLA
COLLABORATION MEETING ORSAY, 7-Sept-2004
2TESLA COLLABORATION MEETING WORKING GROUP
TTF2 LAL ORSAY, 7-SEPT-04 Morning (9H00? 10H30,
11H00?12H30) 9H00 ? 10H30 Carneiro
Cryogenics Installations TTF2 in 2004 and Future
Plans Lange (20) TESLA Cavities in
the VUV-FEL LINAC Modules Kostin
(20) Status of the TTF-II vacuum system
Zapfe (20) Power Supplies for TTF2 and
Pulse Cable for Modulator Eckoldt
(30) 11H00 ? 12H30 Koerfer Status RF
System Choroba (15)
Commissioning of the LLRF for the VUV-FEL
Simrock (10) RF Control Improvement for
TTF II with low latency FPGA feedback Jezynski
10 VUV-FEL Controls Rehlich
(15) TTF 2 Diagnostics Status and
Availability of Toroids, BPMs, Castro (15)
3Afternoon (14H00? 16H00, 16H30?18H00) 14H00?
16H00 Carneiro TTF-VUV FEL Optical Systems
Castellano (15) Photoinjector Laser
Operation and Cathode Performance
Sertore (20) Beam based alignment, Dark
current and Thermal emittance Miltchev
(20) Status of Emittance Measurements at the
TTF/VUV-FEL Injector Honkavaara (20) First
Measurements on HOM-Based Alignment in the TESLA
Cavities Baboi (20) 16H30? 18H00 Koerfer
Improvements in LLRF control algorithms and
automatio Brandt (20)
TTF2-Time-Of-Flight Measurements
Kollewe (20) TTF2 Start-Up Simulations
Yurkov (20) TTF2 commissioning
strategy Castro
(10) Discussion about commissioning
Prepared but not presented (available on the
web) Attempt of measurement of linear
dispersion Golubeva (10) Commissioning
445-MeV Optics of the TESLA Test Facility Linac
Balandin (10) Velocity bunching simulations
for TTF2 Carneiro (10)
4Cryogenics Installations TTF2 in 2004 and
Future Plans
- -Assembly and installation of Module M2 (old
type II) - for Position ACC1
- -Commissioning of the new TTF2 set up with
- 5 Cold Accelerating Modules
- -Cool down, operation and tests of the new TTF2
set up - -Shut down June-04 until September-04
- -Cryogenic operation possibillities/redundancies
- Future
- -Preparation and assembly Module M6 (new type 3)
- -Fermilab buildts 3rd Harmonic Module (3.9GHz)
- -Cryogenic supply for Superconducting Magnetic
Energy Storage SMES - -Module Teststand
- -Update Cold Box Hall 3 (2 new screw compressors
already in operation)
R. Lange
5TTF2 since March 2004
Automated Cryo-operation for TTF2-Linac
Linac Transfer
From/to CB HERA or CB Hall 3
Fermilab Feedbox
BCBTL2
BCBTL1
ACC2 Transferl
ACC1 Transferl
VB
VB
Endcap
ACC5 M5
ACC4 M4
ACC1 M2
ACC2 M1
ACC3 M3
BC2
BC3
Overview 21-Mar-04 Start cool down 28-Mar-04
4.3K/1.1bar 29-Mar-04 2 K / 31mbar 07-Jun-04
Shut down, but modules
stay cold at 4.3K/1.1bar 01-Sep-04 End of shut
down
GUN
Cryo losses static Watt Total Module 40/80K 1
300 74 4.3K 3201.6g/s 13 2.0K
21 lt3.5
R. Lange
6TESLA Cavities in the VUV-FEL LINAC Modules
D. Kostin
7Modules Operating Gradients
ACC3
ACC4
ACC5
ACC2
ACC1
D. Kostin
8Cavities _at_ ACC1
EP cavity
D. Kostin
9EP Cavities
(AC72 is installed in ACC1)
D. Kostin
10S. Choroba
11S. Choroba
12S. Choroba
13S. Choroba
14S. Choroba
15S. Simrock
16S. Simrock
17K. Zapfe
18K. Zapfe
19K. Zapfe
20K. Zapfe
21K. Rehlich
22K. Rehlich
23K. Rehlich
24TTF 2 Diagnostics Status andAvailability of
Toroids, BPMs,
Prepared by D. Nölle
P. Castro
25STATUS
- Installation of diagnostics is completed
- exception BPM electronics
- BPM electronics available by end of 2004 (first
boards maybe in November). - For the commissioning use 20-15 TTF1 electronics
(DESY Frascati units) - Not useful for undulator (lt- Electronics
container inside the tunnel) - Problem Orbit tuning is not possible to required
precision - in the collimator
- in the undulator
P. Castro
26TTF/VUV-FEL Photon DiagnosticsStatus and
Availability
Prepared by R. Treusch
P. Castro
27Availability of VUV FEL diagnostics
Parameter Detector(s) Online available
Intensity Profile thermopiles, PtSi photodiodes, MCPs no no limited now
Intensity Position Gas Ionisation Detector YES April 2005
Spectrum Grazing incidence spectrometer (tunnel) no now (Commissioning)
Spectrum VLS Grating Spectrom. YES mid/end 2006
Timing Streak camera YES April 2005
Timing Auto-/Cross-Correlators YES ? (experimental stage)
P. Castro
28TTF-VUV FEL Optical Systems
LNF Frascati L. Cacciotti M. Castellano G.
Di Pirro O. Giacinti R. Sorchetti
Roma 2 L.Catani E. Chiadroni A.Cianchi M.
Raparelli
DESY K. Honkavaara
M. Castellano
29Total Camera Number
18 Standard Optical System 3 Gun Camera 4 Fixed
magnification (1 BC2 3 Bypass) 2 Diffractors
All of them are working
M. Castellano
30M. Castellano
31K. Honkavaara
32K. Honkavaara
33K. Honkavaara
34K. Honkavaara
35D. Sertore
36D. Sertore
37D. Sertore
38Beam based alignment, Dark current and Thermal
emittance measurements J-H.Han,M.Krasilnikov,V.Mi
ltchev, PITZ, DESY, Zeuthen
- Beam based alignment
- Laser alignment
- Solenoid alignment
- Dark current
- Thermal emittance
V. Miltchev
39Beam Based Alignment Conclusions
- Beam based alignment (BBA) of the gun can be
done in two consequent steps - 1. Alignment of the laser on the cathode
- 2. Solenoid alignment
- Beam based laser alignment at PITZ is a
well-established procedure. To implement it at
TTF a calibrated camera at double diagnostic
cross screen is required - Mechanical beam line misalignment complicates
the BBA, introducing an additional uncertainty - Some steps in the gun solenoid alignment have
been done. It is complicated by an uncertainty
introduced by mechanical beamline misalignment,
not perfectly aligned laser on the cathode and
some uncertainty in machine parameters (rf field
amplitude and absolute phase, solenoid
calibration). For further alignment more detailed
study is needed.
V. Miltchev
40Modeling of the Field Emission Source
Well conditioned (less dark current)
Edge of the Mo plug 8000 macro particles
Edge of Cs2Te film 2000 macro particles
Cs2Te flim (5 mm ?) 2000 macro particles
Mo plug (16 mm ?) 8000 macro particles
V. Miltchev
41FC1 and FC2 (42 MV/m)
Faraday cup 1
Faraday cup 2
Main reason of the mismatch between measurement
and simulation beamline misalignment and the
effect of steerers. ? lower energy part of the
dark current is filtered out.
V. Miltchev
42Thermal emittance measurements
- The final goal is to estimate the average kinetic
energy Ek of the emitted photo electrons. - Assuming isotropic emission
- An estimate for could be given by
measuring the transverse - emittance vs. laser spot r.m.s. size s,
provided that eRF, eSC 0 - Use very small charge (2-3 pC) and short laser
pulses (6-8 ps FWHM) - Use single slit scanning and/or solenoid scan to
measure emittance - Check the dependence of the transverse emittance
on applied electric field on the cathode -
V. Miltchev
43Thermal emittance measurements
Transverse emittance for different r.m.s. laser
spot sizes measured with the single slit scanning
method at a charge of about 3pC and an
accelerating gradient at the cathode of 32 MV/m.
V. Miltchev
44Thermal emittance measurements
Summary
- The transverse emittance was measured for very
low charge of 2-3 pC and short laser pulses of
6-8 ps FWHM - The scaling of transverse emittance with laser
spot r.m.s. size was measured - The average kinetic energy Ek of the emitted
photo electrons was estimated to be 0.8 0.1eV - Thermal emittance was measured as a function of
the applied field a the cathode - An increasing of the thermal emittance with
accelerating gradient was observed -
V. Miltchev
45N. Baboi
46N. Baboi
47N. Baboi
48M. Kollewe
49M. Kollewe
50M. Kollewe
51M. Kollewe
52M. Kollewe
53M. Yurkov
54M. Yurkov
55M. Yurkov
56M. Yurkov
57TTF2 commissioning strategy
P. Castro
P. Castro
58BEAM COMMISSIONING STEPS - SUMMARY
- re-commissioning of gun injector
- setup cavity phases ACC2-5 ? beam energy
- setup bunch compression
- setup beam linear optics, optimize orbit
- commissioning of diagnostics
1st beam (bypass)
3 weeks
- setup collimation
- emittance measurements and optics matching
- beam-based alignment in undulator section
- commiss. of photon diag. with spon. emission
FEL 30 nm 1 bunch
10 weeks
Saturation 6-100 nm
- commissioning of FEL diagnostics
- study of FEL beam, compression schemes, etc.
- establish reproducible settings, etc.
8 weeks
P. Castro