Study of the space charge effects for J-PARC Main Ring Alexander Molodozhentsev (KEK) SAD Workshop, September 5-7, 2006.

Slides:



Advertisements
Similar presentations
Current Status of Virtual Accelerator at J-PARC 3 GeV Rapid Cycling Synchrotron H. Harada*, K. Shigaki (Hiroshima University in Japan), H. Hotchi, F. Noda,
Advertisements

Dr. Zafer Nergiz Nigde University THE STATUS OF TURKISH LIGHT SOURCE.
Helmholtz International Center for Oliver Boine-Frankenheim GSI mbH and TU Darmstadt/TEMF FAIR accelerator theory (FAIR-AT) division Helmholtz International.
Space Charge meeting – CERN – 09/10/2014
Impedance measurements at SLS E. Koukovini-Platia CERN, EPFL TIARA mid-term meeting, Madrid, 13 th June 2012 Many thanks to M. Dehler, N. Milas, A. Streun.
Searching for Quantum LOVE at the Australian Synchrotron Light Source Eugene Tan On behalf of Rohan Dowd 120/10/2010Eugene Tan – IWLC 2010, Genega ASLS.
Resonance Crossing Experiment in PoP FFAG (preliminary report) M. Aiba (Tokyo Univ.) for KEK FFAG Group FFAG W.S. KEK.
100 MeV- 1 GeV Proton Synchrotron for Indian Spallation Neutron Source Gurnam Singh Beam Dynamics Section CAT, Indore CAT-KEK-Sokendai School on Spallation.
Yichao Jing 11/11/2010. Outline Introduction Linear lattice design and basic parameters Combined function magnets study and feasibility Nonlinear dynamics.
S.J. Brooks RAL, Chilton, OX11 0QX, UK Options for a Multi-GeV Ring Ramping field synchrotron provides fixed tunes and small.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, N.Kazarinov.
3 GeV,1.2 MW, Booster for Proton Driver G H Rees, RAL.
Virtual Accelerator at J-PARC 3 GeV Rapid Cycling Synchrotron H. Harada*, K. Shigaki (Hiroshima University in Japan), H. Hotchi, F. Noda, H. Sako, H. Suzuki,
New Progress of the Nonlinear Collimation System for A. Faus-Golfe J. Resta López D. Schulte F. Zimmermann.
Studies on Lattice Calibration With Frequency Analysis of Betatron Motion R. Bartolini DIAMOND Light Source Ltd FMA workshop, Orsay, LURE, 1 st and 2 nd.
Details of space charge calculations for J-PARC rings.
Advanced Accelerator Design/Development Proton Accelerator Research and Development at RAL Shinji Machida ASTeC/STFC/RAL 24 March 2011.
J-PARC Accelerators Masahito Tomizawa KEK Acc. Lab. Outline, Status, Schedule of J-PARC accelerator MR Beam Power Upgrade.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, A.Drozhdin, N.Kazarinov.
Dynamic Aperture Study for the Ion Ring Lattice Options Min-Huey Wang, Yuri Nosochkov MEIC Collaboration Meeting Fall 2015 Jefferson Lab, Newport News,
1 FFAG Role as Muon Accelerators Shinji Machida ASTeC/STFC/RAL 15 November, /machida/doc/othertalks/machida_ pdf/machida/doc/othertalks/machida_ pdf.
Part III Commissioning. Proof of Principle FFAG (POP) study The world first proton FFAG –Commissioned in March –From 50 keV to 500 keV in 1ms. –Proof.
Electron Model for a 3-10 GeV, NFFAG Proton Driver G H Rees, RAL.
Beam Loss Simulation in the Main Injector at Slip-Stacking Injection A.I. Drozhdin, B.C. Brown, D.E. Johnson, I. Kourbanis, K. Seiya June 30, 2006 A.Drozhdin.
A U.S. Department of Energy Office of Science Laboratory Operated by The University of Chicago Office of Science U.S. Department of Energy Containing a.
Main Ring + Space charge effects WHAT and HOW … Alexander Molodozhentsev for AP_MR Group May 10, 2005.
Alexander Molodozhentsev KEK for MR-commissioning group September 20, 2005 for RCS-MR commissioning group September 27, 2005 Sextupole effect for MR -
‘Computer power’ budget for the CERN Space Charge Group Alexander Molodozhentsev for the CERN-ICE ‘space-charge’ group meeting March 16, 2012 LIU project.
Vertical Emittance Tuning at the Australian Synchrotron Light Source Rohan Dowd Presented by Eugene Tan.
Frequency Map Analysis Workshop 4/2/2004 Peter Kuske Refinements of the non-linear lattice model for the BESSY storage ring P. Kuske Linear Lattice My.
Nonlinear Dynamic Study of FCC-ee Pavel Piminov, Budker Institute of Nuclear Physics, Novosibirsk, Russia.
1 NICA Collider: status and further steps O.S. Kozlov LHEP, JINR, Dubna for the NICA team Machine Advisory Committee, JINR, Dubna, October 19-20, 2015.
28-May-2008Non-linear Beam Dynamics WS1 On Injection Beam Loss at the SPring-8 Storage Ring Masaru TAKAO & J. Schimizu, K. Soutome, and H. Tanaka JASRI.
1 EMMA Tracking Studies Shinji Machida ASTeC/CCLRC/RAL 4 January, ffag/machida_ ppt & pdf.
J-PARC Accelerator and Beam Simulations Sep. 7th, SAD2006 Masahito Tomizawa J-PARC Main Ring G., KEK Outline of J-PARC Accelerator Characteristics of High.
Simulation of resonances and beam loss for the J-PARC Main Ring Alexander Molodozhentsev (KEK) Etienne Forest (KEK) for the ICFA HB08 Workshop ICFA HB08.
H. Bartosik, Y. Papaphilippou. PS2 meant as potential replacement of existing PS PS2 main characteristics given by LHC requirements – Circumference defined.
J-PARC Spin Physics Workshop1 Polarized Proton Acceleration in J-PARC M. Bai Brookhaven National Laboratory.
PTC-ORBIT code for CERN machines (PSB, PS, SPS) Alexander Molodozhentsev (KEK) Etienne Forest (KEK) Group meeting, CERN June 1, 2011 current status …
FMA workshop April 1st and 2nd, 2004 L. Nadolski1 Guiding Lines for Computing and Reading a Frequency Map New FMA Calculations for SOLEIL including Insertion.
By Verena Kain CERN BE-OP. In the next three lectures we will have a look at the different components of a synchrotron. Today: Controlling particle trajectories.
The Introduction to CSNS Accelerators Oct. 5, 2010 Sheng Wang AP group, Accelerator Centre,IHEP, CAS.
Off-momentum DA of RCS 3D_BM & QFF & CC AP meeting / December 8, 2004 Alexander Molodozhentsev Etienne Forest KEK.
Space charge studies at the CERN PS A. Huschauer, Raymond Wasef H. Damerau, S. Gilardoni, S.Hancock, D. Schoerling, R. Steerenberg Acknowledgements: All.
Pushing the space charge limit in the CERN LHC injectors H. Bartosik for the CERN space charge team with contributions from S. Gilardoni, A. Huschauer,
The nonlinear dynamics of SIS100 at injection G. Franchetti Beam dynamics meet Magnets II 18/4/2012G.Franchetti1 Magnet multipoles: Dipole: Akishin et.
Thomas Roser SPIN 2006 October 3, 2006 A Study of Polarized Proton Acceleration in J-PARC A.U.Luccio, M.Bai, T.Roser Brookhaven National Laboratory, Upton,
Beam Diagnostics Seminar, Nov.05, 2009 Das Tune-Meßverfahren für das neue POSI am SIS-18 U. Rauch GSI - Strahldiagnose.
Beam Loss Budget during Injection Process for MR Alexander Molodozhentsev KEK for RCS-MR group meeting
ICFA mini-Workshop on Beam Commissioning for High Intensity Accelerators Yasuhiro Watanabe (J-PARC / JAEA) Tracking between bending and quadrupole families.
J-Parc Neutrino Facility Primary Proton Beam Design A. K. Ichikawa(KEK), Y.Iwamoto(KEK) and K.Tanabe(Tokyo) et.al. 7 th Nov. 2003,
C. Biscari, D. Alesini, A. Ghigo, F. Marcellini, LNF-INFN, Frascati, Italy B. Jeanneret, CERN, Geneva, Switzerland CLIC DRIVE BEAM FREQUENCY MULTIPLICATION.
Halo Collimation of Protons and Heavy Ions in SIS-100.
Optimization of the Collider rings’ optics
A.Lachaize CNRS/IN2P3 IPN Orsay
Space charge studies at the SPS
Multi-Turn Extraction studies and PTC
Beam-beam effects in eRHIC and MeRHIC
Large Booster and Collider Ring
Sabrina Appel, GSI, Beam physics Space charge workshop 2013, CERN
Jeffrey Eldred, Sasha Valishev
Multiturn extraction for PS2
Beam-beam R&D for eRHIC Linac-Ring Option
Beam dynamics study for J-PARC Main Ring with PTC-ORBIT
Update on PTC/ORBIT space charge studies in the PSB
Preliminary results of the PTC/ORBIT convergence studies in the PSB
Electron Rings Eduard Pozdeyev.
Optics Measurements in the PSB
Yuri Nosochkov Yunhai Cai, Fanglei Lin, Vasiliy Morozov
JLEIC Ion Integration Goals
Presentation transcript:

Study of the space charge effects for J-PARC Main Ring Alexander Molodozhentsev (KEK) SAD Workshop, September 5-7, 2006

2 Outline of the talk:  Main parameters of J-PARC Main Ring  Tool-Box and Model for the space charge study for MR  Resonance excitation and Emittance growth  Lost beam power for MR

3 J-PARC Accelerator Complex LINAC RCS Main Ring

4 J-PARC Main Ring: Features Injection Energy3 GeV Extraction Energy50 GeV (Maximum) Circumference m Maximum Beam Power0.75 MW * for 50 GeV Repetition Rate0.285 Hz (T per ~ 3.5sec) Harmonic Number9 8 bunches Nominal Tune (x/y)22.4/20.8 Natural Chromaticity (x/y)~ -30 Beam Emittance / Chamber Acceptance 54 / 81 .mm.mrad 1.Imaginary Transition gamma: the missing bend structure 2.Slow extraction scheme based on the 3Q x resonance (3Q x =67) * … needs in 1MW beam power from RCS

5 J-PARC Main Ring: Beam Power “Day-1”“Day-2” LINAC Energy [MeV] RCS Beam Power at 3 GeV [MW] MR Beam Power at 3 GeV [kW] ~ 4.76% from RCS Beam Power 13.7 – MR Beam Power at 50 GeV [kW]228.5 – MR Harmonic Number Number of Bunches Beam Intensity  – “Free-space” incoherent space charge tune shift (W k =3GeV, Uniform:54  mm.mrad, B f ~ 0.2 * ) ~(- 0.04) – (-0.08) ~ (-0.13) * “Fundamental” harmonic RF-cavity

6 J-PARC Main Ring: Strict Limitation of Beam Losses Technical Design Requirement: MR Collimator should accept about 1% from the total beam power Maximum particle losses at the MR collimator at the injection energy should be less than 450W. Other areas around MR:: < 0.5W/m Behavior of the 99% emittance … Study of the Halo formation

7 Step 1: Single particle dynamics (COSY Infinity / M.Berz et al.)  Combined effect of fringe field of the MR magnets and the ‘chromatic’ sextupole fields … Main field nonlinearity for MR is the ‘chromatic’ sextupole fields.  Optimization of the ‘bare’ working point for MR … Recommended ‘bare’ working points are located in the region with the following betatron tunes to provide maximum beam survival at the MR scraper: Q x = 22.4 / Q y = 20.8 and Q x = / Q y = 20.9 (Requirements: the ‘bare’ working point should be located near the 3Q x =67 resonance line to use this resonance for the ‘slow’ extraction; the expecting space charge tune-shift is about  Q SpCh = -0.2).

8 TOOL-Box: ORBIT-MPI Step 2: Multi particle tracking with ring dynamics and loss detection around the ring. External E&M fields (LINEAR & NONLINEAR) :  Symplectic Tracking (“Teapot” type: Drift-Kick) Space charge force:  self-consistent solution based on the PIC model with FFT (non-symplectic … convergence study)

9 A.Shishlo talk (SNS) / April 21, 2004

10 Space charge model for Main Ring (ORBIT-MPI)  At the injection energy the transverse beam size (< ± 6cm) is much smaller than the longitudinal one ( ~ 50m, for B f = 0.3) and the synchrotron oscillation is slow (~ 500 turns) … then the (2&1/2)D FFT model for the space charge simulation can be used at least at the beginning.  Poisson FFT solver with boundary conditions to involve the beam environment into calculation.  Initial particle distribution for MR should be the ‘realistic’ one, obtained after the RCS tracking study… we used for this study the RCS particle distribution at 3GeV.

11 Convergence study for MR (c5) Particle losses at the MR scraper position (60  mm.mrad) for different number of the macro-particles: 200’000 mp & 100’000 mp N FFT = 100x100 N az = 1100 N bin = 512 Bare working point: Qx = / Qy = 20.82

12 Footprint for 1.8 kW/bunch, B f =0.2(LM) Laslett incoherent tune shift (estimation) :  Parab.100% = 54  mm.mrad::  incoh ~ (for  ~1) Rectangular beam pipe ::  70 mm WP#1: Qx=22.43, Qy=20.82WP#2: Qx=22.30, Qy=20.92 Footprint after 5000 turns Q y =21 Q x +Q y =43 2Q x -Q y =24 3Q y =62 2Q x +Q y =65 Q x +Q y =43

13 Space charge tune shift 3.6kW/bunch, B f =0.2LM QxQx QyQy 4Q x = 90 2Q x –2Q y =3 4Q x =89 Q x +2Q y =64 4Q y = 83 3Q x =67 -Q x +2Q y =19 ‘ Bare’ working point: Q x0 = Q y0 = Chromatic tune shift (after correction) ∆ CH ~ for ∆p/p = ± 1% Amplitude dependent tune shift ∆ AM ~ for 54  mm.mrad Incoherent space charge tune shift (including chamber boundary ± 70mm) (0.6MW, RCS_Beam_050906, B f = 0.2, L-matched initial beam distribution) ∆ SpCh ~ RCS Beam Power = 0.6 MW / 3NBT_CLM = 54  Q x + Q y =43 3Q y = 62 2Q x – Q y =24

14 Resonance excitation for MR ResonanceHarmonic number Type of resonance Source of resonance * Status [2,0]45Normal ‘quadrupole’ Q-error & misalignment  [3,0] [1,2], [-1,2] Normal ‘sextupole’ Sextupole field comp. in BM + Sextupole errors + FF_BM  [4,0],[2,-2], [2,2], [0,4] 90, 3 86, 83 Normal ‘octupole’ Space charge Sextupole Field  [1,-1]43Skew ‘quadrupole’Magnet errors, Q magnet tilt ----  [0,3], [2,1], [2,-1] 62, 65, 24 Skew ‘sextupole’Magnet error, SX magnet tilt ----  * … at the leading order

15 Measured * field components, involved into consideration …  Sextupole component of MR Bending magnets (96+1) at the injection energy… MAD ~ 5.2  [m -2 ] :: 1  = 4.2  [m -2 ], cut=3 .  Sextupole component of MR Sextupole magnets (72) at the injection energy … average relative deviation from the required values is |  b 3 | < * Measurement has been performed by using the rotating coil (March, 2006)  Quadrupole strength of MR Quadrupole magnets (216) at the injection energy … {  B / L /(B / L)} k :: 1  = ×10 -4, cut = 4  Location of each magnet is fixed after the shuffling procedure.

16 Injection study: Edge focusing … Vertical  -beating effect:: (  /  ) y ~ 2…3 % (without quadrupole components of OMS) Timing of Opposite Field Magnet Septum

17 Space Charge effect & Nonlinearities: ‘IDEAL’ lattice Beam Power: 1.8kW/bunch 99% emittance (H/V) vz Turns_Number for different ‘bare’ working points Emittance growth is caused by the ‘structure’ resonances: combined effect of the space charge and the sextupole field nonlinearity: 4Q x =90 and 2Q x -2Q y =3.

18 Effect of the emittance growth in both transverse phase planes has been observed for both ‘bare’ working points. Explanation of the effect:  for the working point with Q x =20.42, the ‘tail’ particles can be trapped by the 4Q x =90 resonance, excited first of all by the sextupole field nonlinearities of the chromatic sextupole magnets (the second-order effect of the sextupole nonlinearity) … plus the coupling effect, caused by the 2Q x -2Q y =3 resonance.  for the working point with Q x =20.42, the ‘tail’ particles have influence of the ‘lattice’ resonance Q y =21 … … plus the coupling effect, caused by the 2Q x -2Q y =3 resonance. Space Charge effect & Nonlinearities: ‘ideal’ lattice

19 Effect of the Injection Dogleg Wp1: Q x = 22.42, Q y = Injection ‘dogleg’:  break the MR super-periodicity  Excitation of ‘non-structure’ resonances, in particular [1,2,64], [3,0,67] and [0,4,83]

20 Excitation non-structure resonances Normal quadrupole resonances in addition to normal sextupole&octupole resonances  Add to simulations … quadrupole strength errors (measured) in combination with the measured sextupole components of the dipole magnets and the measured sextupole strength errors. After the ‘shuffling’ procedure’ the positions of BM/QM/SM have been fixed. Skew quadrupole and sextupole resonances  Add to simulations … misalignment error (transverse tilt) of the quadrupole and sextupole magnets

21 Budget of the beam losses Lost % Lost Power 1st W 2nd W 3rd W 4th W Total3.45%124.2 W MR Scraper Acceptance = 70  mm.mrad Batch number MR Beam Power: 1.8kW/bunch … RCS Beam Power: 0.3MW B f = 0.2 (V RF =210kV) NO Tilt NO Q_Err 250 W

22 Estimation of Particle Losses (dual harmonic RF, B f = 0.3) ATAC’06 60  70  1st0.2%0.1% 2nd1.5%0.35% 3rd3%0.92% 4th4.5%1.63% Lost Power ~ 662 W~ 216 W MR Scraper Acceptance Batch number Mismatched initial longitudinal distribution RCS Beam Power = 0.6 MW / 3NBT_CLM = 54  ‘Bare’ working point: Q x0 = Q y0 = NO Errors

23 Acceleration: Particle losses at MR Scraper Total losses for 8 bunches (h=9) ~ 50 W Wp#1 Realistic RF&BM-table NO Errors !!!

24 ORBIT_MPI: Multi-Processor Machine operation Dell PowerEdge 6800: QUAD 64-bit Intel Xeon Processors: … computational performance in a range of a few GFlops/CPU. ~ 100’000 mp (2&1/2 model)... 1 day :: ~ 3500 turns KEK SuperComputer (A):: HITACHI SR11000 model K1 (April 2006) … calculation server consisted of 16 nodes, each node has 16 CPUs (total 256CPUs). The total peak performance is 2.15 TFlops (or GFlops/node) and the maximum memory is 32GB/node. Users have access at the same time to 4 nodes maximum (64 CPUs). The CPU peak performance is about 8.4 GFlops/CPU. Expected reduction of the simulation time is ~ 20 times.

25 Conclusion: To provide reliable estimation of the emittance growth (in particular, the 99% emittance behavior) and the particle losses for the ‘real’ machine operation study, it is necessary to use the space charge tracking code, like ORBIT_MPI, designed for multi-CPU computers. For MR study we introduced different resonance excitation step-by-step by using measured field data. Estimated particle losses at the MR scraper is below the acceptable level. Thanks for your attention.