Lecture17(Course Summary).PPT - E. Wilson - 3/3/2016 - Slide 1 COURSE SUMMARY A Design Study of a Compressor ring for A Neutrino Factory MT 2009 E. J.

Slides:



Advertisements
Similar presentations
ISS meeting, (1) R. Garoby (for the SPL study group) SPL-based Proton Driver for Facilities SPL-based Proton Driver for Facilities at CERN:
Advertisements

Proton / Muon Bunch Numbers, Repetition Rate, RF and Kicker Systems and Inductive Wall Fields for the Rings of a Neutrino Factory G H Rees, RAL.
1 ILC Bunch compressor Damping ring ILC Summer School August Eun-San Kim KNU.
2nd EuroNu Plenary Meeting Review of CERN Proton Driver bunch compression studies 02/06/2010M.M. - EUROnu1.
Beam stability in the SPL - Proton Driver accumulator for a Neutrino Factory at CERN E.Benedetto (CERN) 21/7/09 NUFACT’09 Workshop, July ‘09.
Thomas Roser Snowmass 2001 June 30 - July 21, MW AGS proton driver (M.J. Brennan, I. Marneris, T. Roser, A.G. Ruggiero, D. Trbojevic, N. Tsoupas,
ALPHA Storage Ring Indiana University Xiaoying Pang.
Sergey Antipov, University of Chicago Fermilab Mentor: Sergei Nagaitsev Injection to IOTA ring.
(ISS) Topics Studied at RAL G H Rees, RAL, UK. ISS Work Areas 1. Bunch train patterns for the acceleration and storage of μ ± beams. 2. A 50Hz, 1.2 MW,
Storage Ring : Status, Issues and Plans C Johnstone, FNAL and G H Rees, RAL.
S.J. Brooks RAL, Chilton, OX11 0QX, UK Options for a Multi-GeV Ring Ramping field synchrotron provides fixed tunes and small.
August 27, 2006R. Garoby Introduction 5 GeV version of the SPL Scenarios for accumulation and compression Conclusion SPL-BASED 5 GeV PROTON DRIVER.
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.
Proton Driver: Status and Plans C.R. Prior ASTeC Intense Beams Group, Rutherford Appleton Laboratory.
EDM2001 Workshop May 14-15, 2001 AGS Intensity Upgrade (J.M. Brennan, I. Marneris, T. Roser, A.G. Ruggiero, D. Trbojevic, N. Tsoupas, S.Y. Zhang) Proton.
Update of 3.2 km ILC DR design (DMC3) Dou Wang, Jie Gao, Gang Xu, Yiwei Wang (IHEP) IWLC2010 Monday 18 October - Friday 22 October 2010 Geneva, Switzerland.
Beam dynamics on damping rings and beam-beam interaction Dec 포항 가속기 연구소 김 은 산.
Advanced Accelerator Design/Development Proton Accelerator Research and Development at RAL Shinji Machida ASTeC/STFC/RAL 24 March 2011.
1 Muon Acceleration and FFAG II Shinji Machida CCLRC/RAL/ASTeC NuFact06 Summer School August 20-21, 2006.
J-PARC Accelerators Masahito Tomizawa KEK Acc. Lab. Outline, Status, Schedule of J-PARC accelerator MR Beam Power Upgrade.
June 23, 2005R. Garoby Introduction SPL+PDAC example Elements of comparison Linacs / Synchrotrons LINAC-BASED PROTON DRIVER.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, A.Drozhdin, N.Kazarinov.
1 FFAG Role as Muon Accelerators Shinji Machida ASTeC/STFC/RAL 15 November, /machida/doc/othertalks/machida_ pdf/machida/doc/othertalks/machida_ pdf.
1 Proposal for a CESR Damping Ring Test Facility M. Palmer & D.Rubin November 8, 2005.
Electron Model for a 3-10 GeV, NFFAG Proton Driver G H Rees, RAL.
Lecture 25 - E. Wilson - 12/15/ Slide 1 Lecture 6 ACCELERATOR PHYSICS HT E. J. N. Wilson
BEAM TRANSFER CHANNELS, BEAM TRANSFER CHANNELS, INJECTION AND EXTRACTION SYSTEMS OF NICA ACCELERATOR COMPLEX Tuzikov A., JINR, Dubna, Russia.
Module 5 A quick overview of beam dynamics in linear accelerators
1 EMMA Tracking Studies Shinji Machida ASTeC/CCLRC/RAL 4 January, ffag/machida_ ppt & pdf.
Adams Accelerator Institute 10 - E. Wilson - 1/24/ Slide 1 Lecture 14 ACCELERATOR PHYSICS MT 2004 E. J. N. Wilson.
H. Bartosik, Y. Papaphilippou. PS2 meant as potential replacement of existing PS PS2 main characteristics given by LHC requirements – Circumference defined.
Fermilab and Muons Proton Driver (for ν-Factory, μ + -μ - Collider, …) David Neuffer Fermilab.
Lecture 7 - E. Wilson - 2/16/ Slide 1 Lecture 7 - Circulating Beams and Imperfections ACCELERATOR PHYSICS MT 2009 E. J. N. Wilson.
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.
Zeuten 2 - E. Wilson - 2/26/ Slide 1 Transverse Dynamics – E. Wilson – CERN – 16 th September 2003  The lattice calculated  Solution of Hill 
The Introduction to CSNS Accelerators Oct. 5, 2010 Sheng Wang AP group, Accelerator Centre,IHEP, CAS.
FFAG’ J. Pasternak, IC London/RAL Proton acceleration using FFAGs J. Pasternak, Imperial College, London / RAL.
NuFACT06 Muon Source at Fermilab David Neuffer Fermilab.
Operated by the Southeastern Universities Research Association for the U.S. Depart. Of Energy Thomas Jefferson National Accelerator Facility Alex Bogacz,
RCS design Valeri Lebedev AAC Meeting November 16-17, 2009.
Accumulator & Compressor Rings with Flexible Momentum Compaction arccells MAP 2014 Spring Meeting, Fermilab, May 27-31, 2014 Y. Alexahin (FNAL APC)
Operated by the Southeastern Universities Research Association for the U.S. Depart. Of Energy Thomas Jefferson National Accelerator Facility Alex Bogacz,
Longitudinal aspects on injection and acceleration for HP-PS Antoine LACHAIZE On behalf of the HP-PS design team.
Update on RF parameters A.Lachaize11 th HPPS design meeting04/09/13.
HP-PS beam acceleration and machine circumference A.LachaizeLAGUNA-LBNO General meeting Paris 18/09/13 On behalf of HP-PS design team.
Lecture 5 - E. Wilson - 6/29/ Slide 1 Lecture 5 ACCELERATOR PHYSICS MT 2014 E. J. N. Wilson.
FFAG Studies at BNL Alessandro G. Ruggiero Brookhaven National Laboratory FFAG’06 - KURRI, Osaka, Japan - November 6-10, 2006.
Lecture 8 - Circulating Beams and Imperfections
Off-axis injection lattice design studies of HEPS storage ring
Towards a Common Proton Driver for a Neutrino Factory
J-PARC main ring lattice An overview
A.Lachaize CNRS/IN2P3 IPN Orsay
Large Booster and Collider Ring
Jeffrey Eldred, Sasha Valishev
Multiturn extraction for PS2
Progress activities in short bunch compressors
FFAG Accelerator Proton Driver for Neutrino Factory
Lecture 6 ACCELERATOR PHYSICS MT 2011 E. J. N. Wilson.
Progress towards Pulsed Multi-MW CERN Proton Drivers
CEPC Injector Damping Ring
Lecture 6 ACCELERATOR PHYSICS MT 2015 E. J. N. Wilson.
LHC (SSC) Byung Yunn CASA.
Lecture 7 - Circulating Beams and Imperfections
A Design Study of a Compressor ring for
Negative Momentum Compaction lattice options for PS2
Lecture 6 ACCELERATOR PHYSICS HT E. J. N. Wilson
Kicker and RF systems for Damping Rings
Negative Momentum Compaction lattice options for PS2
3.2 km FODO lattice for 10 Hz operation (DMC4)
Presentation transcript:

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 1 COURSE SUMMARY A Design Study of a Compressor ring for A Neutrino Factory MT 2009 E. J. N. Wilson LECTURE 17

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 2 Putting “it” together  The SPS Design Committee get down to business (1971)

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 3 SPL

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 4 SPL Output Parameters – for the neutrino factory Ion speciesH-H- Kinetic energy5GeV Mean current during the pulse40mA Mean beam power4MW Pulse repetition rate50Hz Pulse duration0.4ms Bunch frequency352.2MHz Duty cycle during the pulse62 (5/8)% rms transverse emittances0.4  mm mrad Longitudinal rms emittance0.3  deg MeV Length535m

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 5 Neutrino Factory Demands ParameterBasic valueRange Beam energy [GeV] Burst repetition rate [Hz]50? Number of bunches per burst (n)41 – 6 ? Total duration of the burst [  s] ~ Time interval between bunches [  s] (t int ) 16~ 50/(n-1) Bunch length [ns] Specifications (from R. Palmer’s conclusion at ISS meeting in RAL on Thursday 27, April 2006)

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 6 Accumulate and Compress Scenario

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 7 Space charge Q shift  Radial force equals rate of change of momentum

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 8 Smooth approx. - choosing No. of periods

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 9 Period geometry  Everything must add up for the ring

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 10 Phase advance per cell  The beta at the F quadrupole which defines the scale of the apertures goes through a minimum at about 70 deg/cell.  Other considerations which might lead to close to 90 degrees per cell are »Sensitivity to closed orbit errors »Ease of locating correctors »Schemes for correcting the chromaticity in the arcs without exciting resonances

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 11

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 12 Basic Cell of the C0mpressor

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 13 Insertion for 3 Bunch Compressor

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 14 Compressor Lattice  Your Christmas Present!

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 15 Correction of chromaticity  Parabolic field of a 6 pole is really a gradient which rises linearly with x  If x is the product of momentum error and dispersion  The effect of all this extra focusing cancels chromaticity  Because gradient is opposite in v plane we must have two sets of opposite polarity at F and D quads where betas are different

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 16 Parameters of the Magnets of the Compressor

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 17 Magnet design

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 18 Various coil and yoke designs  ''C' Core: Easy access Less rigid  ‘H core’: Symmetric; More rigid; Access problems.  ''Window Frame' High quality field; Major access problems Insulation thickness

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 19 RF Cavity  constraint is Voltage per meter and MW of power (Shunt impedance and Q)  pressure from need to provide a good acceleration rate or large bucket (e.g. for bunch rotation)

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 20 Rf frequency (injection)  At injection, in order to use the Keil Schnell criterion to combat instabilites we must have enough voltage to reach a threshold value of :

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 21 Rf frequency(in collision))  When colliding bunches, we want a short bunch either: or:  If h is small, the bucket area must be much bigger  Hence  But check synchrotron wave number < 0.1

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 22  This is a biased rigid pendulum  For small amplitudes  Synchrotron frequency  Synchrotron “tune” Synchrotron motion (continued)

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 23

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 24 The bunch and bucket at start of rotation

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 25 Intensity and impedance  Local enlargement in the beam tube which can resonate like a cavity  Voltage experienced has same form as the current which excites it  Impedance  Relates force on particles to the Fourier component of the beam current which excites the force.  A complex quantity - REAL if the voltage and current are in phase - IMAGINARY if 90 degrees or "i" between voltage and current (L = +, C = –) - different from r.f. wave by 90 degrees!

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 26 Instability  Keil Schnell stability criterion:

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 27 Some parameters of accumulator and compressor Table 6: Main parameters of the accumulator and compressor for a neutrino factory RingParameter6 bunches case Accumulato r Circumference [m]318.5 Nb. of accumulation turns400 Type of magnetsNC CompressorCircumference [m]314.2 Nb. of compression turns36 RF voltage on h=3 (MV]4 Transition gamma2.3 Type of magnetsSC Interval between bunches [  s] 12

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 28 LHC parameters

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 29 ORGANISATION OF DESIGN A. Lattice Working Group Rossbach,J. and Schmüser, P. (1992). Basic course on accelerator optics. Proceedings of the 1986 CERN Accelerator School, Jycaskyla, Finland, CERN Choose a lattice 3. Decide phase advance per cell 4. Calculate beta max and min 5. Decide period geometry 6. Calculate beta max and min 7. Calculate dispersion 8. Calculate transition energy B. Errors and corrections 9. Identify sources of orbit distortion 10. Correction of chromaticity 11. Effect of errors 12. Identify sources of orbit distortion 13. Acceptance required C. Magnet and power supply The magnet aperture - the most expensive component 15. Calculating magnet stored energy 16. Resonant power supply design D. RF RF Cavity tuning (frequency swing) 18. Choice of RF frequency (scaling) 19. Choice of RF voltage (injection) 20. Bucket size for capture and acceleration E. Collective effects 21. Instability thresholds 1. Keep a parameter list

Lecture17(Course Summary).PPT - E. Wilson - 3/3/ Slide 30 THE “MOMENT OF TRUTH”  Adams, waiting for the first beam in the SPS, asks his team if they have remembered everything.