Implications of HOMs on Beam Dynamics at ESS

Slides:



Advertisements
Similar presentations
Tom Powers Practical Aspects of SRF Cavity Testing and Operations SRF Workshop 2011 Tutorial Session.
Advertisements

ESS End-to-End Optics and Layout Integration Håkan Danared European Spallation Source Catania, 6 July 2011.
ESS SPOKE LINAC (WP4) Sebastien BOUSSON Guillaume OLRY ESS/SPL Meeting - Lund – 2010/07/01.
Experience with Bunch Shape Monitors at SNS A. Aleksandrov Spallation Neutron Source, Oak Ridge, USA.
Roger Ruber, Volker Ziemann, Gergana Hamberg Uppsala University
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,
 An h=4 (30 MHz) RF system will be used for electron operation. For protons, this would correspond to h=56, and the 1 kV maximum gap voltage would only.
SCRF Activities at IPN Orsay Sébastien Bousson On behalf of the SCRF group Eurisol Net Meeting – CERN, 28 th June 2011.
Progress of SRF and ERL at Peking University Lu Xiangyang Institute of Heavy Ion Physics Peking University.
SRF Results and Requirements Internal MLC Review Matthias Liepe1.
Introduction and Charge to the Review of ESS Target building and Instrument Hall design requirements Roland Garoby November 2014, Lund
Preliminary design of SPPC RF system Jianping DAI 2015/09/11 The CEPC-SppC Study Group Meeting, Sept. 11~12, IHEP.
Activities of Superconducting RF Accelerators at Nanjing University Sun An Proton Linear Accelerator Institute Institute of Energy Sciences, Nanjing University.
Dave McGinnis Chief Engineer – Accelerator Division
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.
704MHz Warm RF Cavity for LEReC Binping Xiao Collider-Accelerator Department, BNL July 8, 2015 LEReC Warm Cavity Review Meeting  July 8, 2015.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, A.Drozhdin, N.Kazarinov.
SINGLE-STAGE BUNCH COMPRESSOR FOR ILC-SB2009 Nikolay Solyak Fermilab GDE Baseline Assessment Workshop (BAW-2) SLAC, Jan , 2011 N.Solyak, Single-stage.
HWDB: Operations at the Spallation Neutron Source Workshop on Accelerator Operations August 6-10, 2012 Glen D. Johns Accelerator Operations Manager.
ESS Medium Beta Cavity Prototypes Manufacturing HALF CELLS RESULTS SUMMARY Six medium beta cavities will be manufactured for the Elliptical Cavities Cryomodule.
Preliminary Functional Analysis of ESS Superconducting Radio-Frequency Linac C. Darve, N. Elias, J. Fydrych, D. Piso European Spallation Source ESS AB,
Beam Dynamics in the ESS Linac Under the Influence of Monopole and Dipole HOMs A.Farricker 1, R.M.Jones 1, R.Ainsworth 2 and S.Molloy 3 1 The University.
Design Optimization of MEIC Ion Linac & Pre-Booster B. Mustapha, Z. Conway, B. Erdelyi and P. Ostroumov ANL & NIU MEIC Collaboration Meeting JLab, October.
Aaron Farricker 107/07/2014Aaron Farricker Beam Dynamics in the ESS Linac Under the Influence of Monopole and Dipole HOMs.
Longitudinal HOM damping estimations for SPL cavity. status W. Weingarten 26 July 20101SPL Cavity WG Meeting.
Sensitivity of HOM Frequency in the ESS Medium Beta Cavity Aaron Farricker.
Longitudinal HOM power estimations for pulsed beams.rev W. Weingarten 31 May 20101SPL Cavity WG Meeting.
Comparison of Fermilab Proton Driver to Suggested Energy Amplifier Linac Bob Webber April 13, 2007.
The Introduction to CSNS Accelerators Oct. 5, 2010 Sheng Wang AP group, Accelerator Centre,IHEP, CAS.
Marcel Schuh CERN-BE-RF-LR CH-1211 Genève 23, Switzerland 3rd SPL Collaboration Meeting at CERN on November 11-13, 2009 Higher.
The Superconducting cavities of the European Spallation Source Superconducting Technologies Workshop CERN – 4 & 5 December 2012 Sébastien Bousson (CNRS/IN2P3/IPN.
Status of the 1.2 MW MB-IOT for ESS Morten Jensen CLIC Workshop 2016, January, CERN.
ESS AD RETREAT 5 th December 2011, Lund “A walk down the Linac” SPOKES Sébastien Bousson IPN Orsay.
HOMSC Fermilab HOM Couplers for CERN SPL Cavities K. Papke, F. Gerick, U. van Rienen 1 Work supported by the Wolfgang-Gentner-Programme.
SRF COLLABORATION MEETING MAY.2016 ESS MEDIUM BETA CAVITY MANUFACTURING CEA Saclay/ESS ECCTD WU Cavités | Enrico Cenni.
1 Project X Workshop November 21-22, 2008 Richard York Chris Compton Walter Hartung Xiaoyu Wu Michigan State University.
Group Meeting October 15 th 2012 Lee Carver. Outline Multi-Harmonic Cavity (MHC) Design Project - Cavity Designs, Couplers, HOM analysis Electron Two.
Aaron Farricker 107/07/2014Aaron Farricker Beam Dynamics in the ESS Linac Under the Influence of Monopole and Dipole HOMs.
Spoke section of the ESS linac: - the Spoke cryomodules - the cryogenic distribution system P. DUTHIL (CNRS-IN2P3 IPN Orsay / Division Accélérateurs) on.
MEW Meeting 05/06/14 Aaron Farricker 1. Effect Of HOMs Near Machine lines HOMs on or near machine lines get resonantly excited. Modes in real cavities.
ESS SC cavities development G. Devanz TTC meeting, march 1st 2011, Milano.
A CW Linac scheme for CLIC drive beam acceleration. Hao Zha, Alexej Grudiev 07/06/2016.
MEW Meeting 28/05/15 Aaron Farricker. Outline Wakefield ahead of a bunch Wakefield in CST comparison of Eigenmode and Wakefield solvers.
HOMs in high-energy part of the Project-X linac. V. Yakovlev, N. Solyak, J.-F. Ostiguy Friday 26 June 2009.
WP5 Elliptical cavities
Bocheng Jiang SSRF AP group
Physics design on the main linac
Overview and System Design for ESS LLRF Systems
Andrei Shishlo ORNL SNS Project Florence, Italy November 2015
Higher Order Modes and Beam Dynamics at ESS
WG-1 Session Cavity Performance Cryomodule Performance
Physics design on Injector-1 RFQ
HOM power in FCC-ee cavities
Tunable Electron Bunch Train Generation at Tsinghua University
SC spoke cavity for China-ADS 3~10MeV injector
1- Short pulse neutron source
Update of CLIC accelerating structure design
Optimum cryomodule length at the ESS
CEPC RF Power Sources System
ERL Main-Linac Cryomodule
Overview Multi Bunch Beam Dynamics at XFEL
Status of HOMS Spectra Measurements in 1.3 GHz Cavities for LCLS-II
SPS-DQW HOM Measurements
Physics Design on Injector I
CEPC SRF Parameters (100 km Main Ring)
ACCSYS Collaboration Board Triestre, 3rd october 2017
Roger Ruber for the FREIA team 11 June 2013, Uppsala
Update on Crab Cavity Simulations for JLEIC
RF system for MEIC Ion Linac: SRF and Warm Options
eSPS Impedance Considerations Aaron Farricker Acknowledgements: T
Presentation transcript:

Implications of HOMs on Beam Dynamics at ESS Aaron Farricker Aaron Farricker

Outline The European Spallation Source The ESS Cavities and Mode Spectra Impact of HOMs on the Beam Methods of HOM Mitigation The Wakefield From a Non-Relativistic Charge Aaron Farricker

The European Spallation Source (ESS) The ESS is a spallation neutron facility being build in Lund, Sweden. The ESS collaboration consists of 19 countries from Europe The facility consists of a superconducting proton linac which will collide a proton beam with a Solid target to produce neutron which will be directed into several experimental halls Major Beam Parameters Pulse Length (ms) 2.86 Energy (GeV) 2 Peak Current (mA) 62.5 Pulse Rep. Rate (Hz) 14 Average Power (MW) 5 Peak Power (MW) 125 Aaron Farricker

The ESS Linac Beta=0.5 Spoke Cavities # of CryoModules 13 Warm Section Cold Section (2K SCRF) Beta=0.5 Spoke Cavities # of CryoModules 13 # of Cavities 26 Eacc (MV/m) 9 Frequency (MHz) 352.21 Beta=0.67 Elliptical Cavities # of CryoModules 9 # of Cavities 36 Eacc (MV/m) 16.7 Frequency (MHz) 704.42 Beta=0.86 Elliptical Cavities # of CryoModules 21 # of Cavities 84 Eacc (MV/m) 19.9 Frequency (MHz) 704.42 Aaron Farricker

Cavity Mode Spectra High Beta In both cavities the accelerating mode is the one with the highest R/Q by more than an order of magnitude All other modes have relatively low R/Q and it has been shown they are of little concern However if a mode shifts onto a harmonic of the bunch frequency a resonant growth in the HOM voltage will occur As a result of this ESS requires all HOMs are at least 5 MHz from any machine resonance In all the designs a10 MHZ gap is found HOMs of Concern Accelerating Mode Machine Harmonic Medium Beta Aaron Farricker

What Happens During Manufacturing CEA Saclay have produced 2 prototypes which meet all requirements for the accelerating mode but not for the HOMs (TUPB007 SRF’15 Peauger et al.) The ESS cavities will be manufactured from high purity niobium (RRR>250) The process shaping the half cells will be carried out using the deep drawing process Then half cells and end groups will be welded together The structure is then mechanically stretched to tune the accelerating mode frequency and field shape All of these processes introduce errors onto the original geometry and can shift HOM frequencies As a result of this CEA asked for the ESS requirement to be looked at in detail. Cavity ID P01 P02 Design Frequency at 300 K Measured 1418.178 1402.254 1407.848 1418.674 1404.666 1408.258 Voltage Build Up as a function of Mode Frequency Aaron Farricker

Implications on the Beam Impact of a single HOM lying on a Machine Resonance Beam dynamics simulations following a drift-kick-drift scheme have been used These simulations have indicated that even a single cavity can have a drastic impact on the beam (right) As a result there is some limit which must be applied The big question is whether the 5 MHz limit imposed by ESS is too strict or not To ascertain this many simulations are required as the HOM frequency spread is random (hopefully) Medium Beta Q=108 Q=106 High Beta Q=108 Q=106 Aaron Farricker

Is a HOM Frequency limit Needed? Medium Beta Clearly resonantly excited HOMs can have a significant impact on the beam (slide 7) As a result of ESS not using HOM couplers a limit of at least 5 MHz separation is required However this has proved problematic (slide 6) The real question is 5 MHz adequate or too strict? A reduction in this limit would make manufacturing much easier but at what cost to machine performance On the right the Impact of randomly generated HOM frequencies following a 2 MHz wide uniform distribution is shown as a function of the central frequency difference from the machine resonance (mean of 1,000 simulations per point) The transition between growth and no growth is less than 100 kHz wide Q=108 Q=106 High Beta Q=108 Q=106 Aaron Farricker

The Wakefield The wakefield for a beam of beta=1 is well understood The wakefield is readily decomposed into a series of modes over which a sum can be taken (Condon Method) This can be analytically for a closed pillbox Comparison of the Wakefield from simulation (red) and the analytic form (blue) Aaron Farricker

Beta<1 Beta=0.9 wakefield on axis Red from simulation Blue analytic When beat<1 fields from the bunch can exist ahead and behind the charge This means that a wakefield could be present ahead of the exciting bunch Attempts are being made to reconcile the analytic form at beta<1 with simulations The primary method considered is to integrate the wakefield off axis to remove the static component from space charge Work on this is ongoing and much improvement has been seen Beta=0.9 wakefield off axis Aaron Farricker