1 CERN 1 Mar. 2007 E-CLOUD Build-up in Grooved Chambers Marco Venturini Center for Beam Physics, LBNL ECL2 -- CERN, 1-2 March 2007.

Slides:



Advertisements
Similar presentations
PyECLOUD G. Iadarola, G. Rumolo Thanks to: F. Zimmermann, G. Arduini, H. Bartosik, C. Bhat, O. Dominguez, M. Driss Mensi, E. Metral, M. Taborelli.
Advertisements

Heat load due to e-cloud in the HL-LHC triplets G. Iadarola, G. Rumolo 19th HiLumi WP2 Task Leader Meeting - 18 October 2013 Many thanks to: H.Bartosik,
9-12 April 2007 International Linear Collider DR electron cloud R&D effort: Clearing electrode and triangular fin M. Pivi T. Raubenheimer, J. Seeman, T.
BUILD-UP SIMULATIONS FOR DAFNE WIGGLER W/ ELECTRODES Theo Demma.
KEK Recent results of beam tests on clearing electrode and grooves 2010/1/191ILC DR WebEx Meeting Y. Suetsugu, KEK.
Electron-cloud instability in the CLIC damping ring for positrons H. Bartosik, G. Iadarola, Y. Papaphilippou, G. Rumolo TWIICE workshop, TWIICE.
Damping ring K. Ohmi LC Layout Single tunnel Circumference 6.7 km Energy 5 GeV 2 km 35 km.
How e-cloud effect affects the ILC DR Vacuum System Dr. Oleg B. Malyshev ASTeC Daresbury Laboratory.
Latest ILC DR wiggler simulations M. Pivi, T. Raubenheimer, L. Wang (SLAC) July, 2005.
E-Cloud Effects in the Proposed CERN PS2 Synchrotron M. Venturini, M. Furman, and J-L Vay (LBNL) ECLOUD10 Workshshop, Oct Cornell University Work.
SuperB and the ILC Damping Rings Andy Wolski University of Liverpool/Cockcroft Institute 27 April, 2006.
ECLOUD Calculations of Field Gradients During Bunch Passage Jim Crittenden Cornell Laboratory for Accelerator-Based Sciences and Education Electron Cloud.
45 th ICFA Beam Dynamic Workshop June 8–12, 2009, Cornell University, Ithaca New York Modelling Cyclotron Resonances in ECLOUD 1) Comparison with CesrTA.
First approach to the SuperB Rings M. Biagini, LNF-INFN April 26th, 2006 UK SuperB Meeting, Daresbury.
ECLOUD Calculations of Coherent Tune Shifts for the April 2007 Measurements - Study of SEY Model Effects - Jim Crittenden Cornell Laboratory for Accelerator-Based.
LEPP, the Cornell University Laboratory for Elementary-Particle Physics, has joined with CHESS to become the Cornell Laboratory for Accelerator-based Sciences.
Electron Cloud in ilcDR: Update T. Demma, INFN-LNF.
45 th ICFA Beam Dynamic Workshop June 8–12, 2009, Cornell University, Ithaca New York Modeling Cyclotron Resonances in ECLOUD Jim Crittenden Cornell Laboratory.
Tagger and Vacuum Chamber Design. Outline. Design considerations. Stresses and deformations. Mechanical assembly.
45 th ICFA Beam Dynamic Workshop June 8–12, 2009, Cornell University, Ithaca New York Recent Studies with ECLOUD Jim Crittenden Cornell Laboratory for.
ElectronsdFud Simulation Work at Cornell Jim Crittenden Cornell Laboratory for Accelerator-Based Sciences and Education.
Introduction Status of SC simulations at CERN
Electron Clouds at SLAC Johnny Ng ILC Damping Rings Collaboration Meeting March 4, 2009.
Electron Cloud Simulations Using ORBIT Code - Cold Proton Bunch model April 11, 2007 ECLOUD07 Yoichi Sato, Nishina Center, RIKEN 1 Y. Sato ECLOUD07.
Electron Cloud Studies for Tevatron and Main Injector Xiaolong Zhang AD/Tevatron, Fermilab.
1 Electron Cloud Cyclotron Resonances for Short Bunches in a Magnetic Field * C. M. Celata a, Miguel A. Furman, J.-L. Vay, and Jennifer W. Yu b Lawrence.
SPS scrubbing experience: electron cloud observables L. Mether on behalf of the LIU-SPS e-cloud team LIU SPS scrubbing review, September 8, 2015.
Webex Electron Cloud Evaluations for ILC DR Mauro Pivi on behalf of the ILC Electron Cloud Working Group - by Webex - KILC12 – Daegu Korea April 25, 2012.
ILC damping ring Workshop, Dec 19, 2007, KEK, L. WANG Ecloud simulation 2007 ILC Damping Rings Mini-Workshop December, 2007 Lanfa Wang, SLAC.
ILC08 Chicago November 2008 Summary of Recent Results from SLAC M. Pivi, J. Ng, D. Arnett, G. Collet, T. Markiewicz, D. Kharakh, R. Kirby, F. Cooper,
March 23, 2010 CMAD a tracking and e-cloud beam instability parallel code (M.Pivi SLAC) Taking MAD(X) optics file at input, thus tracking the beam in a.
Electron cloud in the wigglers of ILC Damping Rings L. Wang SLAC ILC Damping Rings R&D Workshop - ILCDR06 September 26-28, 2006 Cornell University.
FCC electron cloud study plan K. Ohmi (KEK) Mar FCC electron cloud study meeting CERN.
Electron Model for a 3-10 GeV, NFFAG Proton Driver G H Rees, RAL.
Physics of electron cloud build up Principle of the multi-bunch multipacting. No need to be on resonance, wide ranges of parameters allow for the electron.
Compare options: simulations recent history Cloud density near (r=1mm) beam (m -3 ) before bunch passage, values are taken at a cloud equilibrium density.
Compare options: simulations recent history Cloud density near (r=1mm) beam (m -3 ) before bunch passage, values are taken at a cloud equilibrium density.
Midwest Accelerator Physics Meeting. Indiana University, March 15-19, ORBIT Electron Cloud Model Andrei Shishlo, Yoichi Sato, Slava Danilov, Jeff.
EMMA: Pulsed magnets Kiril Marinov MaRS group, ASTeC, Daresbury Laboratory 1.
IPM EM Simulations 9 th DITANET Topical Workshop on Non-Invasive Beam Size Measurement for High Brightness Proton and Heavy Ion Accelerators April.
CERN, LIU-SPS ZS Review, 20/02/ Brief review on electron cloud simulations for the SPS electrostatic septum (ZS) G. Rumolo and G. Iadarola in LIU-SPS.
Cesr-TA Simulations: Overview and Status G. Dugan, Cornell University LCWS-08.
Nov 17, 2009 Webex Assessing the 3.2 km Ring feasibility: Simulation parameters for electron cloud Build-up and Instability estimation LC DR Electron Cloud.
Progress on electron cloud studies for HL-LHC A. Axford, G. Iadarola, A. Romano, G. Rumolo Acknowledgments: R. de Maria, R. Tomás HL-LHC WP2 Task Leader.
3 rd INSTALLATION: chicane magnetic field tests PEP-II e+ ring 1 st and 2 nd Feb 2008 Electron cloud installation studies at SLAC ILC tests - SLAC Cherrill.
Electron cloud in Final Doublet IRENG07) ILC Interaction Region Engineering Design Workshop (IRENG07) September 17-21, 2007, SLAC Lanfa Wang.
FCC-hh: First simulations of electron cloud build-up L. Mether, G. Iadarola, G. Rumolo FCC Design meeting.
Electron Cloud Studies Theo Demma INFN-LNF Frascati.
E-cloud Remedies and PS2 vacuum design J.M. Jimenez AT Department – Vacuum Group CARE-HHH-APD BEAM’07 Thursday 04 October Session 2: PS2 E-cloud.
RFA Simulations Joe Calvey LEPP, Cornell University 6/25/09.
R&D GOALS AND MILESTONES TOWARDS A TECHNICAL DESIGN REPORT TDR (2008) First Intnl. Teleconference Ecloud, Impedance/Instabilities - M. Pivi, SLAC 31 October.
LARP CM12, 9 April 2009M. Furman: PS2 ecloud p. 1 PS2 Electron-Cloud Build-Up Studies: Status LARP CM12, Napa, CA, 9 April 2009 Miguel A. Furman LBNL.
3 February 2010 ILC Damping Ring electron cloud WG effort Mauro Pivi SLAC on behalf of ILC DR working group on e- cloud ILC DR Webex Meeting Jan 3, 2010.
Electron cloud measurements in Cesr-TA during the July-August run for the SPSU Study Team, report by S. Calatroni and G. Rumolo thanks to J.
Tagger and Vacuum Chamber Design Jim Kellie Glasgow University.
International Linear Collider R&D on electron cloud (SLAC)
Update to ECLOUD Calculations for the
Impedance & SEY of grooved surface
Impedance & SEY of grooved Surface Ecloud in Quadpole
Ecloud in quadrupole & Sextupole
J.A.Crittenden, Y.Li, X.Liu, M.A.Palmer, J.P.Sikora (Cornell)
Jim Crittenden Electron Cloud/Impedance Meeting 27 May 2015
Electron Cloud in ilcDR: Update
SuperB General Meeting June , Perugia (Italy)
Status of Ecloud Build-Up Simulations for the ILC DR’s
Impedance of grooved surface
ILC Damping Ring electron cloud WG effort
Electron Cloud in ilcDR: Update
Electron Cloud Build-up in ilcDR
R&D GOALS AND MILESTONES TOWARDS A TECHNICAL DESIGN REPORT TDR (2008)
Presentation transcript:

1 CERN 1 Mar E-CLOUD Build-up in Grooved Chambers Marco Venturini Center for Beam Physics, LBNL ECL2 -- CERN, 1-2 March 2007

2 CERN 1 Mar Outline of work ãAugment existing version of POSINST to model e-cloud build-up in the presence of grooved walls —Electron orbits are properly followed and collisions located on the groove surface where they occur but … —… when solving the Poisson equation for the electron self-field the boundaries are those of the smooth chamber (field enhancement at the groove edges not accounted) ãFeatures implemented so far: —Rectangular chamber cross section —Grooves are placed on top and bottom of wall —(Isosceles) triangular grooves with option to account for rounded tips ãMotivations: —Characterization of e-cloud dynamics more from ‘first principles’ instead of passing through an intermediate calculation of an ‘effective’ secondary yield for the grooved wall. —Validate previous calculations by M.Pivi, G. Stupakov, and L.Wang. —Help settle some alleged disagreement with other calculations —Provide modeling tools for ongoing and future measurements

3 CERN 1 Mar Calculations done so far: ãParameter choice specific for the ILC-DR dipoles. —Input deck for POSINST provided by M.Pivi with setting used for previous smooth-chamber DR simulations ãExploration of dependence of e-cloud build up on: —Groove angle and height —Radius of the rounded groove tips —Magnitude of magnetic field ãContact with previous calculations by extracting and effective SEY ( by comparison with e-cloud build-up curves for smooth chambers )

4 CERN 1 Mar ILC DR basic parameters used in simulations ãChamber sizes: 2.3*2.3 cm (rectangular)  Max SEY (for smooth surface)  = 1.75 ãMax. no. of macro-e = 20K found to be adequate (i.e. get small noise in longitudinal e-density) Dipole magnetic field0.194 T Beam sizes in bends  x =0.62 mm,  y =8  m,  z =6mm Particle/bunchN=2*10 10 RF bucket spacing1.52 ns (=0.46m) [ f RF =650 MHz, C=6.11Km] Bunch spacing6.1 ns (one every four RF buckets) No. bunches/train111 Train length 0.68  s (=204m) Bunch-train structure parameters: Beam/dipole parameters:

5 CERN 1 Mar Geometry of triangular grooves  Geometry of triangular grooves is defined by angle  and height h g   =0 o == flat surface Snapshot of macro-electron distribution in chamber w/ grooves

6 CERN 1 Mar E-cloud dependence on groove angle  E-cloud density suppressed by a factor ~200 for groove angles  >75 o E-cloud build-up during bunch-train passage for various  Max e-cloud density during bunch-train passage vs. 

7 CERN 1 Mar Extract an effective SEY from comparison with data from smooth chamber  The effective SEY for surface with groove angle  is defined as the SEY of a smooth chamber that results in the same max of e-cloud accumulation E-cloud build-up during bunch-train passage for smooth walls, various max SEY  critical angle  ~75 o critical angle  ~75 o Effective SEY  for various groove angles Shallow grooves increase yield!

8 CERN 1 Mar A higher B-field degrades e-cloud suppression E-cloud build-up during bunch-train passage for various B Max e-cloud density vs. B for fixed groove geometry ãA larger cyclotron radius (smaller B-field) enhances chance that secondary electrons may be promptly reabsorbed in wall collision B=0.2T (dipoles) B=0.2T (dipoles) B=1.6T (wiggler) B=1.6T (wiggler)

9 CERN 1 Mar Dependence on groove height ãDependence appears to be generally mild over a large span of height variations Max of e-cloud density vs. height h g for two groove angles Max of e-cloud density vs. groove angle  for three groove heights h g

10 CERN 1 Mar Triangular grooves with smooth tips  Geometry of triangular grooves is defined by angle , height h g, and tip radius r g ãSmoothing groove tips may be desirable to ease impedance, manufacturing WALL INNER CHAMBER In present model only the groove edges on the chamber inner side are smoothened In present model only the groove edges on the chamber inner side are smoothened

11 CERN 1 Mar Smoother tips spoil effectiveness of grooves ãFinite groove-tip radius enhances dependence of groove effectiveness on groove height Max of cloud density vs. groove-tip radius for two groove height h g Max of cloud density vs. height h g for 3 choices of groove-tip radius ãSpoiling effect of smooth groove-tips can be compensated by making the grooves deeper.

12 CERN 1 Mar Conclusions  Isosceles triangular grooves with steepness angle  >75 o reduce effective SEY to < 1 —E-cloud build up for a 111 bunch train is reduced by a factor 200.  Results seem about consistent with previous calculations by L.Wang (  ~70 o for effective SEY < 1, SLAC-PUB ) ãA larger magnetic field makes the grooving less effective. —In wigglers the groove angle likely to have to be steeper to provide same e-cloud suppression effect as in dipoles ãRounding of the tips spoils e-cloud suppression, which can be compensated by deepening the grooves