Frequency tuning, space charge compensation and hollow beam structure

Slides:



Advertisements
Similar presentations
UV FUNDAMENTALS. F Ultraviolet is… u A Type of Electromagnetic Energy u Found Between X-Rays and Visible Light u Wavelength Range: 5 nm to 400 nm Rays.
Advertisements

Wireless LAN RF Principles
Producing an X-ray Exposure
McGraw-Hill/Irwin Copyright © 2006 by The McGraw-Hill Companies, Inc. All rights reserved. Chapter 4 Future Value, Present Value and Interest Rates.
A typical case of SD structure at high spin in 194Hg! sig_tot = 1barn Atarget = 186, thikness = 0.5mg/cm 2 beam intensity = 5pnA, N = which.
Year 6 mental test 15 second questions Numbers and number system Numbers and the number system, Measures and Shape.
Low Alpha & CSR in the MLS (PTB) G. Wüstefeld (BESSY) et al, ESLS XVI, Daresbury, Nov 28th Low Alpha Optics and Coherent Synchrotron Radiation.
Stefan Hild, Andreas Freise University of Birmingham Roland Schilling, Jerome Degallaix AEI Hannover January 2008, Virgo week, Pisa Advanced Virgo: Wedges.
TURKEY AWOS TRAINING 1.0 / ALANYA 2005 MEASUREMENT OF VISIBILITY.
Plasma Window Options and Opportunities for Inertial Fusion Applications Leslie Bromberg Ady Herskovitch* MIT Plasma Science and Fusion Center ARIES meeting.
RFQ development for high power beams
Chapter3 Pulse-Echo Ultrasound Instrumentation
Study on the Injection System for Compact Cyclotron Mass Spectrometry Do Gyun Kim, Joonyeon Kim, H. C. Bhang Department of Physics, Seoul National University.
Development of the FLNR Cyclotron Complex /2009 Priority 1 Dubna,
An introduction to Ultraviolet/Visible Absorption Spectroscopy
Moacir L. Ferreira Jr. July 08, 2011
Stochastic cooling and 56 MHz SRF update for Run-14 W. Fischer 21 January 2014.
Chemistry Chapter Acids and Bases. (Self-Ionization of Water) H 2 O + H 2 O  H 3 O + + OH -  Two water molecules collide to form Hydronium and.
Chapter Six Study Guide.
Electromagnetic Waves G5 - X Rays. Coolidge tube (X-ray tube) K = Hot filament cathode A = Tungsten anode U h = Heater Voltage (e.g. 12V) U a = Accelerating.
Measurements of adiabatic dual rf capture in the SIS 18 O. Chorniy.
Fusion Physics - Energy Boon or Nuclear Gloom? David Schilter and Shivani Sharma.
CARE07, 29 Oct Alexej Grudiev, New CLIC parameters. The new CLIC parameters Alexej Grudiev.
EM Radiation Sources 1. Fundamentals of EM Radiation 2. Light Sources
Plasma Window Performance Leslie Bromberg Katie Maurer Ady Herskovitch* MIT Plasma Science and Fusion Center ARIES meeting Madison, WI April 23, 2002 *Brookhaven.
Super-B Factory Workshop January 19-22, 2004 Beam pipes M. Sullivan 1 Detector Beam Pipe Diameter Discussion M. Sullivan Super-B Factory Workshop Hawaii.
Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.
Diversion of Plasma in Beam Port with a Vertical Magnetic Field D. R. Welch, D. V. Rose, S. S. Yu and W. Sharp Presented at the ARIES Project Meeting April.
HIAT 2009, 9 th June, Venice 1 DESIGN STUDY OF MEDICAL CYCLOTRON SCENT300 Mario Maggiore on behalf of R&D Accelerator team Laboratori Nazionali del Sud.
Ion Beam Cocktail Development and ECR Ion Source Plasma Physics Experiments at JYFL Olli Tarvainen 11th International Conference on Heavy Ion Accelerator.
By Andy Smith G7IZU This PowerPoint presentation will play automatically in a few seconds. v
Giovanni Ciavola I3 EURONS-2 COMPLECS Town Meeting, Sept. 19th, 2007, Helsinki 1 INFN - GSI - GANIL - LPSC - JYFL - KVI CERN - ATOMKI- TSL - NIPNE - IKF-
Carbon Injector for FFAG
Beam ripple minimization: influence of plasma instability.
Conventional Tubes Conventional Device tubes cannot be used for frequencies above 100MHz 1. Interelectrode capacitance 2. Lead Inductance effect 3. Transit.
Design of Stable Power-Recycling Cavities University of Florida 10/05/2005 Volker Quetschke, Guido Mueller.
Parameter sensitivity tests for the baseline variant Konstantin Lotov, Vladimir Minakov, Alexander Sosedkin Budker Institute of Nuclear Physics SB RAS,
December 2007ESF-Workshop, Athens, Greece University of Jyväskylä, Department of Physics ECR ion source for the highly charged, intensive ion beams H.
New Progress of High Current Gasdynamic Ion Source
Limitation of the ECRIS performance by kinetic plasma instabilities O. Tarvainen, T. Kalvas, H. Koivisto, J. Komppula, R. Kronholm, J. Laulainen University.
AAC February 4-6, 2003 Protons on Target Ioanis Kourbanis MI/Beams.
704MHz Warm RF Cavity for LEReC Binping Xiao Collider-Accelerator Department, BNL July 8, 2015 LEReC Warm Cavity Review Meeting  July 8, 2015.
ICIS2015,Aug , 2015, New York, USA Further improvement of RIKEN 28GHz SC-ECRIS for production of highly charged U ion beam T. Nakagawa (RIKEN, Nishina.
ICIS2015 in NY Y.HIGURASHI Y. Higurashi (RIKEN Nishina center) 1.Introduction RIKEN RIBF and RIKEN 28GHz SC-ECRIS 2.Emittance measurements 1.4D.
Haifeng Huang and Kevin K. Lehmann
A mass-purification method for REX beams
Results of the argon beam test at Linac3 D. Küchler BE/ABP/HSL Including feedback from R. Scrivens and M. Bodendorfer.
EFDA EUROPEAN FUSION DEVELOPMENT AGREEMENT Task Force S1 J.Ongena 19th IAEA Fusion Energy Conference, Lyon Towards the realization on JET of an.
Giovanni Ciavola, JRA-07 ISIBHI JRA-07 Ion Sources for Intense Beams of Heavy Ions (ISIBHI) EURONS PCC Meeting, Groningen, Holland, December 2006.
experiences of Ion Source commissioning at CEA Saclay
X-ray absorption spectroscopy (XAS)
Pekka Suominen 2010 CERN Plasma ion sources for radioactive molecular ion beams.
Mitglied der Helmholtz-Gemeinschaft Jörg Wolters, Michael Butzek Focused Cross Flow LBE Target for ESS 4th HPTW, Malmö, 3 May 2011.
Damping of Coupled-bunch Oscillations with Sub-harmonic RF Voltage? 1 H. Damerau LIU-PS Working Group Meeting 4 March 2014.
Large Area Plasma Processing System (LAPPS) R. F. Fernsler, W. M. Manheimer, R. A. Meger, D. P. Murphy, D. Leonhardt, R. E. Pechacek, S. G. Walton and.
#3205 Summary Studying beam instabilities along bunch train 3 observables – INJ-BPM-01 fast bunch electronics – INJ FCUP-01 – Laser pulse power. Laser.
NNP Non Neutral Plasma Physics Group Intense Beam Transport and Space Charge Compensation Strategies Oliver Meusel August th International Conference.
Studies on 2.45 GHz microwave ion sources Abhishek Nag IISER, KOLKATA Presented By: G.O. Rodrigues IUAC, New Delhi Supervised By:
Recent progress of RIKEN 28GHz SC-ECRIS for RIBF T. Nakagawa (RIKEN) 1.Introduction RIKEN Radio isotope factory project 2.RIKEN 28GHz SC-ECRIS Structure(Sc-coils,
CHARACTERIZATION OF MICROWAVE DISCHARGE ION SOURCE FOR HIGH PROTON BEAM PRODUCTION IN CW AND PULSED MODE Rosalba Miracoli Consegna del premio “Francesco.
(Towards a) Luminosity model for LHC and HL-LHC F. Antoniou, M. Hostettler, Y. Papaphilippou, G. Papotti Acknowledgements: Beam-Beam and Luminosity studies.
H. Koivisto, EMILIE workshop, rd March 2016, GANIL, France Research of CB ECRIS plasma with the aid of injected 1+ beam H Koivisto 1, O Tarvainen.
Page The ESS Proton Source & LEBT WP6-WU2 L. Celona Warm Linac meeting, 06 July 2011, INFN-LNS, Catania WU 1 – Management (S. Gammino) WU 2 – Proton Source.
Development of X-band 50MW klystron in BVERI
Space charge studies at the SPS
Machine studies during beam commissioning
Single-frequency operation mode Double-frequency operation mode
Design of Stable Power-Recycling Cavities
November 14, 2008 The meeting on RIKEN AVF Cyclotron Upgrade Progress report on activity plan Sergey Vorozhtsov.
November 7, 2008 The meeting on RIKEN AVF Cyclotron Upgrade Progress report on activity plan Sergey Vorozhtsov.
Presentation transcript:

Frequency tuning, space charge compensation and hollow beam structure H. Koivisto, V. Toivanen, O. Steczkiewicz, L. Celona, O. Tarvainen, T. Ropponen, S. Gammino and G. Ciavola Content: - Frequency tuning vs. intensity - Frequency tuning vs. beam structure variations - Frequency tuning vs. emittance - Frequency tuning vs. calculated modes - Space charge compensation measurements

Frequency tuning: general The frequency of the JYFL 14 GHz ECRIS was scanned between 14.050 - 14.135 GHz (by Rohde & Schwarz signal generator) Forward power of the Klystron was kept constant using internal Automatic Level Control (ALC) feature The first frequency tuning experiments: with mass analyzed beams, with emittance information, with TWTA

Frequency tuning vs. ion beam intensity Measurements with different charge states: general behavior Ar6+: 110 W - no variations in beam current - small variations in drain current - clear variations in reflected power

Ar9+ - small changes in beam current - clear changes in reflected power - local minimum in reflected power => local intensity maxima!

Ar12+: 520 W Conclusion: Effect of frequency tuning increases vigorously as a function of charge state! - Similar variations in reflected power as earlier - strong variations in ion beam intensity!

What causes the intensity variations! Is it because the total power in the plasma chamber fluctuates with the reflected power (Ptot = Pforward - Preflected)? Most probably no: Difference in Ptotal of 3 % (490 W and 505 W) cannot generate the difference of 30 % in Ar12+ intensity (7 µA versus 10 µA) ! Losses not included! Ar12+ 2) Same Ptotal cannot generate stable 10 µA at 14.06 GHz and very unstable 5 µA at 14.08 GHz Changes in mode structure/ plasma-wave coupling?

Frequency tuning versus beam structure variations 14.05 GHz ≈ 110 µA Ar9+ 14.09 GHz ≈ 105 µA 14.108 GHz ≈ 95 µA Intensity variations less than ± 10 % Still clear variations in beam structure, same beam size (same focusing) Mode structure changes?

Frequency tuning + TWTA b) c) 14.070 GHz + 11.56 GHz 14.100 GHz + 11.56 GHz 14.135 GHz + 11.56 GHz Ar8+ In some cases two concentric hollow beams can be seen when double frequency heating is used with the frequency tuning a clear indication that the hollow beam structure can formed also in the plasma a clear indication that the frequency tuning causes changes in plasma

Frequency tuning versus emittance - strong effect on the beam emittance beculiar behavior: usually lowest emittance for high charge states (9+ and higher) in the beginning of frequency scan, for lower charge states in the middle of the scan! More measurements have to be perform to understand the behavior

What is the density of calculated modes (JYFL 14 GHz ECRIS)? Density of calculated modes and density of intensity fluctuations are at the same order => the intensity variations come from changes in mode excitation!?

∆f=f0/Q Q-value estimation with the aid of reflected power Q ≈ 2200 (similar values have been obtained earlier by Catania group) ∆f=f0/Q

Q-value estimation with the aid of intensity variations: Q-value has to be relatively high in order to see any intensity variations! For example: Q = 10 => ∆f = 1.4 GHz , very wide peak! Ar9+ Distance of neighboring peaks ≈ 10 MHz => Q = 1410 Q-value of empty chamber: 20 000 -100 000 Indicates that most of the power is dissipated by the plasma

Space charge compensation effect: preliminary unpublished results! Objective: improvement of space charge compensation gas feeding Gas was fed into the beam line close to the focal points (He, N2, Ar) emittance scanner Faraday cup beam viewer

Space charge compensation effect: preliminary unpublished results! Ar8+, 10 kV, 143 µA, 1.8E-7 mbar Ar8+, 10 kV, 120 µA, 6.2E-6 mbar 277 π mm mrad 140 π mm mrad Indicates that hollow beam structure can be formed also in the beam line Beam size decreases! Clear optimum for brightness is found!

- clear improvement in ion beam transmission efficiency (incl - clear improvement in ion beam transmission efficiency (incl. cyclotron) - marginal change in accelerated beam intensity a) intensity decreased due to losses caused by high pressure b) analysis show that the intensity within the acceptance of cyclotron changed marginally Better space charge compensation can improve the beam quality drastically. Losses has to be avoided: filament?

Summary - frequency tuning can be an efficient tool to: 1) Increase the intensity of highly charged ion beams 2) Affect the beam quality - Q-value with the plasma absorption is high (≈ 2000) better space charge compensation can improve the ion beam quality Please see interesting posters by O. Tarvainen and T. Ropponen