Author: Toivanen, V.A.
Paper Title Page
TUCOBK03 Time Evolution of Plasma Potential in Pulsed Operation of ECRIS 93
 
  • O.A. Tarvainen, H. A. Koivisto, T. Ropponen, V.A. Toivanen
    JYFL, Jyväskylä, Finland
  • Y. Higurashi, T. Nakagawa
    RIKEN Nishina Center, Wako, Japan
 
  The time evolution of plasma potential has been measured in pulsed operation mode with electron cyclotron resonance ion sources at JYFL and RIKEN. Three different ion sources with microwave frequencies ranging from 6.4 to 18 GHz were employed for the experiments. The plasma potential during the preglow and afterglow transients was compared with steady state conditions. The plasma potential was observed to increase 25-75 % during the preglow and 10-30 % during the afterglow. We describe the experimental procedure and present the results of the study in detail.  
slides icon Slides TUCOBK03 [0.973 MB]  
 
TUPOT010 Effects of Microwave Frequency Fine Tuning on the Performance of JYFL 14 GHz ECRIS 137
 
  • V.A. Toivanen, V.P. Aho, J. Ärje, P. Jones, J.A. Kauppinen, H. A. Koivisto, P. Peura, O.A. Tarvainen
    JYFL, Jyväskylä, Finland
  • L. Celona, G. Ciavola, S. Gammino
    INFN/LNS, Catania, Italy
  • A. Galatà
    INFN/LNL, Legnaro (PD), Italy
  • D. Mascali
    CSFNSM, Catania, Italy
  • T. Ropponen
    NSCL, East Lansing, Michigan, USA
 
  Measurements have been carried out at Department of Physics, University of Jyväskylä (JYFL) to study the effects of microwave frequency fine tuning on the performance of JYFL 14 GHz electron cyclotron resonance ion source. The frequency was varied within an 85 MHz band around the normal operation frequency of 14.085 GHz. The radial bremsstrahlung emission was measured for plasma diagnostics purposes and mass separated ion beam currents extracted from the ion source were recorded at the same time. Also, beam quality studies were conducted by measuring the ion beam emittance and shape with and without enhanced space charge compensation. The obtained results are presented and possible origins of seen phenomena in measured quantities are discussed.  
poster icon Poster TUPOT010 [0.678 MB]  
 
TUPOT013 Influence of Initial Plasma Density and Mean Electron Energy on the Preglow Effect 146
 
  • I. Izotov, V. Sidorov, V. Skalyga, V. Zorin
    IAP/RAS, Nizhny Novgorod, Russia
  • H. A. Koivisto, O.A. Tarvainen, V.A. Toivanen
    JYFL, Jyväskylä, Finland
 
  The investigation of the Preglow effect is driven with the aim of creating a short-pulsed multicharged ion source. Recent experimental investigations have revealed strong influence of seed electrons, i.e. initial plasma density, on the amplitude and duration of the Preglow peak [1]. Present work, consisting of experiments and simulations, is dedicated to further investigation of the Preglow dependence on initial plasma density and electrons energy. Experimental investigation was performed at University of Jyväskylä (JYFL) with the A-ECR type ECRIS operated with 14 GHz frequency. Helium was used for the study. An initial ionization degree of the gas was varied by changing the pulse duration and duty factor. Time-resolved ion currents of He+ and He2+ were recorded. Calculations were made by using 0-dimensional model described in references [2], [3] and based on the balance equations for the particles confined in the magnetic trap. Results of simulation are compared with experimental Preglow peaks and discussed. Good agreement between experimental data and simulation encourages us to conduct a further study, aimed at optimizing the Preglow by tuning source parameters and initial plasma conditions.
[1] O. Tarvainen et al, Rev. Sci. Instrum., 81, 02A303, 2010.
[2] T. Thuillier et al, Rev. Sci. Instrum., 79, 02A314, 2008.
[3] I. Izotov et all. IEEE Trans. Plasma Sci. 36, 1494, 2008.
 
poster icon Poster TUPOT013 [0.569 MB]  
 
WECOAK05 Maximum Bremsstrahlung Energy Versus Different Heating Limits 175
 
  • H. A. Koivisto, V.P. Aho, P. Jones, P. Peura, J.H. Sarén, O.A. Tarvainen, V.A. Toivanen
    JYFL, Jyväskylä, Finland
 
  A comprehensive set of bremsstrahlung measurements have been performed at JYFL (University of Jyväskylä, Department of Physics) in order to understand the parameters affecting the time evolution of electron energy. In order to extend the understanding of electron heating, a new set of measurements with the JYFL 6.4 GHz ECRIS have been initiated to further study the parameters affecting the maximum bremsstrahlung energy. In the measurements the effect of magnetic field gradient, microwave power, plasma size and gas pressure were studied. In the analysis, main focus will be given to compare the results with different theoretical electron heating limits.  
slides icon Slides WECOAK05 [0.739 MB]