Author: Gammino, S.
Paper Title Page
MOWZO03 Status of the AISHa Ion Source at INFN-LNS 10
 
  • L. Celona, G. Calabrese, G. Castro, F. Chines, S. Gammino, O. Leonardi, G. Manno, D. Mascali, A. Massara, S. Passarello, D. Siliato, G. Torrisi
    INFN/LNS, Catania, Italy
  • G. Costanzo
    INFN-Pavia, Pavia, Italy
  • C. Maugeri, F. Russo
    CNAO Foundation, Pavia, Italy
 
  The AISHa ion source is an Electron Cyclotron Resonance Ion Source designed to generate high brightness multiply charged ion beams with high reliability, easy operations and maintenance for hadrontheraphy applications. The R&D performed by the INFN-LNS team during the 2019/2020 has allowed the improvement of the AISHa performances up to 20% for some of the extracted beams: both injection and extraction flanges has been improved and a movable electrode has been installed. The low energy beam transport has been equipped of an Emittance Measurement Unit (EMU), working through the beam wire scanners principle, for the measurement of the vertical and horizontal emittance of the beams of interest for hadrontherapy applications. Beam emittance has been characterized as a function of q/m and of the beam intensity to highlight space charge effects. If necessary, the beam wire scanners can be used for the characterization of the beam shape. The perspectives for further developments and plasma diagnostics will be also highlighted.  
slides icon Slides MOWZO03 [24.738 MB]  
DOI • reference for this paper ※ https://doi.org/10.18429/JACoW-ECRIS2020-MOWZO03  
About • Received ※ 27 September 2020 — Revised ※ 12 November 2020 — Accepted ※ 06 February 2022 — Issue date ※ 05 July 2022
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MOYZO01 Imaging in X-ray Ranges to Locally Investigate the Effect of the Two-Close-Frequency Heating in ECRIS Plasmas 27
 
  • R. Rácz, S. Biri, Z. Perduk
    Atomki, Debrecen, Hungary
  • G. Castro, L. Celona, S. Gammino, D. Mascali, M. Mazzaglia, E. Naselli, G. Torrisi
    INFN/LNS, Catania, Italy
  • A. Galatà
    INFN/LNL, Legnaro (PD), Italy
  • E. Naselli
    Catania University, Catania, Italy
  • J. Pálinkás
    University Debrecen, Debrecen, Hungary
 
  Plasma instabilities limit the ECR Ion Sources performances in terms of flux of the extracted highly charged ions by causing beam ripple and unstable operation conditions. In a 14 GHz ECRIS (Atomki, Debrecen), the effect on the plasma instabilities in an Argon plasma at Two Close Frequencies heating scheme (the frequency gap is smaller than 1 GHz) has been explored. A special multi-diagnostic setup [1, 2] has been designed and implemented consisting of detectors for the simultaneous collection of plasma radio-self-emission and of high spatial resolution X-ray images in the 500 eV - 20 keV energy domain (using an X-ray pin-hole camera setup). We present the comparison of plasma structural changes as observed from X-ray images in single and double-frequency operations. The latter has been particularly correlated to the confinement and velocity anisotropy, also by considering results coming from numerical simulations.
[1] S. Biri et al. Journal of Instrumentation 13(11):C11016 DOI: 10.1088/1748-0221/13/11/C11016
[2] E. Naselli et. al. Journal of Instrumentation 14(10):C10008 DOI: 10.1088/1748-0221/14/10/C10008
 
slides icon Slides MOYZO01 [7.325 MB]  
DOI • reference for this paper ※ https://doi.org/10.18429/JACoW-ECRIS2020-MOYZO01  
About • Received ※ 25 September 2020 — Revised ※ 11 November 2020 — Accepted ※ 17 December 2020 — Issue date ※ 24 January 2021
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MOYZO02 High Resolution X-ray Imaging as a Powerful Diagnostics Tool to Investigate ECRIS Plasma Structure and Confinement Dynamics 32
 
  • E. Naselli, G. Castro, L. Celona, S. Gammino, D. Mascali, M. Mazzaglia, G. Torrisi
    INFN/LNS, Catania, Italy
  • S. Biri, Z. Perduk, R. Rácz
    Atomki, Debrecen, Hungary
  • A. Galatà
    INFN/LNL, Legnaro (PD), Italy
  • E. Naselli
    Catania University, Catania, Italy
  • J. Pálinkás
    DU, Debrecen, Hungary
 
  High resolution spatially-resolved X-ray spectroscopy, by means of a X-ray pin-hole camera setup* ** operating in the 0.5-20 keV energy domain, is a very powerful method for ECRIS plasma structure evaluation. We present the setup installed at a 14 GHz ECRIS (ATOMKI, Debrecen), including a multi-layered collimator enabling measurements up to several hundreds of watts of RF pumping power and the achieved spatial and energy resolution (0.5 mm and 300 eV). Results coming by a new algorithm for analyzing Integrated (multi-events detection) and Photon-Counted images (single-event detection) to perform energy-resolved investigation will be described. The analysis permits to investigate High-Dynamic-Range (HDR) and spectrally resolved images, to study the effect of the axial and radial confinement (even separately), the plasma radius, the fluxes of deconfined electrons distinguishing fluorescence lines of the materials of the plasma chamber (Ti, Ta) from plasma (Ar) fluorescence lines. This method allows a detailed characterization of warm electrons, important for ionization, and to quantitatively estimate local plasma density and spectral temperature pixel-by-pixel.
*S. Biri et al., JINST 13(11):C11016-C11016, DOI:10.1088/1748-0221/13/11/C11016
**E. Naselli et al., JINST 14(10):C10008-C10008, DOI:10.1088/1748-0221/14/10/C10008
 
slides icon Slides MOYZO02 [26.629 MB]  
DOI • reference for this paper ※ https://doi.org/10.18429/JACoW-ECRIS2020-MOYZO02  
About • Received ※ 27 September 2020 — Revised ※ 02 October 2020 — Accepted ※ 18 November 2020 — Issue date ※ 17 December 2020
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TUXZO02
Experimental Evidence of E.M. trapped E.M. waves in a Simple Mirror Magnetic-Trap  
 
  • G. Castro, L. Celona, S. Gammino, O. Leonardi, D. Mascali, G. Torrisi
    INFN/LNS, Catania, Italy
  • R. Miracoli
    ESS Bilbao, Zamudio, Spain
 
  This work presents the first experimental characterization of cavity modes trapped within a plasma column in an axis-symmetric magnetic trap. Trapped wave has been characterized by means of a movable antenna as a function of the Bmin/BECR ratio and plasma parameters. The study demonstrates that E.M waves can be enclosed two R-cutoff layers, close to the B minimum position. Results suggest that the trapped waves consist of waves propagating across the magnetic field and storing large part of the E.M. power. If R-cut-off is removed by increasing the density, trapped waves are not detected longer. A typical Electron Energy Distribution Function composed by two different electron populations is measured in the layer where trapped waves are revealed, suggesting that additional heating is occurring.  
slides icon Slides TUXZO02 [6.058 MB]  
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