The RF negative ion source NIO1 (Negative Ion Optimization 1) [1], built at Consorzio RFX in Padova (Italy), aims at investigating basic issues of ion source physics while providing a tool to benchmark and validate beam simulation codes. On the other hand, because of its small size and its modular design, NIO1 represents a valuable testbed for DEMO relevant solutions, such as energy recovery and alternative systems for ion beam neutralization [1]. To such purposes it is important to improve NIO1 performance to make it comparable to those achieved or expected by other ITER relevant negative ion sources, such as ELISE [2] or SPIDER [3] and already a. In particular the latest NIO1 upgrades focused on reducing the co-extracted electrons by enlarging the magnetic field strength close to the plasma grid and on improving the beam optics. As anticipated in [4], a new extraction grid was designed [5] to guarantee a better optics and a significant reduction of the beamlet deflection. The present paper presents the computation of the NIO1 beam optics as a function of the operating parameters. Throughout this work, the finite element code OPERA3D [6] and the Monte Carlo particle tracing code EAMCC3D [7] were used to model the NIO1 accelerator in both its previous and new configurations. Results from simulations are also compared with the data from NIO1 diagnostic calorimeter [8].

Modeling of beam acceleration for the negative ion source NIO1

Serianni G;
2018

Abstract

The RF negative ion source NIO1 (Negative Ion Optimization 1) [1], built at Consorzio RFX in Padova (Italy), aims at investigating basic issues of ion source physics while providing a tool to benchmark and validate beam simulation codes. On the other hand, because of its small size and its modular design, NIO1 represents a valuable testbed for DEMO relevant solutions, such as energy recovery and alternative systems for ion beam neutralization [1]. To such purposes it is important to improve NIO1 performance to make it comparable to those achieved or expected by other ITER relevant negative ion sources, such as ELISE [2] or SPIDER [3] and already a. In particular the latest NIO1 upgrades focused on reducing the co-extracted electrons by enlarging the magnetic field strength close to the plasma grid and on improving the beam optics. As anticipated in [4], a new extraction grid was designed [5] to guarantee a better optics and a significant reduction of the beamlet deflection. The present paper presents the computation of the NIO1 beam optics as a function of the operating parameters. Throughout this work, the finite element code OPERA3D [6] and the Monte Carlo particle tracing code EAMCC3D [7] were used to model the NIO1 accelerator in both its previous and new configurations. Results from simulations are also compared with the data from NIO1 diagnostic calorimeter [8].
2018
Istituto gas ionizzati - IGI - Sede Padova
Inglese
17th International Conference on Ion Sources (ICIS 2017)
2011
080023-1
080023-3
3
9780735417274
https://aip.scitation.org/doi/abs/10.1063/1.5053378
AMER INST PHYSICS, CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1
MELVILLE, NY 11747-4501
STATI UNITI D'AMERICA
September 15-20, 2017
Geneva (Switzerland)
Negative Ion Source
Negative Ion Optimization 1
NIO1
beam acceleration
Article Number: 080023 / Electronic ISSN: 1551-7616 / http://www.scopus.com/inward/record.url?eid=2-s2.0-85054178375&partnerID=q2rCbXpz / This wark has been carried out within the framework of EUROfusion Consortium and has received funding from the Euratom research and training programme 2014-2018 under grant agreement N. 633053.
4
none
Pimazzoni, A; Cavenago, M; Serianni, G; Veltri, P
273
info:eu-repo/semantics/conferenceObject
04 Contributo in convegno::04.01 Contributo in Atti di convegno
   Implementation of activities described in the Roadmap to Fusion during Horizon 2020 through a Joint programme of the members of the EUROfusion consortium
   EUROfusion
   H2020
   633053
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/351170
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