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. Due to 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 expected for other negative ion sources e.g. the full-size ITER ion source prototype SPIDER [2]. 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 [3], a new extraction grid was designed [4] to guarantee a better optics and a significant reduction of the beamlet deflection which proved to be quite large with the previous set of magnets [5]. The present paper presents the computation of the NIO1 beam optics as a function of the operating parameters. Throughout this work, the finite element codes OPERA 3D [6] and EAMCC [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 beamline diagnostics [8].
Modeling of Beam Acceleration for the Negative Ion Source NIO1
Serianni Gianluigi;
2017
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. Due to 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 expected for other negative ion sources e.g. the full-size ITER ion source prototype SPIDER [2]. 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 [3], a new extraction grid was designed [4] to guarantee a better optics and a significant reduction of the beamlet deflection which proved to be quite large with the previous set of magnets [5]. The present paper presents the computation of the NIO1 beam optics as a function of the operating parameters. Throughout this work, the finite element codes OPERA 3D [6] and EAMCC [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 beamline diagnostics [8].I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
