Abstract

A model for simulating charge exchange (CX) of fast ions with background atoms in magnetically confined fusion plasmas has been implemented in the ASCOT orbit-following code. The model was verified by comparing simulated reaction mean free paths to analytical values across a range of fusion-relevant parameters. ASCOT was used to simulate beam ions slowing down in the presence of CX reactions in a MAST-U target scenario. ASCOT predicts the CX-induced loss of beam power to be , which agrees to within with the TRANSP prediction. Due to CX, plasma heating and current drive by beam ions are strongly reduced towards the edge. However, an overall lower but noticeable increase of up to in current drive is predicted closer to the core. The simulated deposition of fast CX atoms on the wall is concentrated around the outer midplane, with estimated peak power loads of 70–80 kW m−2 on the central poloidal field coils (P5) and the vacuum vessel wall between them. This analysis demonstrates that ASCOT can be used to simulate fast ions in fusion plasmas where CX reactions play a significant role, e.g. in spherical tokamaks and stellarators.

Highlights

  • Charge-exchange (CX) reactions with background neutrals have been shown to have caused significant beam-ion losses in MAST [1], and the same issue is likely to arise in MAST-U

  • We introduce the new charge exchange (CX) model of the ASCOT code, its testing and demonstrative results regarding the impact of CX on beam ions in MAST-U

  • Figure 11. 2D projection of the reaction rate of CX neutralization of beam ions simulated by ASCOT

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Summary

Introduction

Charge-exchange (CX) reactions with background neutrals have been shown to have caused significant beam-ion losses in MAST [1], and the same issue is likely to arise in MAST-U. CX losses of beam ions result in the loss of heating power and

Current affiliation
Simulating charge exchange for fast ions
Verification by mean free path estimation
Simulating beam-ion charge exchange in MAST-U
Scenario inputs and approximations
Charge-exchange losses
Heating and current drive
Wall power loads
Findings
Summary and discussion
Full Text
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