28 September 2026 to 2 October 2026
Lausanne, Switzerland
Europe/Paris timezone
Please register to the meeting through the LOC website: https://tmep26.epfl.ch/

Investigation of Fast-Ion Velocity Distribution Functions via Neutron Emission Spectroscopy on EAST

30 Sept 2026, 09:35
25m
Beaulieu Congress and Exhibition Center (Lausanne, Switzerland)

Beaulieu Congress and Exhibition Center

Lausanne, Switzerland

Local website: https://tmep26.epfl.ch/
Oral EPs in stellarators and 3D configurations I EP diagnostics and analysis methods

Speaker

Andong Xu (Peking University)

Description

This report presents an overview of the experimental results and data processing advancements in fast-ion diagnostics using neutron emission spectroscopy (NES) on the EAST tokamak.

The EAST NES system comprises multiple spectrometers arranged along four lines of sight (LOS), including a time-of-flight enhanced diagnostic (TOFED), a stilbene crystal, three liquid scintillators, a CLYC, a LaCl$_3$ spectrometer, and a newly installed single-crystal diamond spectrometer in the 2026 campaign. These detectors, varying in viewing angles and physical principles, cover different regions of the fast-ion phase space (particularly energies > 100 keV), enabling a systematic evaluation of diagnostic capabilities.

During synergistic NBI and third-harmonic ICRF heating, a significant broadening of the neutron spectra was observed across multiple spectrometers, indicating fast-ion acceleration well beyond the injection energy [1]. TRANSP simulations, validated by synthetic spectra generated by the GENESIS code and the instrument response functions (IRFs), as well as a weight-function analysis, revealed a fast-ion tail extending up to ~600 keV with a pronounced pitch-angle asymmetry favoring co-current velocities. Orbit calculations demonstrated that this asymmetry is primarily governed by the fast-ion loss boundaries on EAST.

Furthermore, in high poloidal beta ($\beta_{\mathrm{p}}$) discharges that achieved a record fusion neutron rate ($S_{\mathrm{n}}=3.9\times 10^{14}\,\mathrm{s}^{-1}$) on EAST, fast-ion behaviors under NBI and second-harmonic ICRF heating were analyzed by combining NES and neutron flux monitors (NFMs) [2]. Analysis shows that while the synergistic effect directly contributes $\sim30\%$ to the total neutron rate via the formation of a high-energy fast-ion tail, this enhancement is partially offset by NBI-induced profile degradation. Orbit phase-space analysis using the ORBIT code further revealed that synergistic heating drives suprathermal ions into smaller orbits (e.g., stagnation orbits), leading to the spatial redistribution of fast ions and the peaking of the neutron emissivity profile.

By systematically evaluating detectors across various distances, shielding configurations, and detection principles (TOF, organic, and Cl-based inorganic scintillators), this work establishes a comprehensive benchmark of NES for fast-ion diagnostics. Ongoing efforts focus on 4-LOS NES-only tomography and the development of orbit-space weight functions to understand the pronounced orbit effects typical of medium-sized tokamaks like EAST. Collectively, these advancements provide critical insights into high-fidelity fast-ion measurements, offering a robust technical framework for the design and optimization of NES-based diagnostics in future burning plasma devices.

References
[1] A.D. Xu et al 2026 Nucl. Fusion 66 066024
[2] A.D. Xu et al 2026 Nucl. Fusion (submitted)

Author

Andong Xu (Peking University)

Co-authors

Prof. Baolong Hao (Southwestern Institute of Physics, Chengdu, China) Prof. Baonian Wan (Institute of Plasma Physics, Chinese Academy of Sciences, Hefei, China) Mr Chenyu Pan (Institute of Plasma Physics, Chinese Academy of Sciences, Hefei, China) Prof. Giuseppe Gorini (University of Milano Bicocca, Milan, Italy) Prof. Guoqiang Zhong (Institute of Plasma Physics, Chinese Academy of Sciences, Hefei, China) Mr Jiayi Zhang (School of Physics, Peking University, Beijing, China) Prof. Juan Huang (Institute of Plasma Physics, Chinese Academy of Sciences, Hefei, China) Prof. Liqun Hu (Institute of Plasma Physics, Chinese Academy of Sciences, Hefei, China) Prof. Marco Tardocchi (Institute for Plasma Science and Technology, National Research Council (CNR), Milan, Italy) Prof. Massimo Nocente (University of Milano Bicocca, Milan, Italy) Mr Mingyuan Xu (Institute of Plasma Physics, Chinese Academy of Sciences, Hefei, China) Prof. Pan Li (Institute of Plasma Physics, Chinese Academy of Sciences, Hefei, China) Mr Tao Yu (School of Physics, Peking University, Beijing, China) Prof. Tieshuan Fan (School of Physics, Peking University, Beijing, China) Prof. Wei Zhang (Institute of Plasma Physics, Chinese Academy of Sciences, Hefei, China) Prof. Xiangqing Li (School of Physics, Peking University, Beijing, China) Mr Xiangyu Hong (Institute of Energy, Hefei Comprehensive National Science Center (Anhui Energy Laboratory)) Prof. Xinjun Zhang (Institute of Plasma Physics, Chinese Academy of Sciences, Hefei, China) Mr Xutao Xu (School of Physics, Peking University, Beijing, China) Mr Yongqiang Zhang (Institute of Plasma Physics, Chinese Academy of Sciences, Hefei, China) Mr Yubo Zhang (Institute of Plasma Physics, Chinese Academy of Sciences, Hefei, China) Dr Yunhe Li (School of Physics, Peking University, Beijing, China) Mr Zishi Liu (School of Physics, Peking University, Beijing, China) Mr Ziyu Wang (School of Physics, Peking University, Beijing, China)

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