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Fast-ion orbit sensitivity of neutron and gamma-ray diagnostics for one-step fusion reactions

作者:H. Järleblad, L. Stagner, M. Salewski, J. Eriksson, M. Nocente, J. Rasmussen, Ž. Štancar, Ye. O. Kazakov, B. Simmendefeldt, Jet Contributors · 发表于:Nuclear Fusion · 年份:2022 · DOI:10.1088/1741-4326/ac63d3 · 被引用次数:26 · 研究领域:Magnetic confinement fusion research、Nuclear Physics and Applications、Nuclear reactor physics and engineering

Abstract Fast ions in the MeV-range can be diagnosed by neutron emission spectroscopy (NES) and gamma-ray spectroscopy (GRS). In this work, we present orbit weight functions for one-step fusion reactions, using NES and GRS diagnostics on perpendicular and oblique lines-of-sight (LOS) at Joint European Torus (JET) as examples. The orbit weight functions allow us to express the sensitivities of the diagnostics in terms of fast-ion (FI) orbits and can be used to swiftly reproduce synthetic signals that have been computed by established codes. For diagnostically relevant neutron energies for the D(D, n) 3 He reaction, the orbit sensitivities of the NES diagnostics follow a predictable pattern. As the neutron energy of interest increases, the pattern shifts upwards in FI energy. For the GRS diagnostic and the T(p, γ ) 4 He reaction, the orbit sensitivity is shown to be qualitatively different for red-shifted, blue-shifted and nominal gamma birth energies. Finally, we demonstrate how orbit weight functions can be used to decompose diagnostic signals into the contributions from different orbit types. For a TRANSP simulation of the JET discharge (a three-ion ICRF scenario) considered in this work, the NES signals for both the perpendicular and oblique LOS are shown to originate mostly from co-passing orbits. In addition, a significant fraction of the NES signal for the oblique LOS is shown to originate from stagnation orbits.