Since 18 of December 2019 conferences.iaea.org uses Nucleus credentials. Visit our help pages for information on how to Register and Sign-in using Nucleus.

6–10 Dec 2021
Virtual Event
Europe/Vienna timezone
Official invitations and technical information that will enable designated participants to join the virtual event will be sent 1–2 weeks before the meeting.

Orbit Weight Functions for Neutron Emission and One-step Reaction Gamma-Ray Spectroscopy Diagnostics

8 Dec 2021, 15:50
20m
Virtual Event

Virtual Event

Oral Diagnostics for Energetic Particles Runaway Electrons, Disruptions, and Diagnostics

Speaker

Henrik Järleblad (DTU Physics, Technical University of Denmark)

Description

Fast-ion distribution functions in the MeV-range can be diagnosed by neutron emission spectroscopy (NES) and gamma-ray spectroscopy (GRS). For a given fast-ion distribution function and diagnostic energy bin, a measurement signal will have contributions originating from various fast-ion orbits [Ref1][Ref2]. These contributions depend on the sensitivity of the diagnostic in orbit phase space, which can be mapped using weight functions. Velocity-space weight functions have previously been used to map the sensitivity in 2D velocity space[Ref3][Ref4][Ref5]. In this work, we present and discuss 3D orbit weight functions for the Joint European Torus NES diagnostic TOFOR[Ref6], an NE213-scintillator[Ref7] and a high-purity germanium GRS diagnostic[Ref8]. The complicated three-dimensional structures of these so-called orbit sensitivities can be mapped by varying the fast-ion energy while tracing out the topological boundaries between different orbit types. Furthermore, the sensitivity is found to vary depending on the diagnostic energy bin of interest, as determined by the requirement to produce a sufficient amount of up- or down-shift of the nominal birth energy of neutrons from D(D,n)$^{3}$He and gammas from T(p,$\gamma$)$^{4}$He. Using this approach, signal contribution split into orbit types is presented for the first time.

A fast-ion energy (E) slice of an orbit weight function for TOFOR. The plot shows normalized fast-ion orbit sensitivity for a specific diagnostic energy (Ed) bin for JET discharge #94701 at 10.7932 s

A fast-ion energy (E) slice of an orbit weight function for the NE213-scintillator. The plot shows normalized fast-ion orbit sensitivity for a specific diagnostic energy (Ed) bin for JET discharge #94701 at 10.7932 s

A fast-ion energy (E) slice of an orbit weight function for the high-purity germanium diagnostic. The plot shows normalized fast-ion orbit sensitivity for a specific diagnostic energy (Ed) bin for JET discharge #94701 at 10.7932 s

--- References ---
[Ref1] H. Järleblad et al, Rev. Sci. Instrum. 92, 043526 (2021)
[Ref2] L. Stagner & W. W. Heidbrink, Phys. Plasmas 24, 092505 (2017)
[Ref3] M. Salewski et al, Nucl. Fusion 58, 096019 (2018)
[Ref4] J. Eriksson et al, Plasma Phys. Control. Fusion 61, 014027 (2019)
[Ref5] B.S. Schmidt et al, Rev. Sci. Instrum. 92, 053528 (2021)
[Ref6] M. Gatu Johnson et al, Nucl. Instrum. Methods Phys. Res., Sect. A 591, 417 (2008)
[Ref7] F. Binda et al, Rev. Sci. Instrum. 85, 11E23 (2014)
[Ref8] M. Tardocchi et al, Phys. Rev. Letters 107, 205002 (2011)

Speaker's Affiliation Department of Physics, Technical University of Denmark, Kgs. Lyngby, Denmark
Member State or IGO Denmark

Primary author

Henrik Järleblad (DTU Physics, Technical University of Denmark)

Co-authors

Luke Stagner (Oak Ridge Institute for Science and Education) Mirko Salewski (Technical University of Denmark) Mr Jacob Eriksson (Department of Physics and Astronomy, Uppsala University, Sweden) Massimo Nocente (Dipartimento di Fisica, Università di Milano-Bicocca) Mr Jesper Rasmussen (Department of Physics, Technical University of Denmark, Kgs. Lyngby, Denmark) Mr Bo Schmidt (Department of Physics, Technical University of Denmark, Kgs. Lyngby, Denmark)

Presentation materials