TY - JOUR
T1 - Scoping study of detecting high harmonic fast waves in NSTX-U hot core plasma directly using beam emission spectroscopy
AU - Rutherford, Grant
AU - Shiraiwa, Syun'Ichi
AU - Smith, David R.
AU - Bertelli, Nicola
N1 - Publisher Copyright:
© 2021 U.S. Government.
PY - 2021/5/1
Y1 - 2021/5/1
N2 - In this paper, we used radio frequency (RF) full wave simulation to explore the feasibility of generating a density beat oscillation formed by high harmonic fast waves (HHFWs) in the National Spherical Tokamak Experiment-Upgrade (NSTX-U) and of measuring it numerically with 2D beam emission spectroscopy (BES). This oscillation is of interest as it can be used to determine the injected RF fields. We began by computing HHFW fields in NSTX-U under a variety of experimental conditions and antenna configurations with Petra-M, a 3D RF wavefield solver. These fields were then used to evaluate the amplitude of δne,beat/ne0 in the volume of measurement, which we predict to be between 5 × 10-10 and 10-9, although it is highly dependent on plasma parameters. Trends in magnetic field, core temperature, core density, and antenna phasing are presented, and the parameters most suitable to this measurement are identified. Finally, we developed a synthetic BES diagnostic to compare the experimental BES signal against.
AB - In this paper, we used radio frequency (RF) full wave simulation to explore the feasibility of generating a density beat oscillation formed by high harmonic fast waves (HHFWs) in the National Spherical Tokamak Experiment-Upgrade (NSTX-U) and of measuring it numerically with 2D beam emission spectroscopy (BES). This oscillation is of interest as it can be used to determine the injected RF fields. We began by computing HHFW fields in NSTX-U under a variety of experimental conditions and antenna configurations with Petra-M, a 3D RF wavefield solver. These fields were then used to evaluate the amplitude of δne,beat/ne0 in the volume of measurement, which we predict to be between 5 × 10-10 and 10-9, although it is highly dependent on plasma parameters. Trends in magnetic field, core temperature, core density, and antenna phasing are presented, and the parameters most suitable to this measurement are identified. Finally, we developed a synthetic BES diagnostic to compare the experimental BES signal against.
UR - https://www.scopus.com/pages/publications/85105856379
UR - https://www.scopus.com/inward/citedby.url?scp=85105856379&partnerID=8YFLogxK
U2 - 10.1063/5.0040399
DO - 10.1063/5.0040399
M3 - Article
C2 - 34243267
AN - SCOPUS:85105856379
SN - 0034-6748
VL - 92
JO - Review of Scientific Instruments
JF - Review of Scientific Instruments
IS - 5
M1 - 053521
ER -