David C. Speirs, Juan Ruiz-Ruiz, Maurizio Giacomin, Valerian H. Hall-Chen, Alan D. R. Phelps, Roddy Vann, Peter G. Huggard, Hui Wang, Anthony Field, Kevin Ronald
{"title":"Simulation and analysis of a high-k electron scale turbulence diagnostic for MAST-U","authors":"David C. Speirs, Juan Ruiz-Ruiz, Maurizio Giacomin, Valerian H. Hall-Chen, Alan D. R. Phelps, Roddy Vann, Peter G. Huggard, Hui Wang, Anthony Field, Kevin Ronald","doi":"arxiv-2408.15807","DOIUrl":null,"url":null,"abstract":"Plasma turbulence on disparate spatial and temporal scales plays a key role\nin defining the level of confinement achievable in tokamaks, with the\ndevelopment of reduced numerical models for cross-scale turbulence effects\ninformed by experimental measurements an essential step. MAST-U is a\nwell-equipped facility having instruments to measure ion and electron scale\nturbulence at the plasma edge. However, measurement of core electron scale\nturbulence is challenging, especially in H mode. Using a novel synthetic\ndiagnostic approach, we present simulated measurement specifications of a\nproposed mm-wave based collective scattering instrument optimised for measuring\nboth normal and binormal electron scale turbulence in the core and edge of\nMAST-U. A powerful modelling framework has been developed that combines\nbeam-tracing techniques with gyrokinetic simulations to predict the\nsensitivity, localisation and spectral range of measurement. For the\nreconstructed MAST 022769 shot, a maximum measurable normalised bi-normal\nwavenumber of $k_{\\perp} \\rho_{e} \\sim 0.6$ was predicted in the core and\n$k_{\\perp} \\rho_{e} \\sim 0.79$ near the pedestal, with localisation lengths\n$L_{FWHM}$ ranging from $\\sim$ 0.4 m in the core at $k_{\\perp} \\rho_{e} \\sim\n0.1$ to ~0.08m at $k_{\\perp} \\rho_{e} \\sim 0.45$. Synthetic diagnostic analysis\nfor the 022769 shot using CGYRO gyrokinetic simulation spectra reveal that ETG\nturbulence wavenumbers of peak spectral intensity comfortably fall within the\nmeasurable range of the instrument from the core to the pedestal. The proposed\ndiagnostic opens up opportunities to study new regimes of turbulence and\nconfinement in association with upcoming non-inductive, microwave based current\ndrive experiments on MAST-U and can provide insight into cross-scale turbulence\neffects, while having suitability to operate during burning plasma scenarios on\nfuture reactors such as STEP.","PeriodicalId":501274,"journal":{"name":"arXiv - PHYS - Plasma Physics","volume":"185 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-08-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Plasma Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2408.15807","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
Plasma turbulence on disparate spatial and temporal scales plays a key role
in defining the level of confinement achievable in tokamaks, with the
development of reduced numerical models for cross-scale turbulence effects
informed by experimental measurements an essential step. MAST-U is a
well-equipped facility having instruments to measure ion and electron scale
turbulence at the plasma edge. However, measurement of core electron scale
turbulence is challenging, especially in H mode. Using a novel synthetic
diagnostic approach, we present simulated measurement specifications of a
proposed mm-wave based collective scattering instrument optimised for measuring
both normal and binormal electron scale turbulence in the core and edge of
MAST-U. A powerful modelling framework has been developed that combines
beam-tracing techniques with gyrokinetic simulations to predict the
sensitivity, localisation and spectral range of measurement. For the
reconstructed MAST 022769 shot, a maximum measurable normalised bi-normal
wavenumber of $k_{\perp} \rho_{e} \sim 0.6$ was predicted in the core and
$k_{\perp} \rho_{e} \sim 0.79$ near the pedestal, with localisation lengths
$L_{FWHM}$ ranging from $\sim$ 0.4 m in the core at $k_{\perp} \rho_{e} \sim
0.1$ to ~0.08m at $k_{\perp} \rho_{e} \sim 0.45$. Synthetic diagnostic analysis
for the 022769 shot using CGYRO gyrokinetic simulation spectra reveal that ETG
turbulence wavenumbers of peak spectral intensity comfortably fall within the
measurable range of the instrument from the core to the pedestal. The proposed
diagnostic opens up opportunities to study new regimes of turbulence and
confinement in association with upcoming non-inductive, microwave based current
drive experiments on MAST-U and can provide insight into cross-scale turbulence
effects, while having suitability to operate during burning plasma scenarios on
future reactors such as STEP.