A new quasilinear saturation rule for tokamak turbulence with application to the isotope scaling of transport

H. G. Dudding, F. J. Casson, D. Dickinson, B. S. Patel, C. M. Roach, E. A. Belli, G. M. Staebler

Research output: Contribution to journalArticlepeer-review

11 Scopus citations

Abstract

A new quasilinear saturation model SAT3 has been developed for the purpose of calculating radial turbulent fluxes in the core of tokamak plasmas. The new model is shown to be able to better recreate the isotope mass dependence of nonlinear gyrokinetic fluxes compared to contemporary quasilinear models, including SAT2(Staebler et al 2021 Nucl. Fusion 61 116007), while performing at least as well in other key equilibrium parameters. By first quantifying the isotope scaling of gyrokinetic flux spectra, it is shown that the deviation from the gyroBohm scaling of fluxes originates primarily in the magnitude of the saturated potentials. Using this result SAT3 was formulated using observations made from gyrokinetic data, including a novel and robust relation between the 1D potential spectrum and the radial spectral widths. This serves to define the underlying functional forms of SAT3 before then connecting to the linear dynamics, including a difference in saturation level between ITG- and TEM-dominated turbulence, with the resulting free parameters having been fit to a database of high-resolution nonlinear CGYRO simulations. Additional features outside of the database are included, including E × B shear and multi-ion plasma capability. The methodology used in the development of SAT3 represents an algorithm which can be used in the improvement and generation of future saturation models.

Original languageEnglish
Article number096005
JournalNuclear Fusion
Volume62
Issue number9
DOIs
StatePublished - Sep 2022
Externally publishedYes

Funding

The authors would like to thank Y. Camenen and J. Citrin for their discussions and insights that contributed to this work. This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom Research and Training Programme 2014–2018 and 2019–2020 under Grant Agreement No. 633053. The views and opinions expressed herein do not necessarily reflect those of the European Commission. This work was supported by the Engineering and Physical Sciences Research Council [EP/L01663X/1, EP/R034737/1, EP/T012250/1, EP/W006839/1]. The authors would like to acknowledge access to the CINECA High-Performance Computer MARCONI, and to the JFRS-1 resource through QST.

Keywords

  • gyrokinetic
  • isotope
  • quasilinear
  • saturation
  • transport
  • turbulence

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