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Understanding the L-H transition isotope effect in DIII-D

ORAL · Invited

Abstract

Recent database and gyro-kinetic analysis of DIII-D plasmas in low-confinement mode (L-mode) just before transition to high-confinement mode (H-mode) have identified decreased carbon impurity content as the dominant isotope effect responsible for increasing the L-H power threshold (PLH) in hydrogen at ITER-relevant low collisionality. Increased Zeff in deuterium, due to enhanced (mass dependent) physical and chemical sputtering of graphite (carbon) from diverter and main chamber tiles, is found to increase the ITG critical gradient, stabilizing ITG modes [1]. Gyro-fluid and gyro-kinetic simulations capture the observed impurity isotope effect and its influence on electron and ion heat transport and power loss, via the TGLF and CGYRO codes, respectively. Edge simulations identify subdominant, intrinsic main ion mass effects due to electron non-adiabaticity [2] and differences in normalized E⨉B shear, that also contribute significantly to the isotope scaling of PLH. At high collisionality, no isotope effect is observed, as previously documented [3]. Measurements of density and electron temperature fluctuations using the Beam Emission Spectroscopy (BES) and Correlation Electron Cyclotron Emission (CECE) diagnostics, respectively, were found to agree well with turbulence predictions from flux matched CGYRO simulations at ρ = 0.7, 0.9, & 0.95. This comparison was made possible via advanced synthetic diagnostics. The observed PLH reduction with low-Z impurity dilution opens the important prospect of improving H-mode access in ITER hydrogen plasmas via Ne or N seeding.

[1] S. Migliuolo 1992 Nucl. Fusion 32 1331

[2] Belli, E. A. et al 2020 PRL 125.1 015001

[3] Z. Yan et al. 2017 Nucl. Fusion 57, 126015

Presenters

  • Kyle Callahan

    University of California, Los Angeles

Authors

  • Kyle Callahan

    University of California, Los Angeles

  • Lothar Schmitz

    University of California, Los Angeles

  • Troy A Carter

    University of California, Los Angeles

  • Shaun R Haskey

    Princeton Plasma Physics Laboratory

  • Colin Chrystal

    General Atomics - San Diego

  • Emily A Belli

    General Atomics

  • Christopher G Holland

    University of California, San Diego

  • Kathreen E Thome

    GA

  • George R McKee

    University of Wisconsin - Madison, UWisc. Madison

  • Arash Ashourvan

    General Atomics

  • Guiding Wang

    University of California, Los Angeles

  • Quinn Pratt

    University of California, Los Angeles

  • Zheng Yan

    University of Wisconsin - Madison

  • Matthias Knolker

    General Atomics

  • Florian Effenberg

    Princeton Plasma Physics Laboratory

  • Alessandro Bortolon

    Princeton Plasma Physics Laboratory, PPPL

  • Filipp Khabanov

    Wisconsin-Madison, University of Wisconsin-Madison, University of Wisconsin–Madison, University of Wisconsin- Madison, UWM