Affiliation:
1. Department of Physics and Astronomy, University of California Los Angeles, Los Angeles, CA 90095, USA
Abstract
The isotope dependence of the low- to high confinement-mode (L- to H-mode) transition power threshold
P
LH
presents significant challenges for the initial (non-nuclear) hydrogen operations phase of the international thermonuclear experimental reactor (ITER). Here, we examine the isotope dependence of turbulence and
E
×
B
flow correlation properties in the L-mode edge plasma, leading up to the L-H transition. At marginal auxiliary power (near
P
LH
), turbulence is initially suppressed periodically during limit cycle oscillations (LCO) that precede the transition to sustained H-mode confinement. We present evidence that the long-range (toroidal) correlation of the
E
×
B
edge plasma flow across the LCO phase is much weaker in hydrogen than in deuterium in the DIII-D tokamak, congruent with the higher threshold power
P
LH
required to access LCO and H-mode in hydrogen. Concomitantly, the time required to initially quench edge turbulence via localized edge
E
×
B
flow shear is significantly longer in hydrogen (1–1.5 ms) than in deuterium (approx. 100 µs). No toroidal long-range correlation of the turbulence amplitude is observed, in agreement with expectations based on the relatively short poloidal turbulence correlation length. Radial edge turbulence and flow correlation lengths are longer in deuterium than in hydrogen plasmas as one would expect from ‘naïve’ gyro-Bohm isotope transport scaling, despite the substantially higher thermal flux across the last closed flux surface in hydrogen before the L-H transition.
This article is part of a discussion meeting issue 'H-mode transition and pedestal studies in fusion plasmas'.
Funder
U.S. Department of Energy
Subject
General Physics and Astronomy,General Engineering,General Mathematics
Cited by
1 articles.
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1. H-mode transition and pedestal studies;Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences;2023-01-02