Abstract

We theoretically assess two mechanisms thought to be responsible for the enhanced performance observed in plasma discharges of the Wendelstein 7-X stellarator experiment fueled by pellet injection. The effects of the ambipolar radial electric field and the electron density peaking on the turbulent ion heat transport are separately evaluated using large-scale gyrokinetic simulations. The essential role of the stellarator magnetic geometry is demonstrated, by comparison with a tokamak.

Highlights

  • The effects of the ambipolar radial electric field and the electron density peaking on the turbulent ion heat transport are separately evaluated using large-scale gyrokinetic simulations

  • We focus on two phases of the discharge, see Fig. 1: (i) The electron cyclotron resonance (ECR) phase t 1⁄4 ð4 − 5Þ s, during which the effect of the pellets has vanished long after their injection into the plasma; this phase is essentially equivalent to the initial ECR-heated part of the discharge, prior to pellet injection. (ii) The pellet enhanced performance (PEP) phase t 1⁄4 ð1.65 − 1.75Þ s, taking place shortly after the pellet injections

  • Focusing on the radial location where the electric field reaches its most negative value, corresponding to the ion root solution of the ambipolarity relation [22], we notice that the PEP phase is characterized by both larger normalized electron density gradient a=Lne 1⁄4 ð−a=neÞdne=dr and ion temperature gradient a=LTi compared to the ECR phase

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Summary

Introduction

The effects of the ambipolar radial electric field and the electron density peaking on the turbulent ion heat transport are separately evaluated using large-scale gyrokinetic simulations. Such discharges involve transient phases characterized by enhanced performance, following shortly after the injection of cryogenic hydrogen pellets into an electron cyclotron resonance (ECR)-heated plasma [5].

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