Transport Variations in High qmin>1.5 Plasmas with Heating and Current Drive Actuators

POSTER

Abstract

‘Predict-first’ methodology was employed to develop an experimental plan on DIII-D to study the effect of heating and current drive actuators on the current and pressure profiles of high-qmin>1.5, βN>3 plasmas, with the goal of achieving stable unchanging Vloop profiles as early in the discharge as possible to avoid the appearance of deleterious tearing modes. Predictive transport modeling conducted with TGLF in TRANSP indicated how varying the Ip ramp rate, ECCD timing, and NBI timing would change these profiles. During the experiment, qmin>2 discharges were sustained and their tearing instability, qmin, and performance was altered by these actuators. Changing the Ip ramp rate had little effect on the discharge but applying ECCD and/or NBI earlier increased qmin and improved n=2 tearing stability. TGLF predicted the effect of ECCD but not the other results. Increased fast-ion transport was also observed. Comparison of pre-experiment modeling, experimental results including turbulence data, and post-experiment simulations will be discussed in detail. These results will be used to validate transport models in this regime and to prepare for the upcoming 2019 campaign when increased off-axis co-Ip NBI power will be available.

Presenters

  • K.E. Thome

    GA, General Atomics

Authors

  • K.E. Thome

    GA, General Atomics

  • John Roderick Ferron

    General Atomics, General Atomics - San Diego, GA

  • C Craig Petty

    General Atomics, General Atomics - San Diego, GA

  • B.S. S Victor

    Lawrence Livermore National Laboratory, LLNL

  • Christopher T Holcomb

    Lawrence Livermore Natl Lab, LLNL

  • Eugenio Schuster

    Lehigh U, Lehigh Univ, Lehigh University

  • William P. Wehner

    Lehigh U, Lehigh Univ, Lehigh University

  • Jin Myung Park

    Oak Ridge National Lab, ORNL, ORNL, ORNL

  • B.A. A Grierson

    PPPL, Princeton Plasma Phys Lab, Princeton Plasma Physics Laboratory

  • Francesca M Poli

    Princeton Plasma Phys Lab, PPPL