Simulation of KSTAR ITER scenarios with the RAPTOR code

POSTER

Abstract

The RApid Plasma Transport SimulatOR (RAPTOR) code has been applied to KSTAR ITER Baseline (IBS), hybrid scenario, and KSTAR-DIII-D joint hybrid experiments. RAPTOR evolves magnetic flux and kinetic profiles relevant for scenario access optimization, which is typically performed through heating and current drive actuator scans in experiment. Validation work presented here compares RAPTOR predictions with experimental plasma parameter evolution through hybrid and IBS access phases. We compare safe and unsafe plasma current rampdown trajectories with KSTAR experiments. RAPTOR’s capabilities offer fast nonlinear optimization of scenario actuator trajectories, informing intuition of the effects of actuator location and timing in scenario experiments. RAPTOR can provide initial scenario setup conditions for efficient translation of DIII-D ITER scenario plasmas to superconducting devices like KSTAR, whose shaping coil and plasma current ramp rates differ from those available to copper devices. Imminent work attempting ITER scenario access in KSTAR experiments guided by RAPTOR will quantify the effectiveness of this workflow.

*This material is based upon work supported by the Department of Energy under Award Number(s) DE-SC0023399.Disclaimer: This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof.

Presenters

  • William Boyes

    • ORAU

Authors

  • William Boyes

    • ORAU
  • Olivier Sauter

    • EPFL
    • SPC-EPFL
    • Ecole Polytechnique Federale de Lausanne
  • Nicolas Eidietis

    • General Atomics
    • GA
  • Jayson L Barr

    • General Atomics - San Diego
  • Cassandre Contre

    • EPFL
  • Wilkie Choi

    • General Atomics