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Alfvén Eigenmodes and Neoclassical tearing modes for orbit-following implementations

  • E. Hirvijoki*
  • , A. Snicker
  • , T. Korpilo
  • , P. Lauber
  • , E. Poli
  • , M. Schneller
  • , T. Kurki-Suonio
  • *Corresponding author for this work
  • Aalto University
  • Max-Planck-Institut für Plasmaphysik (IPP)

Research output: Contribution to journalArticleScientificpeer-review

Abstract

Magnetohydrodynamical instabilities such as Alfvn Eigenmodes and Neoclassical tearing modes redistribute energetic particles and, thus, potentially endanger the confinement of, e.g., fusion born alphas in Tokamaks. The orbit-following studies so far have been restricted either to time-independent approximation of the rotating modes, or to an axisymmetric magnetic field, which is an assumption severely compromised in ITER. In this paper we extend the previous work to accommodate time-dependent modes in non-axisymmetric magnetic fields.

Original languageEnglish
Pages (from-to)2589-2593
JournalComputer Physics Communications
Volume183
Issue number12
DOIs
Publication statusPublished - Dec 2012
MoE publication typeA1 Journal article-refereed

UN SDGs

This output contributes to the following UN Sustainable Development Goals (SDGs)

  1. SDG 7 - Affordable and Clean Energy
    SDG 7 Affordable and Clean Energy

Keywords

  • General coordinates
  • MHD activity
  • Non-axisymmetry
  • Particle following

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