Efficient generation of energetic ions in multi-ion plasmas by radio-frequency heating

Tutkimustuotos: Lehtiartikkelivertaisarvioitu


  • JET contributors
  • Alcator C-Mod Team


  • TEC Partner, Lab Plasma Phys, LPP ERM KMS
  • EURATOM CCFE Fus Assoc, Euratom, Culham Sci Ctr
  • Massachusetts Institute of Technology
  • Max Planck Inst Plasma Phys, Max Planck Society
  • Swiss Federal Institute of Technology Lausanne
  • Natl Fus Res Inst, National Fusion Research Institute (NFRI)
  • Forschungszentrum Julich GmbH, Helmholtz Association, Research Center Julich, Inst Energie & Klimaforsch Plasmaphys
  • ITER Org
  • Chinese Academy of Sciences
  • Polytechnic University of Madrid
  • ULB, Universite Libre de Bruxelles, Fluid & Plasma Dynam
  • Seoul National University
  • Inst Plasma Res, Institute for Plasma Research (IPR)
  • Univ Elect Sci & Technol China, University of Electronic Science & Technology of China
  • Uppsala University
  • European Commiss
  • University of Milano-Bicocca
  • Royal Institute of Technology
  • VTT Technical Research Centre of Finland


We describe a new technique for the efficient generation of high-energy ions with electromagnetic ion cyclotron waves in multi-ion plasmas. The discussed three-ion scenarios are especially suited for strong wave absorption by a very low number of resonant ions. To observe this effect, the plasma composition has to be properly adjusted, as prescribed by theory. We demonstrate the potential of the method on the world-largest plasma magnetic confinement device, JET (Joint European Torus, Culham, UK), and the high-magnetic-field tokamak Alcator C-Mod (Cambridge, USA). The obtained results demonstrate efficient acceleration of He-3 ions to high energies in dedicated hydrogendeuterium mixtures. Simultaneously, effective plasma heating is observed, as a result of the slowing-down of the fast He-3 ions. The developed technique is not only limited to laboratory plasmas, but can also be applied to explain observations of energetic ions in space-plasma environments, in particular, He-3-rich solar flares.


JulkaisuNature Physics
TilaJulkaistu - lokakuuta 2017
OKM-julkaisutyyppiA1 Julkaistu artikkeli, soviteltu

ID: 25727643