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Impact of Magnetic Field Configuration on Heat Transport in Stellarators and Heliotrons

  • Felix Warmer
  • , K. Tanaka
  • , P. Xanthopoulos
  • , M. Nunami
  • , M. Nakata
  • , C. D. Beidler
  • , S. A. Bozhenkov
  • , M. N.A. Beurskens
  • , K. J. Brunner
  • , O. P. Ford
  • , G. Fuchert
  • , H. Funaba
  • , J. Geiger
  • , D. Gradic
  • , K. Ida
  • , H. Igami
  • , S. Kubo
  • , A. Langenberg
  • , H. P. Laqua
  • , S. Lazerson
  • T. Morisaki, M. Osakabe, N. Pablant, E. Pasch, B. Peterson, S. Satake, R. Seki, T. Shimozuma, H. M. Smith, T. Stange, A. V. Stechow, H. Sugama, Y. Suzuki, H. Takahashi, T. Tokuzawa, T. Tsujimura, Y. Turkin, R. C. Wolf, I. Yamada, R. Yanai, R. Yasuhara, M. Yokoyama, Y. Yoshimura, M. Yoshinuma, D. Zhang, Team W7-X Team

Research output: Contribution to journalArticlepeer-review

Abstract

We assess the magnetic field configuration in modern fusion devices by comparing experiments with the same heating power, between a stellarator and a heliotron. The key role of turbulence is evident in the optimized stellarator, while neoclassical processes largely determine the transport in the heliotron device. Gyrokinetic simulations elucidate the underlying mechanisms promoting stronger ion scale turbulence in the stellarator. Similar plasma performances in these experiments suggests that neoclassical and turbulent transport should both be optimized in next step reactor designs.

Original languageEnglish (US)
JournalPhysical review letters
Volume127
Issue number22
DOIs
StatePublished - Nov 24 2021

All Science Journal Classification (ASJC) codes

  • General Physics and Astronomy

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