Computer Simulations of Twisted Flux Tubes and Magnetic Reconnection

  • T. Hayashi
  • M. Ozaki
  • H. Kitabata
  • T. Sato
Part of the Astrophysics and Space Science Library book series (ASSL, volume 229)

Abstract

To investigate the dynamical problem of continuously twisted flux tubes, elaborate three-dimensional MHD simulations have been performed (Amo, et al. 1995). Initially a uniform straight axial magnetic field is assumed. A twisting motion is applied continuously at both ends of the flux tube. An excess magnetic energy is accumulated in the system as the twist goes on. When the flux tube is largely twisted and free energy is sufficiently stored, the structure becomes unstable to kink modes.

Keywords

Magnetic Reconnection Flux Tube Magnetic Flux Tube Twist Flux Tube Magnetic Reconnec 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. H. Amo, T. Sato, A. Kageyama, K. Watanabe, R. Horiuchi, T. Hayashi, Y. Todo, T.H. Watanabe, H. Takamaru, Phys. Rev. E 51, 3838 (1995).ADSCrossRefGoogle Scholar
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Copyright information

© Springer Science+Business Media Dordrecht 1998

Authors and Affiliations

  • T. Hayashi
    • 1
  • M. Ozaki
    • 1
  • H. Kitabata
    • 1
  • T. Sato
    • 1
  1. 1.National Institute for Fusion ScienceToki, GifuJapan

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