MISC

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2015年1月8日

Flow damping due to stochastization of the magnetic field

Nature Communications
  • K. Ida
  • M. Yoshinuma
  • H. Tsuchiya
  • T. Kobayashi
  • C. Suzuki
  • M. Yokoyama
  • A. Shimizu
  • K. Nagaoka
  • S. Inagaki
  • K. Itoh
  • T. Akiyama
  • M. Emoto
  • T. Evans
  • A. Dinklage
  • X. Du
  • K. Fujii
  • M. Goto
  • T. Goto
  • M. Hasuo
  • C. Hidalgo
  • K. Ichiguchi
  • A. Ishizawa
  • M. Jakubowski
  • K. Kamiya
  • H. Kasahara
  • G. Kawamura
  • D. Kato
  • M. Kobayashi
  • S. Morita
  • K. Mukai
  • I. Murakami
  • S. Murakami
  • Y. Narushima
  • M. Nunami
  • S. Ohdach
  • N. Ohno
  • M. Osakabe
  • N. Pablant
  • S. Sakakibara
  • T. Seki
  • T. Shimozuma
  • M. Shoji
  • S. Sudo
  • K. Tanaka
  • T. Tokuzawa
  • Y. Todo
  • H. Wang
  • H. Yamada
  • Y. Takeiri
  • T. Mutoh
  • S. Imagawa
  • T. Mito
  • Y. Nagayama
  • K. Y. Watanabe
  • N. Ashikawa
  • H. Chikaraishi
  • A. Ejiri
  • M. Furukawa
  • T. Fujita
  • S. Hamaguchi
  • H. Igami
  • M. Isobe
  • S. Masuzaki
  • T. Morisaki
  • G. Motojima
  • K. Nagasaki
  • H. Nakano
  • Y. Oya
  • Y. Suzuki
  • R. Sakamoto
  • M. Sakamoto
  • A. Sanpei
  • H. Takahashi
  • M. Tokitani
  • Y. Ueda
  • Y. Yoshimura
  • S. Yamamoto
  • K. Nishimura
  • H. Sugama
  • T. Yamamoto
  • H. Idei
  • A. Isayama
  • S. Kitajima
  • S. Masamune
  • K. Shinohara
  • P. S. Bawankar
  • E. Bernard
  • M. Von Berkel
  • H. Funaba
  • X. L. Huang
  • T. Ii
  • T. Ido
  • K. Ikeda
  • S. Kamio
  • R. Kumazawa
  • C. Moon
  • S. Muto
  • J. Miyazawa
  • T. Ming
  • Y. Nakamura
  • 全て表示

6
DOI
10.1038/ncomms6816

© 2015 Macmillan Publishers Limited. All rights reserved. The driving and damping mechanism of plasma flow is an important issue because flow shear has a significant impact on turbulence in a plasma, which determines the transport in the magnetized plasma. Here we report clear evidence of the flow damping due to stochastization of the magnetic field. Abrupt damping of the toroidal flow associated with a transition from a nested magnetic flux surface to a stochastic magnetic field is observed when the magnetic shear at the rational surface decreases to 0.5 in the large helical device. This flow damping and resulting profile flattening are much stronger than expected from the Rechester-Rosenbluth model. The toroidal flow shear shows a linear decay, while the ion temperature gradient shows an exponential decay. This observation suggests that the flow damping is due to the change in the non-diffusive term of momentum transport.

リンク情報
DOI
https://doi.org/10.1038/ncomms6816
Scopus
https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84948002988&origin=inward 本文へのリンクあり
Scopus Citedby
https://www.scopus.com/inward/citedby.uri?partnerID=HzOxMe3b&scp=84948002988&origin=inward
ID情報
  • DOI : 10.1038/ncomms6816
  • eISSN : 2041-1723
  • SCOPUS ID : 84948002988

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