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  4. Drift Stabilisation of Ballooning Modes in an Inward-Shifted LHD Configuration
 
conference paper

Drift Stabilisation of Ballooning Modes in an Inward-Shifted LHD Configuration

Cooper, W. A.  
•
Brocher, L.
•
Graves, J. P.
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2010
Contributions To Plasma Physics
17th International Stellarator/Heliotron Workshop

A drift-magnetohydrodynamic theory is applied to a background anisotropic pressure equilibrium state to generate a drift corrected ballooning mode equation. The ratio of the mode frequency to the hot particle drift frequency constitutes the critical expansion parameter. The fast particles thus contribute weakly to the instability driving mechanism and also to the diamagnetic drift stabilisation. This equation is used to model the inward-shifted Large Helical Device (LHD) configuration. In the single-fluid limit, a weakly ballooning unstable band that encompasses a third of the plasma volume develops in the core of the plasma at low <beta(dia)> that becomes displaced towards the edge of the plasma at the experimentally achieved <beta(dia)> similar or equal to 5%. Finite diamagnetic drifts (mainly due to the thermal ions) effectively stabilise these ballooning structures at all values of <beta(dia)>. The validity of the large hot particle drift approximation is verified for hot to thermal ion density ratios that remain smaller than 2%. (C) 2010 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

  • Details
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Type
conference paper
DOI
10.1002/ctpp.200900501
Web of Science ID

WOS:000280985400005

Author(s)
Cooper, W. A.  
Brocher, L.
Graves, J. P.
Cooper, G. A.
Narushima, Y.
Watanabe, K. Y.
Date Issued

2010

Published in
Contributions To Plasma Physics
Volume

50

Start page

713

End page

717

Subjects

Drift magnetohydrodynamics

•

ballooning

•

diamagnetic

•

Lhd

•

Stability

Editorial or Peer reviewed

NON-REVIEWED

Written at

EPFL

EPFL units
CRPP  
SPC  
Event nameEvent placeEvent date
17th International Stellarator/Heliotron Workshop

Princeton, NJ

Oct 12-16, 2009

Available on Infoscience
December 16, 2011
Use this identifier to reference this record
https://infoscience.epfl.ch/handle/20.500.14299/75274
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