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Gyrofluid Turbulence Modelling of the Linear Device VINETA

MPS-Authors
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Kervalishvili,  G. N.
Stellarator Theory (ST), Max Planck Institute for Plasma Physics, Max Planck Society;

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Kleiber,  R.
Stellarator Theory (ST), Max Planck Institute for Plasma Physics, Max Planck Society;

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Schneider,  R.
Helmholtz Junior Research Group 'Computational Material Science' (Junior Research Group HFG-Greifswald), Max Planck Institute for Plasma Physics, Max Planck Society;
Stellarator Theory (ST), Max Planck Institute for Plasma Physics, Max Planck Society;

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Scott,  B. D.
Tokamak Theory (TOK), Max Planck Institute for Plasma Physics, Max Planck Society;

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Grulke,  O.
VINETA, Max Planck Institute for Plasma Physics, Max Planck Society;
Stellarator Scenario Development (E5), Max Planck Institute for Plasma Physics, Max Planck Society;

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Windisch,  T.
VINETA, Max Planck Institute for Plasma Physics, Max Planck Society;
Stellarator Scenario Development (E5), Max Planck Institute for Plasma Physics, Max Planck Society;

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Citation

Kervalishvili, G. N., Kleiber, R., Schneider, R., Scott, B. D., Grulke, O., & Windisch, T. (2006). Gyrofluid Turbulence Modelling of the Linear Device VINETA. Contributions to Plasma Physics, 46, 739-743. Retrieved from http://www3.interscience.wiley.com/cgi-bin/fulltext/112770568/PDFSTART.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0027-0EAB-9
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