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Influence of construction errors on Wendelstein 7-X magnetic configurations

Author
ANDREEVA, T1 ; BRAUER, T1 ; ENDLER, M1 ; KISSLINGER, J2 ; TOUSSAINT, U. V2
[1] Max-Planck-Institut für Plasmaphysik, EURATOM Association, Teilinstitut Greifswald, Wendelsteinstrasse 1, 17491 Greifswald, Germany
[2] Max-Planck Institut für Plasmaphysik. EURATOM Association. Boltzmannstr. 2, 85748, Garching, Germany
Conference title
Proceedings of the 25th Symposium on Fusion Technology (SOFT-25)
Conference name
Symposium on Fusion Technology (SOFT-25) (SOFT-25) (25 ; Rostock 2008-09-15)
Author (monograph)
ZOHM, Hartmut (Editor)1
Max-Planck-Institut für Plasmaphysik (IPP), Germany (Organiser of meeting)
[1] Max-Planck-Institut für Plasmaphysik, 85748 Garching, Germany
Source

Fusion engineering and design. 2009, Vol 84, Num 2-6, pp 408-412, 5 p ; ref : 3 ref

CODEN
FEDEEE
ISSN
0920-3796
Scientific domain
Energy; Metallurgy, welding
Publisher
Elsevier, Amsterdam
Publication country
Netherlands
Document type
Conference Paper
Language
English
Author keyword
Construction uncertainties Magnetic field perturbation Stellarator Wendelstein 7-X
Keyword (fr)
Bobine supraconductrice Champ magnétique Plasma Réacteur fusion nucléaire Stellarator
Keyword (en)
Superconducting coils Magnetic field Plasma Nuclear fusion reactor Stellarator
Keyword (es)
Campo magnético Plasma Reactor fusión nuclear Estelarator
Classification
Pascal
001 Exact sciences and technology / 001D Applied sciences / 001D06 Energy / 001D06D Energy. Thermal use of fuels / 001D06D04 Installations for energy generation and conversion: thermal and electrical energy. / 001D06D04E Controled nuclear fusion plants

Discipline
Energy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
21921582

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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