Author
Listed:
- T. Sunn Pedersen
(Max Planck Institute for Plasma Physics
University of Greifswald)
- M. Otte
(Max Planck Institute for Plasma Physics)
- S. Lazerson
(Princeton Plasma Physics Laboratory)
- P. Helander
(Max Planck Institute for Plasma Physics
University of Greifswald)
- S. Bozhenkov
(Max Planck Institute for Plasma Physics)
- C. Biedermann
(Max Planck Institute for Plasma Physics)
- T. Klinger
(Max Planck Institute for Plasma Physics
University of Greifswald)
- R. C. Wolf
(Max Planck Institute for Plasma Physics
Technical University Berlin)
- H. -S. Bosch
(Max Planck Institute for Plasma Physics
Technical University Berlin)
Abstract
Fusion energy research has in the past 40 years focused primarily on the tokamak concept, but recent advances in plasma theory and computational power have led to renewed interest in stellarators. The largest and most sophisticated stellarator in the world, Wendelstein 7-X (W7-X), has just started operation, with the aim to show that the earlier weaknesses of this concept have been addressed successfully, and that the intrinsic advantages of the concept persist, also at plasma parameters approaching those of a future fusion power plant. Here we show the first physics results, obtained before plasma operation: that the carefully tailored topology of nested magnetic surfaces needed for good confinement is realized, and that the measured deviations are smaller than one part in 100,000. This is a significant step forward in stellarator research, since it shows that the complicated and delicate magnetic topology can be created and verified with the required accuracy.
Suggested Citation
T. Sunn Pedersen & M. Otte & S. Lazerson & P. Helander & S. Bozhenkov & C. Biedermann & T. Klinger & R. C. Wolf & H. -S. Bosch, 2016.
"Confirmation of the topology of the Wendelstein 7-X magnetic field to better than 1:100,000,"
Nature Communications, Nature, vol. 7(1), pages 1-10, December.
Handle:
RePEc:nat:natcom:v:7:y:2016:i:1:d:10.1038_ncomms13493
DOI: 10.1038/ncomms13493
Download full text from publisher
Corrections
All material on this site has been provided by the respective publishers and authors. You can help correct errors and omissions. When requesting a correction, please mention this item's handle: RePEc:nat:natcom:v:7:y:2016:i:1:d:10.1038_ncomms13493. See general information about how to correct material in RePEc.
If you have authored this item and are not yet registered with RePEc, we encourage you to do it here. This allows to link your profile to this item. It also allows you to accept potential citations to this item that we are uncertain about.
We have no bibliographic references for this item. You can help adding them by using this form .
If you know of missing items citing this one, you can help us creating those links by adding the relevant references in the same way as above, for each refering item. If you are a registered author of this item, you may also want to check the "citations" tab in your RePEc Author Service profile, as there may be some citations waiting for confirmation.
For technical questions regarding this item, or to correct its authors, title, abstract, bibliographic or download information, contact: Sonal Shukla or Springer Nature Abstracting and Indexing (email available below). General contact details of provider: http://www.nature.com .
Please note that corrections may take a couple of weeks to filter through
the various RePEc services.