Journal article
Stellarator impurity flux driven by electric fields tangent to magnetic surfaces
- Abstract:
- The control of impurity accumulation is one of the main challenges for future stellarator fusion reactors. The standard argument to explain this accumulation relies on the, in principle, large inward pinch in the neoclassical impurity flux caused by the typically negative radial electric field in stellarators. This simplified interpretation was proven to be flawed by Helander et al. [Phys. Rev. Lett. 118, 155002 (2017)], who showed that in a relevant regime (low-collisionality main ions and collisional impurities) the radial electric field does not drive impurity transport. In that reference, the effect of the component of the electric field that is tangent to the magnetic surface was not included. In this Letter, an analytical calculation of the neoclassical radial impurity flux incorporating such effect is given, showing that it can be very strong for highly charged impurities and that, once it is taken into account, the dependence of the impurity flux on the radial electric field reappears. Realistic examples are provided in which the inclusion of the tangential electric field leads to impurity expulsion.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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Access Document
- Files:
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(Preview, Accepted manuscript, pdf, 323.2KB, Terms of use)
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- Publisher copy:
- 10.1088/1741-4326/aae8a1
Authors
- Publisher:
- IOP Publishing
- Journal:
- Nuclear Fusion More from this journal
- Volume:
- 58
- Issue:
- 12
- Publication date:
- 2018-11-01
- Acceptance date:
- 2018-10-16
- DOI:
- EISSN:
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1741-4326
- ISSN:
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0029-5515
- Keywords:
- Pubs id:
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pubs:831671
- UUID:
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uuid:b2bf7399-0028-4b6b-8a4e-b8577507c1f6
- Local pid:
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pubs:831671
- Source identifiers:
-
831671
- Deposit date:
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2018-10-18
Terms of use
- Copyright holder:
- EURATOM
- Copyright date:
- 2018
- Notes:
- © EURATOM 2018. This is the accepted manuscript version of the article. The final version is available online from IOP at: https://doi.org/10.1088/1741-4326/aae8a1
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