2018
DOI: 10.1088/1741-4326/aacb86
|View full text |Cite
|
Sign up to set email alerts
|

Observation of Marfes in the Wendelstein 7-X stellarator with inboard limiters

Abstract: In the first operational campaign of the Wendelstein 7-X (W7-X) stellarator we observed Marfe-like radiation belts at the plasma edge. We describe and analyze the behaviour of these radiation belts, especially with respect to the high density inside the belt, with a set of suitable diagnostics. We present evidence suggesting that these Marfe-like radiation belts are triggered by a drop of the edge temperature below 30 eV. From this observation we draw the conclusion that the physical cause of Marfes in tokamak… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1

Citation Types

1
2
0

Year Published

2019
2019
2022
2022

Publication Types

Select...
4
1

Relationship

3
2

Authors

Journals

citations
Cited by 5 publications
(3 citation statements)
references
References 27 publications
1
2
0
Order By: Relevance
“…The beginning of the end of the plasma features a pronounced neutral pressure spike, and an initially poloidally localized, rotating radiation belt before the plasma shrinks and extinguishes itself. This radiation belt is similar to the MARFE observed in tokamaks and it is described in detail in [31].…”
Section: Analysis Of N 2 Seeded Dischargessupporting
confidence: 77%
“…The beginning of the end of the plasma features a pronounced neutral pressure spike, and an initially poloidally localized, rotating radiation belt before the plasma shrinks and extinguishes itself. This radiation belt is similar to the MARFE observed in tokamaks and it is described in detail in [31].…”
Section: Analysis Of N 2 Seeded Dischargessupporting
confidence: 77%
“…The latter typically occurs at low plasma temperatures, where the radiative cooling coefficient is increasing with decreasing temperature (for light impurities like carbon and oxygen the relevant temperature range for this is a few hundred eV). If this happens only locally, it can lead to formation of a Marfe [10], which has also been observed in W7-X [11]. In both cases, the stored energy decreases close to the collapse since a large fraction of the heating power is lost as radiation and is, therefore, not available to the plasma.…”
Section: Introductionmentioning
confidence: 73%
“…A credible path to high performance in stellarators is to increase the plasma density. Often the achievable density, and the control of it, is limited by edge radiation instabilities that occur at low temperatures, usually referred to as MARFEs [23] and also seen in W7-X limiter operation [24]. Reducing the interaction between the edge plasma and edge neutrals often allows higher densities to be reached, and therefore localized and penetrating fueling methods such as pellets or supersonic gas injection with nozzles placed close to the last closed flux-surface are advantageous.…”
Section: Fueling and Detachmentmentioning
confidence: 99%