The subtlety of the outermost stellarator magnetic surface
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arXiv
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| Format: | Preprint |
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2025
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| _version_ | 1866912659533725696 |
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| author | Punjabi, Alkesh Boozer, Allen H. |
| author_facet | Punjabi, Alkesh Boozer, Allen H. |
| contents | An analytic model of the magnetic field line behavior in a stellarator is used to study the subtlety of the concept of an outermost magnetic surface. The analytic model that we use has a central region of nested magnetic surfaces. The outermost perfectly confining surface has a toroidal flux of 0.86 of the toroidal flux of the outermost confining surface. The field lines in the annulus between these surfaces strike a distant wall, but they make tens of thousands of transits through a period of the stellarator before doing so. The number of transits is so large that this region can probably be viewed as having confining surfaces. Between the outermost confining surface and a surface at 1.02 times the toroidal flux field lines go to the walls in four flux tubes: two with inward flux and two with outward flux. One of the inward-outward pairs of flux tubes are adjoining and the other pair is separated. When the toroidal flux is greater than 1.02 of that of the outermost confining surface approximately 85% of the field lines strike the wall before transiting a single period. The loss of plasma from this region is so fast compared to cross-field plasma diffusion that they are probably irrelevant to the study of divertors. In addition to the two inward-outward flux tube pairs that escape from the region inside 1.02 times the flux of the confining region, the outer region has two new inward-outward of flux-tube pairs; one adjoining and one separated. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2510_16999 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | The subtlety of the outermost stellarator magnetic surface Punjabi, Alkesh Boozer, Allen H. Chaotic Dynamics J.2 An analytic model of the magnetic field line behavior in a stellarator is used to study the subtlety of the concept of an outermost magnetic surface. The analytic model that we use has a central region of nested magnetic surfaces. The outermost perfectly confining surface has a toroidal flux of 0.86 of the toroidal flux of the outermost confining surface. The field lines in the annulus between these surfaces strike a distant wall, but they make tens of thousands of transits through a period of the stellarator before doing so. The number of transits is so large that this region can probably be viewed as having confining surfaces. Between the outermost confining surface and a surface at 1.02 times the toroidal flux field lines go to the walls in four flux tubes: two with inward flux and two with outward flux. One of the inward-outward pairs of flux tubes are adjoining and the other pair is separated. When the toroidal flux is greater than 1.02 of that of the outermost confining surface approximately 85% of the field lines strike the wall before transiting a single period. The loss of plasma from this region is so fast compared to cross-field plasma diffusion that they are probably irrelevant to the study of divertors. In addition to the two inward-outward flux tube pairs that escape from the region inside 1.02 times the flux of the confining region, the outer region has two new inward-outward of flux-tube pairs; one adjoining and one separated. |
| title | The subtlety of the outermost stellarator magnetic surface |
| topic | Chaotic Dynamics J.2 |
| url | https://arxiv.org/abs/2510.16999 |