자료유형 | 학위논문 |
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서명/저자사항 | The Role of Three-Dimensional Geometry on Turbulence in Quasi-Helically Symmetric Stellarators. |
개인저자 | Faber, Benjamin J. |
단체저자명 | The University of Wisconsin - Madison. Physics. |
발행사항 | [S.l.]: The University of Wisconsin - Madison., 2018. |
발행사항 | Ann Arbor: ProQuest Dissertations & Theses, 2018. |
형태사항 | 207 p. |
기본자료 저록 | Dissertation Abstracts International 79-12B(E). Dissertation Abstract International |
ISBN | 9780438269040 |
학위논문주기 | Thesis (Ph.D.)--The University of Wisconsin - Madison, 2018. |
일반주기 |
Source: Dissertation Abstracts International, Volume: 79-12(E), Section: B.
Advisers: Chris C. Hegna |
요약 | The ability to optimize stellarator geometry to reduce transport has led to renewed interest in stellarators for magnetic confinement fusion. In this thesis, turbulence in the Helically Symmetric eXperiment (HSX), a quasi-helically symmetric ste |
요약 | The first comprehensive simulations of Trapped Electron Mode turbulence in HSX are presented. HSX geometry introduces a complex landscape of unstable eigenmodes, with strongly ballooning modes, non-symmetric modes, and extended modes all coexist |
요약 | These linear and nonlinear features are the consequence of the low global magnetic shear of HSX, which allows modes to extend far along field lines and requires simulation domains spanning multiple poloidal turns to properly resolve. Subdominant |
일반주제명 | Plasma physics. Physics. |
언어 | 영어 |
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: 이 자료의 원문은 한국교육학술정보원에서 제공합니다. |