2021
DOI: 10.1088/1361-6587/ac031b
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Low n electromagnetic modes in spherical tokamaks

Abstract: The performance of spherical tokamak reactors depends on plasma β, and an upper limit is set by long-wavelength kinetic ballooning modes (KBMs). We examine how these modes become unstable in spherical-tokamak reactor relevant plasmas, which may contain significant fast-ion pressure. In a series of numerically generated equilibria of increasing β, the KBM becomes unstable at sufficiently high plasma β, and for such cases, it is also significantly unstable even in the long-wavelength limit. The β threshold for t… Show more

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Cited by 3 publications
(2 citation statements)
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“…Two species were simulated, a thermal deuterium and electron species. It should be highlighted that no fast ions were included in this work, but must be examined in future work as they may have a significant impact on the micro-stability [20,21]. Furthermore, the impact of including tritium and impurities is also left as future work.…”
Section: Numerical Setupmentioning
confidence: 99%
“…Two species were simulated, a thermal deuterium and electron species. It should be highlighted that no fast ions were included in this work, but must be examined in future work as they may have a significant impact on the micro-stability [20,21]. Furthermore, the impact of including tritium and impurities is also left as future work.…”
Section: Numerical Setupmentioning
confidence: 99%
“…The gradient in the plasma profile can drive several temperature and density gradient instabilities, such as ITG [6,[27][28][29][30], trapped electron mode (TEM) [31,32], universal drift modes [33,34] etc which are electrostatic in nature. Similar profile gradients may also produce electromagnetic instabilities such as kinetic ballooning mode (KBM) [35][36][37][38][39][40] and micro tearing mode [41][42][43][44][45] if the plasma β is high [46,47]. In the present study, the core plasma beta β = 2µ 0 n 0e T 0e /B 2 0 , where T 0e , n 0e and B 0 are the on-axis electron temperature, density and the magnetic field strength with the values of n 0e = 2.3 × 10 19 m −3 , T 0e = 250 eV and B 0 = 1.0 T is approximately 0.1%.…”
Section: Linear Gyrokinetic Simulations With Orb5 and Glogystomentioning
confidence: 99%