2017
DOI: 10.1088/1741-4326/aa958b
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A multi-machine scaling of halo current rotation

Abstract: Halo currents generated during unmitigated tokamak disruptions are known to develop rotating asymmetric features that are of great concern to ITER because they can dynamically amplify the mechanical stresses on the machine. This paper presents a multi-machine analysis of these phenomena. More specifically, data from C-Mod, NSTX, ASDEX Upgrade, DIII-D, and JET are used to develop empirical scalings of three key quantities: (1) the machine-specific minimum current quench time, τ CQ ; (2) the halo current rotatio… Show more

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Cited by 23 publications
(43 citation statements)
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References 50 publications
(115 reference statements)
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“…Following the analysis in Myers et al. (2018), the expected number of full toroidal rotations of a halo current asymmetry can be calculated using multi-machine scalings of the rotation frequency and the halo current rotation duration. The rotation scaling from Myers et al.…”
Section: Disruption Dynamics and Loadingmentioning
confidence: 99%
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“…Following the analysis in Myers et al. (2018), the expected number of full toroidal rotations of a halo current asymmetry can be calculated using multi-machine scalings of the rotation frequency and the halo current rotation duration. The rotation scaling from Myers et al.…”
Section: Disruption Dynamics and Loadingmentioning
confidence: 99%
“…The radial field produced by the poloidal field coil system during the plasma flattop is calculated and the maximum vertical excursion of a full current plasma with a flat q = 1 profile is estimated to be |ΔZ| ≈ 0.5 m. The radial field averaged over the displaced plasma is B R ≈ 0.5 T, giving FIGURE 9. Projected non-axisymmetric halo current behaviour in terms of rotation duration versus rotation count, as scaled from the tokamak database in Myers et al (2018). The plot is presented in a way that facilitates direct comparison with the ITER projection in that reference, where the shaded parallelogram and its unshaded extension represent the projected rotation ranges for the lower and upper bounds of the minimum CQ time, respectively.…”
Section: Vertical Displacement Events and Halo Currentsmentioning
confidence: 99%
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