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Laboratory Study of the Torus Instability Threshold in Solar-relevant, Line-tied Magnetic Flux Ropes

  • Authors: Andrew Alt, Clayton E. Myers, Hantao Ji, Jonathan Jara-Almonte, Jongsoo Yoo, Sayak Bose, Aaron Goodman, Masaaki Yamada, Bernhard Kliem, and Antonia Savcheva

2021 The Astrophysical Journal 908 41.

  • Provider: AAS Journals

Caption: Figure 3.

(a) Numerically calculated hoop force and (b) critical decay index as a function of zap/xf for ε = 0.5, i = 0.5, and nI = 0. Here Fh and ﹩{n}_{\mathrm{cr}}^{}﹩ have been plotted for all of the current closures shown in Figure 2, as well as for no closure, the unphysical situation where there are no return currents. The plots all begin at zap = a because below this height, part of the rope would be below z = 0 and the model breaks down. The hoop force calculations have been done numerically via the Biot–Savart law. For plots varying the other two input parameters, ε and i, see Figure 9.

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