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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 9.

Numerically predicted critical decay indices for solar applications as a function of normalized apex height, plotted for different values of ε and i. The plots here are chosen to be most applicable to solar conditions with an image current closure and toroidal current decay index of nI = 0.5. (a) ﹩{n}_{\mathrm{cr}}^{}({z}_{\mathrm{ap}}/{x}_{{\rm{f}}})﹩ for different values of ε at fixed i = 0.5. (b) ﹩{n}_{\mathrm{cr}}^{}({z}_{\mathrm{ap}}/{x}_{{\rm{f}}})﹩ for different values of i at fixed ε = 0.5. The minimum value of zap/xf where the MFR would pass below z = 0 is also shown for this plot.

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