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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 6.

Measured experimental decay index, n, vs. numerically calculated predicted critical decay index, ﹩{n}_{\mathrm{cr}}^{}﹩, presented on a log–log plot. The represented shots are limited in edge safety factor, qa < 0.67. Eruptive shots are represented with red triangles, while noneruptive shots are blue circles. The experimental parameters, zap/xf, εa/R, and i, of each shot are fit to our numerical model to determine a value of ﹩{n}_{\mathrm{cr}}^{}﹩. The line ﹩n={n}_{\mathrm{cr}}^{}﹩ is also plotted. The model predicts that all shots above this line should be unstable, while the ones below it are stable.

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