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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 2.

Shifted-circle model and different current closure options that are considered. The axis of the flux rope is approximated by the solid blue circle, which has foot points fixed at x = ± xf and apex height zap. Given xf and zap, the radius of curvature, Rsc; center of curvature, zsc; and angle, ϕf, can be determined, making this a 1D model with a single parameter, zap. The dashed curves represent different potential paths that the return current can take below the solar surface at z = 0. The return currents (dashed lines) shown are either fixed paths or a dynamic image current (purple). The fixed paths are horizontal closure between the foot points (red), vertical paths off to z → −∞ (yellow), a fixed semicircular path (green), and a full circle (cyan).

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