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Field-aligned and Magnetic Reconnection Flows in a Magnetohydrodynamic Simulation of Prominence-cavity System

  • Authors: Tie Liu, Yingna Su, Yang Guo, Jie Zhao, Haisheng Ji

Tie Liu et al 2023 The Astrophysical Journal 949 .

  • Provider: AAS Journals

Caption: Figure 2.

Height–time plot of the erupted MFR. The red “+” represents the evolution of the apex of the MFR axis, which is fitted by the function ﹩h(t)={c}_{0}{e}^{({\rm{t}}-{{\rm{t}}}_{0})/\tau }+{c}_{1}(t-{t}_{0})+{c}_{2}﹩ (blue curve). The three red-dashed vertical lines mark the boundaries of the four evolution phases and the three green-dashed vertical lines mark the times of the snapshots shown in Figure 3.

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