Figure 6 from Magnetohydrodynamic Simulation of the X9.3 Flare on 2017 September 6: Evolving Magnetic Topology

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Magnetohydrodynamic Simulation of the X9.3 Flare on 2017 September 6: Evolving Magnetic Topology

Authors: Chaowei Jiang, Peng Zou, Xueshang Feng, Qiang Hu, Rui Liu, P. Vemareddy, Aiying Duan, Pingbing Zuo, Yi Wang, and Fengsi Wei

2018 The Astrophysical Journal 869 13.

Provider: AAS Journals

Caption: Figure 6.

Evolution of twisted flux content. The magnetic flux content S_w of the MFR is calculated as ﹩{S}_{w}=\int | {T}_{w}{B}_{y}| {dxdz}﹩ on the surface y = 0, and the integration is limited to the area with ﹩| {T}_{w}| \gt 1﹩. The number S_w as shown is normalized by its initial value at t = 0.

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