Image Details

Choose export citation format:

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 7.

3D structure of the QSLs that wrap the erupting MFR at simulation time t = 1. (a) The isosurface of Q = 1000. (b) Sampled magnetic field lines that form the QSL. The colors denote the value of height z. A animation of the rotating view of this structure is provided in online. An animation of a moving slice crossing through the MFR in the y direction is available in Figure 8.

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

Other Images in This Article

Show More

Copyright and Terms & Conditions