Figure 4 from Diagnosing a Solar Flaring Core with Bidirectional Quasi-periodic Fast Propagating Magnetoacoustic Waves

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Diagnosing a Solar Flaring Core with Bidirectional Quasi-periodic Fast Propagating Magnetoacoustic Waves

Authors: Yuhu Miao, Dong Li, Ding Yuan, Chaowei Jiang, Abouazza Elmhamdi, Mingyu Zhao, and Sergey Anfinogentov

2021 The Astrophysical Journal Letters 908 L37.

Provider: AAS Journals

Caption: Figure 4.

Nonlinear force-free magnetic field extrapolation. Panels (a)–(f) show the magnetic field line highlighting coronal funnels FL1 and FL2 at different viewing angles. The left column uses height as a color bar to show the magnetic field lines, whereas the right column uses field strength to label color. The FOV of the magnetogram is about 340″ × 200″.

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