Figure 5 from Quasi-periodic Counter-propagating Fast Magnetosonic Wave Trains from Neighboring Flares: SDO/AIA Observations and 3D MHD Modeling

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Quasi-periodic Counter-propagating Fast Magnetosonic Wave Trains from Neighboring Flares: SDO/AIA Observations and 3D MHD Modeling

Authors: Leon Ofman and Wei Liu

2018 The Astrophysical Journal 860 54.

Provider: AAS Journals

Caption: Figure 5.

Initial, bipolar model AR magnetic field configuration for a dipole separation of d = 2.5. An animation of the 3D magnetic field due to the impact of the QFPs is available online.

(An animation of this figure is available.)

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

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