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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 6.

Initial state of the model AR variables, showing a cut in the xz plane at y = 0 for the 3D dipole magnetic field with d = 2.5. (a) Initial density, ρ, and selected magnetic field lines. (b) Initial fast magnetosonic speed, Vf. The color map and contours show the spatial dependence of Vf. (c) Initial normalized background temperature, T. (d) Initial values of plasma β.

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