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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 10.

Temporal evolution of physical variables at x = 1.2, y = 0, z = 3.5 with symmetric excitation of QFPs at x1,2 = ±2.0 (Case 1). The time is in units of τA = 11.9 s. (a) Velocity components Vx (solid), Vy (dashed), and Vz (dotted). (b) Perturbed magnetic field components ΔBx (solid), ΔBy (dashed), and ΔBz (dotted). (c) Density (solid) and temperature (dashed) perturbations, Δρ and ΔT.

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