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Two-dimensional Radiative Magnetohydrodynamic Simulations of Partial Ionization in the Chromosphere. II. Dynamics and Energetics of the Low Solar Atmosphere

  • Authors: Juan Martínez-Sykora, Bart De Pontieu, Mats Carlsson, Viggo H. Hansteen, Daniel Nóbrega-Siverio, and Boris V. Gudiksen

2017 The Astrophysical Journal 847 36.

  • Provider: AAS Journals

Caption: Figure 9.

Total vertical Poynting flux of the advection term for the non-GOL (black) and GOL simulations (green) as a function of height. All values are averaged in time (over 1.5 minutes, snapshots = [360–370]) and in the horizontal direction. The vertical Poynting flux due to the ambipolar diffusion in the GOL simulation (red) is shown as a function of height. The dashed line is for horizontal motions (﹩{{P}_{z}}_{h}﹩), the dotted line is for vertical motions (﹩{{P}_{z}}_{z}﹩) and the solid line is the sum of both.

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