Figure 4 from Two-dimensional Radiative Magnetohydrodynamic Simulations of Partial Ionization in the Chromosphere. II. Dynamics and Energetics of the Low Solar Atmosphere

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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 4.

Median (left panels) and standard deviation (right panels) of the kinetic energy (averaged over 11 minutes, snapshots = [300–370]) for the non-GOL (top panels) and GOL simulations (bottom panels), for ﹩x=[0\mbox{--}40]﹩ Mm.

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