Figure 5 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 5.

Magnetic free energy normalized by the magnetic energy of the potential field extrapolated from z = 0 Mm for the GOL (dashed) and non-GOL simulations (solid) integrated over 11 minutes (snapshots = [300–370]).

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