Figure 12 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 12.

Time series of temperature maps showing spicule evolution in the non-GOL simulation (top) and the GOL simulation (bottom) in the region ﹩x=[16,25]﹩ Mm. Magnetic field is drawn with white lines (see the corresponding Movie 2).

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