Figure 7 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 7.

Histogram of the absolute value of the ambipolar velocity (﹩| {u}_{\mathrm{amb}}| ﹩), integrated over 11 minutes (snapshots = [300–370]), revealing a two-step power law (with a slope of −0.07 at low ambipolar velocities and −0.2 at high ambipolar velocities).

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