Figure 2 from Two-dimensional Radiative Magnetohydrodynamic Simulations of Partial Ionization in the Chromosphere. II. Dynamics and Energetics of the Low Solar Atmosphere

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 2.

Temperature maps for the non-GOL simulation (top panel) and GOL simulation (bottom panel) reveal large differences in the thermal properties. The temperature is shown in a logarithmic scale. Magnetic field lines are drawn on the left-hand side of the temperature map in order to show clearly the temperature map on the right-hand side.

Other Images in This Article

Copyright and Terms & Conditions