Figure 2 from Flare Reconnection-driven Magnetic Field and Lorentz Force Variations at the Sun’s Surface

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Flare Reconnection-driven Magnetic Field and Lorentz Force Variations at the Sun’s Surface

Authors: Krzysztof Barczynski, Guillaume Aulanier, Sophie Masson, and Michael S. Wheatland

2019 The Astrophysical Journal 877 67.

Provider: AAS Journals

Caption: Figure 2.

Evolution of the magnetic field (a) and electric current density (b) with height in the solar atmosphere from z = 0.0 to z = 1.0. The plots present the vector components (color-coded squares) during the eruption (﹩t=208{t}_{{\rm{A}}}﹩) at ﹩[x;y]=[-0.6;0.2]﹩. The dashed line marks z = 0.1.

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