Figure 3 from Spontaneous Current-layer Fragmentation and Cascading Reconnection in Solar Flares. I. Model and Analysis

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Spontaneous Current-layer Fragmentation and Cascading Reconnection in Solar Flares. I. Model and Analysis

Authors: Miroslav Bárta, Jörg Büchner, Marian Karlický, and Jan Skála

Bárta et al. 2011 The Astrophysical Journal 737 24.

Provider: AAS Journals

Caption: Figure 3.

Projection of the initial state ( t = 0) onto the xz-plane. Black lines represent the magnetic field lines; gray areas the magnitude of the current density: its scale is given underneath. Enhanced view of selected area (right panel) can be directly compared with the third panel in Figure 4.

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