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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 5.

Evolution of the magnetic field and electric current density. The evolution of the magnetic field components By(a), Bh(b), Bx(c), and the current density ﹩-{j}_{z}(d)﹩ from ﹩t=164{t}_{{\rm{A}}}﹩ to ﹩t=244{t}_{{\rm{A}}}﹩. The color-coded lines indicated ROIs (boxes 0–9) in Figure 3, in which these quantities are calculated. The same colors were used to identify the arrows that mark the minima of Bh and −jz.

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