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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 9.

Temporal variability of the alternative Lorentz force density ﹩{s}_{z}^{\mathrm{ad}}﹩ and the individual terms (﹩{{\boldsymbol{B}}}_{h}^{2},{B}_{z}^{2}﹩) used to calculate it. For comparison, the diagram also shows fz (﹩| {\boldsymbol{j}}\times {\boldsymbol{B}}{| }_{z}﹩). These quantities are provided for the same boxes 7 (panel (a)) and 9 (panel (b)) as presented in Figure 3.

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