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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 7.

Vertical component of the alternative Lorentz force density changes (﹩\delta {s}_{z}^{\mathrm{ad}}﹩) at three different times during the eruption phase. The change in ﹩{s}_{z}^{\mathrm{ad}}﹩ is defined by the color code. Arrows and electric current density contours are the same as in Figure 4. The animation begins at ﹩t=164{t}_{A}﹩ and ends at ﹩t=244{t}_{A}﹩.

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

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