Figure 8 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 8.

Comparison of temporal variability of the alternative Lorentz force density ﹩{s}_{z}^{\mathrm{ad}}﹩ (a) and the Lorentz force density f_z (b) at z = 0.1. The color-coded lines indicate the ROIs (boxes 0–9) in Figure 3 in which these quantities are calculated. All units are dimensionless.

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