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Energetics and Emission in a Simulated Solar Flare Initialized by a Non-force-free Magnetic Field

  • Authors: W. Bate, M. Gordovskyy, A. Prasad, A. S. Brun, A. Strugarek, M. V. Sieyra, P. K. Browning, S. Inoue, K. Matsumoto, A. Roddanavar

W. Bate et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 2.

In the first panel, the Lorentz force summed in each layer of the extrapolations is shown on a log-scale as a function of height. The solid line represents the NLFF model, and the dashed line represents the non-force-free model. In the second panel, this is recast as average acceleration per layer using force and density. Both dependent variables are presented in normalized units.

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