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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 7.

The green, red, and purple lines show the synthetic 94 Å light curves for both of the simulations, with density scaling factors corresponding to density at the upper domain boundary of ρt = 2 × 108, 9 × 108,  and 1010 cm−3, respectively. The solid lines corresponds to the non-force-free case, and the dashed lines to the NLFF case. The blue line shows the measured AIA 94 Å light curve.

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