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Constraining Turbulent Solar Flare Acceleration Regions by Connecting Kinetic Modeling and X-Ray Observations

  • Authors: Morgan Stores, Natasha Jeffrey, Ewan Dickson, James McLaughlin, Eduard Kontar

Morgan Stores et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 8.

Observed photon flux spectrum of Flare 2 (black) compared to the simulated photon flux spectrum (blue) for simulations using n = 7 × 1010, 36 × 1010, and 43 × 1010 cm−3, shown by the blue, yellow, and pink curves, respectively.

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