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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 11.

Distribution of the acceleration diffusion coefficient D(v, z) in space, from the loop apex to chromospheric boundary, using properties of the acceleration region that produce outputs that best match observations (bold in Table 4) for three different energies, i.e., 10 keV in black, 50 keV in pink, and 80 keV in blue.

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