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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 1.

Top row: SDO/AIA 171 Å images of Flare 1 (left), Flare 2 (middle), and Flare 3 (right). Pink and blue contours show the 50% intensity levels of the 6–12 keV and 50–100 keV X-ray emission, respectively. Flare ribbons observed in 1700 Å are shown by the green 50% contours for Flare 3. Bottom row: corresponding light curves for each event. The gray shaded boxes highlight the time periods studied here for each flare.

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