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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 5.

Flare 3, STIX imaging. Columns left to right: STIX 6–12 keV, 20–30 keV, and 36–74 keV images. Rows show different imaging algorithms, top to bottom: CLEAN (CLEAN beamwidth = 2.0), MEM_GE, EM, and VIS_FWDFIT_PSO. Column 1 shows a white contour of the looptop, defined as the 50% contour of the 6–12 keV emission. The white contours in Columns 2 and 3 highlight footpoints, defined as the 50% contour of the 36–74 keV emission.

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