Image Details

Choose export citation format:

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 3.

Flare 1 RHESSI imaging. Columns left to right: RHESSI 6–12 keV, 20–30 keV, and 50–100 keV images. Rows show different imaging algorithms, top to bottom: Pixon, CLEAN (CLEAN beamwidth = 2.2), VIS_FWDFIT, and MEM_NJIT. 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 50–100 keV emission.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse