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Evolution of Spatial Complexity in Flare Ribbon Substructure and Its Relationship to Magnetic Reconnection Dynamics

  • Authors: Marcel F. Corchado Albelo, Maria D. Kazachenko, Ryan J. French, Vadim M. Uritsky, Emily Mason, Cole A. Tamburri, Rahul Yadav, Benjamin J. Lynch

Marcel F. Corchado Albelo et al 2026 The Astrophysical Journal 1000 .

  • Provider: AAS Journals

Caption: Figure 2.

Spatial evolution of the FRBLE boundaries and local correlation dimension (﹩{ \mathcal D }﹩) over IRIS 1330 Å SJI. Images are shown as ﹩{{\mathrm{log}}}_{10}﹩ intensity (I*; 1–104 DN; reversed gray scale). Rows (a1)–(a9), (b1)–(b9), and (c1)–(c9) show nine consecutive IRIS frames during 17:51–17:53, 17:57–18:00, and 18:15–18:18 UT, respectively. Red boxes mark the middle frames: 17:52 UT (a5), 17:58 UT (b5), and 18:16 UT (c5). Colors show ﹩{ \mathcal D }﹩ along the FRBLE: higher values (yellow; ﹩{ \mathcal D }\gt 1.5﹩) indicate more corrugated/complex segments, while lower values (blue/dark; ﹩{ \mathcal D }\leqslant 1﹩) indicate smoother segments.

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