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MULTIWAVELENGTH OBSERVATIONS OF A SLOW-RISE, MULTISTEP X1.6 FLARE AND THE ASSOCIATED ERUPTION

  • Authors: V. Yurchyshyn, P. Kumar, K.-S. Cho, E.-K. Lim, and V. I. Abramenko

2015 The Astrophysical Journal 812 172.

  • Provider: AAS Journals

Caption: Figure 6.

Preflare IRIS 1330 Å slit-jaw and Hinode SOT Ca II H images showing the general structure of the flare. The green curves highlight (i) the preexisting loops (PL, panel (a)) thought to be part of the erupted fields, (ii) the expanding core fields (CF, panel (b)) that triggered the chain of events, and (iii) bright erupting fragments B1 and B2, which were also visible in the Hα line (B2, Figure 7, top panel) and the AIA channels (ELS1, Figures 9 and 11). The large red rectangle represents the FOV shown in Figures 7 and 8, while the small green box represents the FOV of Figure 4.

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