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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 2.

SDO/HMI Bz magnetogram plotted over the HMI intensity map (left) and an SDO/AIA 1600 Å image taken after the peak of the X1.6 class flare (right). In both images the positive (blue) and negative (red) contours are drawn at ±200, ±500, ±800, and ±1100 G levels. The red circle represent RHESSI 12–25 keV emission drawn at the ≈50% level of the peak intensity. The yellow box outlines the FOV of the NST Hα images shown in Figures 7 and 8. The green box indicates the FOV shown in Figures 3 and 4. The images were not corrected for the projection effect.

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