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Observations of a White-light Flare Associated with a Filament Eruption

  • Authors: Y. L. Song , Y. Guo, H. Tian, X. S. Zhu, M. Zhang, and Y. J. Zhu

2018 The Astrophysical Journal 854 64.

  • Provider: AAS Journals

Caption: Figure 9.

(a1)–(a10) AIA 335 Å images processed using the Multi-Scale Gaussian Normalization (MGN) method. (b1)–(b5) The running difference images of HMI 6173 Å continuum intensity. (c1)–(c5) The HMI LOS magnetograms. All of these images have the same FOV. The red box marks the area where white-light emission enhancement occurred. The magenta, green, and yellow contours with levels of 70% and 90% of the maximum value show the REHSSI 12–25 keV, 25–50 keV. and 50–100 keV sources, respectively.

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