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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 3.

Temporal variations of the microwave (a); white light (b); and soft and hard X-ray (c) fluxes. The dashed line marks the peak times of microwave and hard X-ray fluxes. The dotted line marks the peak time of the white-light emission. In panel (b), the temporal variation of the HMI 6173 Å continuum intensity measures the average intensity in the region R2 that is defined in Figure 2(f) .

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