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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 7.

QSLs on the slices shown in Figure 6(d). They are calculated based on the potential field extrapolation using the HMI full-disk vector magnetogram at 04:00 UT. (a, b) QSLs on the xz and yz planes passing through the center of the negative-polarity sunspot, respectively. A dome-like structure can be seen. (c) QSLs on the plane marked by the white box in Figure 6(d) at the height of Z ∼ 3 Mm. (d) AIA 1600 Å image taken at 04:18 UT. The green contours correspond to the QSLs in panel (c) with a level of Q = 103.

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