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RAPID PENUMBRA AND LORENTZ FORCE CHANGES IN AN X1.0 SOLAR FLARE

  • Authors: Zhe Xu, Yunchun Jiang, Jiayang Yang, Bo Yang, Yi Bi, and Shunping Yu

2016 The Astrophysical Journal Letters 820 L21.

  • Provider: AAS Journals

Caption: Figure 3.

Time profiles of ((a1) and (a2)) the mean intensities, ((b1) and (b2)) mean vertical and horizontal fields, ((c1) and (c2)) field inclination angles, and ((d1) and (d2)) vertical LF changes, measured from HMI intensity images and vector magnetograms over E and D as shown in Figure 2. Time profile of the GOES 1–8 Å SXR flux is overplotted as the orange curves in an arbitrary unit to fit the panels.

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