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On the Nature of the Photospheric Horizontal Magnetic Field Increase in Major Solar Flares

  • Authors: Lijuan Liu, Zhenjun Zhou, Yuming Wang, Xudong Sun, Guoqiang Wang

Lijuan Liu et al 2022 The Astrophysical Journal Letters 934 .

  • Provider: AAS Journals

Caption: Figure 5.

(a)–(b) Scatter plots between two B h -increase parameters and IRS. The solid curve in (a) represents an exponential fitting. The dashed line represents the linear fitting. “cc” indicates the correlation coefficient. (c)–(d) Scatter plots between the parameters and flare magnitude shown for comparison.

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