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A Statistical Study of Photospheric Magnetic Field Changes During 75 Solar Flares

  • Authors: J. S. Castellanos Durán, L. Kleint, and B. Calvo-Mozo

2018 The Astrophysical Journal 852 25.

  • Provider: AAS Journals

Caption: Figure 5.

Area corrected for foreshortening of ﹩{\rm{\Delta }}{B}_{\mathrm{LOS}}﹩ as a function of the peak GOES X-ray flux. Color-coded circles denote the center-to-limb distance μ of each event. The line is the best fit to a power law with a correlation coefficient of ﹩{r}^{2}=0.60﹩.

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