Figure 10 from A Statistical Study of Photospheric Magnetic Field Changes During 75 Solar Flares

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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 10.

Typical stepwise change (black diamonds) that is well fitted by Equation (1) (red line). The blue line is the GOES light curve, and the dashed lines represent the start and end GOES times (from the flare database). 2c is −463 Mx cm⁻², while our method found a step size of −213 Mx cm⁻².

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