Figure 5 from TEMPORAL EVOLUTION AND SPATIAL DISTRIBUTION OF WHITE-LIGHT FLARE KERNELS IN A SOLAR FLARE

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TEMPORAL EVOLUTION AND SPATIAL DISTRIBUTION OF WHITE-LIGHT FLARE KERNELS IN A SOLAR FLARE

Authors: T. Kawate, T. T. Ishii, Y. Nakatani, K. Ichimoto, A. Asai, S. Morita, and S. Masuda

2016 The Astrophysical Journal 833 50.

Provider: AAS Journals

Caption: Figure 5.

Maps of temporal evolution of WL emission. (a) Peak time t_pk of WL (colored dots). (b) Peak intensity of WL ﹩[{I}_{\max }﹩ ﹩(\mathrm{WL})-{I}_{\mathrm{BG}}﹩(WL)]/I_QS(WL) (colored dots). The grayscale background is the preflare WL intensity map at 22:10:00 UT. The thick, black dotted curve shows the magnetic neutral line.

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