Figure 1 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 1.

GOES soft X-ray fluxes and total WL flux. Red thick, blue thick, and black thin lines show 1–8 Å, 0.5–4 Å, and WL flux in our observation, respectively. The soft X-ray fluxes are in W m⁻² unit while WL flux is in arbitrary units.

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