Figure 6 from The Relationship between Extreme Ultraviolet Non-thermal Line Broadening and High-energy Particles during Solar Flares

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The Relationship between Extreme Ultraviolet Non-thermal Line Broadening and High-energy Particles during Solar Flares

Authors: T. Kawate and S. Imada

Kawate & Imada 2013 The Astrophysical Journal 775 122.

Provider: AAS Journals

Caption: Figure 6.

Temporal evolution of the non-thermal line broadening during the intermediate flare. The color image, the green contours, and the black contours correspond to the AIA 131 (Å) intensity map, the non-thermal velocity of Fe xxiv (192.03 Å), and the AIA 1700 (Å) intensity, respectively.

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