Figure 8 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

Kawate & Imada 2013 The Astrophysical Journal 775 122.

Caption: Figure 8.

Example of the Fe xxiv line profile integrated over the EIS FOV during the thermal-rich flare (+: observations; solid line: Gaussian fitting).