Figure 12 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 12.

Relationships among the location of the flare loop (AIA 131 Å: image), the non-thermal line broadening (EIS Fe xxiv: green contours), microwaves (NoRH 17 GHz: red contours), and the flare ribbon (AIA 1700 Å: black contours) at the non-thermal peak of the flares.

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