Figure 9 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 9.

Temporal evolution of the thermal-rich flare event (horizontal line: Fe xxiv full-FOV non-thermal velocity estimated from integrated line profile over the EIS FOV; solid line: Fe xxiv full-FOV intensity integrated from 191.90 to 192.15 Å; dotted line: 17 GHz microwaves).

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