Figure 7 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 7.

Light curves of 17 GHz microwaves (solid line), GOES (dashed line), and HXR 25–50 keV (dotted line) during the thermal-rich flare on 2011 September 25 (event (d)).

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