Figure 13 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 13.

Fe xxiv line spectra integrated over 15 × 15 arcsec ² around the peak position of the non-thermal broadening at the beginning of the thermal-rich flare (event (c), +: observations; solid line: Gaussian fitting).

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