Figure 10 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 10.

Fe xxiv intensity (erg cm ⁻² s ⁻¹ str ⁻¹ Å ⁻¹), velocity (km s ⁻¹), and non-thermal velocity (km s ⁻¹) at the peak time of the non-thermal velocity (see Figure 9) during the thermal-rich flare. Green contours represent non-thermal velocities of 100, 140, and 180 km s ⁻¹.

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