Figure 5 from The Relationship between Extreme Ultraviolet Non-thermal Line Broadening and High-energy Particles during Solar Flares

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 5.

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 4) during the intermediate flare. Green contours represent non-thermal velocities of 100, 140, and 180 km s ⁻¹.

Other Images in This Article

Copyright and Terms & Conditions