Spectroscopic Observations of a Current Sheet in a Solar Flare
Authors: Y. Li, J. C. Xue, M. D. Ding, X. Cheng, Y. Su, L. Feng, J. Hong, H. Li, and W. Q. Gan
2018 The Astrophysical Journal Letters853L15.
Provider: AAS Journals
Caption: Figure 5.
Temporal evolution of the Fe XXIV line intensity (a) and nonthermal velocity (b) distributions along the three vertical slices marked in Figure 3. The black dotted line in each panel is a Gaussian fitting to the average profile, whose FWHM is given.