Figure 5 from Spectroscopic Observations of a Current Sheet in a Solar Flare

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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 Letters 853 L15.

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.

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