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THE FORMATION OF IRIS DIAGNOSTICS. VI. THE DIAGNOSTIC POTENTIAL OF THE C II LINES AT 133.5 nm IN THE SOLAR ATMOSPHERE

  • Authors: Bhavna Rathore, Mats Carlsson, Jorrit Leenaarts, and Bart De Pontieu

2015 The Astrophysical Journal 811 81.

  • Provider: AAS Journals

Caption: Figure 6.

Histogram of average formation height on a ﹩\mathrm{lg}({\tau }_{0})﹩ scale (see Equation (4)) for single-peak (SP; black) and non-single-peak (NSP, red) profiles for the C II 133.4 nm line (left) and the C II 133.5 nm line (right).

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