Figure 1 from THE FORMATION OF IRIS DIAGNOSTICS. VI. THE DIAGNOSTIC POTENTIAL OF THE C II LINES AT 133.5 nm IN THE SOLAR ATMOSPHERE

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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 1.

Temperature (a), total hydrogen population density (b), and column mass (c) as a function of height along a 2D cutout at ﹩x=12\;\mathrm{Mm}﹩ from the 3D model atmosphere. The maximum height across the line profile of ﹩{\tau }_{\nu }=1﹩ is shown for the C II 133.5 nm (red) and C II 133.4 nm (blue) lines.

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