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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 4.

Probability distribution function (PDF) of ﹩\tau =1﹩ height at the line center determined by the line center finding algorithm as a function of the theoretical line core ﹩\tau =1﹩ height (the maximum ﹩\tau =1﹩ height over the line profile) for the C II 133.4 nm line (a) and the C II 133.5 nm line (b). Each column in the panels is scaled to maximum contrast to increase visibility. The inner green contour encompasses 50% and the outer contour encompasses 90% of all points. The red line denotes y = x. The Pearson correlation coefficient is given in the upper left corner.

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