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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 2.

Various C II line profiles from our simulation with the position of the line center using our peak finding algorithm shown with a red vertical line: typical single-peak emission line profile (a), double-peak profile with central depression (b), profile showing three peaks (c), and absorption line profile (d).

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