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The Formation of IRIS Diagnostics. III. Near-ultraviolet Spectra and Images

  • Authors: T. M. D. Pereira, J. Leenaarts, B. De Pontieu, M. Carlsson, and H. Uitenbroek

Pereira et al. 2013 The Astrophysical Journal 778 143.

  • Provider: AAS Journals

Caption: Figure 2.

Effects of IRIS spatial and spectral resolution and noise on the NUV spectrum near the Mg ii k line. The original spectrum was taken from a single simulation pixel. This pixel was brighter than its surroundings and was chosen so that the Mg ii k intensity was similar to the mean observed value. The S/N is measured at the last wavelength shown (280.042 nm). For clarity, spectra of different S/Ns are offset 0.25 nW m −2 Hz −1 sr −1 from each other.

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