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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 6.

PDFs for the gas temperature at an optical depth of unity being T gas when the observed k 2 V (top) and k 2 R (bottom) radiation temperatures are T rad, extracted from spectra convolved with the instrumental profile of IRIS (grayscale; darker means more frequent) and for the original spectra (cyan contours). The red line denotes y = x.

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