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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 7.

Median values of the absolute difference between quantities derived from spectra with and without noise, for bins in the quantities in the x axes. We show results for different S/Ns, as per the legend. The dashed lines of the same color (only shown for S/Ns of 2, 5, and 10) show the results for the noisy spectra when a Wiener filter was applied (see the text). Top panel: effect of noise on the k 3 velocity shifts, middle panel: effect of noise on the k 2 peak separation, and bottom panel: effect of noise on the k 2 V radiation temperature.

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