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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 8.

Velocity maps for three photospheric heights, showing the atmospheric vertical velocity v z at a given geometrical height and the mean velocity shifts Δ v derived from several photospheric lines. The color scale is clipped at −3 km s −1 and 3 km s −1 to maximize contrast. The middle panels shows Δ v when no noise was applied on the spectra and the right panels show the same quantity when Poisson noise was added with a S/N of 10 and a Wiener filter was used on the data (see the text).

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