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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 4.

Velocity maps for the k 3 line core (top panels) and k 2 peaks (bottom panels). The color scale is clipped at −10 km s −1 and 10 km s −1 to maximize contrast. The yellow points represent locations where the detection algorithm failed to find the features. The first column shows the atmospheric velocity at the feature's τ = 1 depth. The remaining columns show the velocity shift of the feature as detected from the spectra, for spectra without noise, with noise at S/N of 5, and with noise at S/N of 5 but using a Wiener filter (see the text), respectively.

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