Figure 9 from The Formation of IRIS Diagnostics. III. Near-ultraviolet Spectra and Images

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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 9.

PDFs for the atmospheric vertical velocity being v _z when the observed velocity shifts derived from photospheric lines are Δ v, at different depths and combining all snapshots. Darker means more frequent. The diagonal red lines depict y = x; the cyan lines depict the zero velocities.

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