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Fig. 2.


Observed and synthetic IRIS and ALMA spectra. Averaged continuum at 2800 (±0.1) Å (panel a: observed, panel b: synthetic from IRIS fit, and panel c: synthetic from IRIS+ALMA fit), averaged k core wavelengths (panel d: observed, panel e: synthetic from IRIS fit, and panel f: synthetic from IRIS+ALMA fit), and 1.25 mm continuum (panel g: observed, panel h: prediction from IRIS fit, and panel i: synthetic from IRIS+ALMA fit). The color bars are in units of kiloKelvin. The panels on the right show examples of observed and synthetic IRIS spectra (arbitrary y-scale) at selected locations. The insets show the core of the Ni I line.

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