Fig. 4.
Observed (Cols. 1 and 3), and best fit (Cols. 2 and 4) images at wavelengths corresponding to the continuum (top), and the line centers of the two reddest IR spectral lines considered in this study. All five lines were inverted, but only the two reddest are shown. The inverted data is the version 1 data (convolved with spectra PSF and with noise added). Stokes V images correspond to wavelengths shifted by 100 mÅ to the red.
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