Fig. 9.
Degraded synthetic data. The panels illustrate data at two wavelengths of the Fe I 6301 and of 6302 Å lines. The former was degraded assuming a telescope with d1 = 1 m and the latter with a telescope aperture d2 = 0.5 m. Stokes Q, U, and V were set to zero in the 6301 line dataset in order to perform numerical experiments. Each dataset was sampled in a different spatial grid.
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