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We investigate, by numerical simulations, the photometric signature ofmagnetic flux tubes in the solar photosphere. We show that the observedcontrast profiles are determined not only by the physical properties of thetube and its surroundings, but also by the peculiarities of the observations,including the line/continuum formation height and the spatial and spectralresolution. The aim is to understand these contributions well enough so thatmulti-wavelength observations can begin to disentangle them.

Photometric properties of magnetic elements: resolved and unresolved features