Applicability of Milne-Eddington inversions to high spatial resolution observations of the quiet Sun
Context. The physical conditions of the solar photosphere change on very small spatial scales both horizontally and vertically. Such a complexity may pose a serious obstacle to the accurate determination of solar magnetic fields. Aims: We examine the applicability of Milne-Eddington (ME) inversions to high spatial resolution observations of the
Orozco Suárez, D. et al.
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2010