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• W3106016122 abstract "Context. The magnetic topology of the solar photosphere in its quietest regions is hidden by the difficulties to disentangle magnetic flux through the resolution element from the field strength of unresolved structures. The observation of spectral lines with strong coupling with hyperfine structure, like the observed Mn i line at 553.7 nm, allows such differentiation." @default.
• W3106016122 created "2020-11-23" @default.
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• W3106016122 date "2008-06-24" @default.
• W3106016122 modified "2023-10-18" @default.
• W3106016122 title "Strength distribution of solar magnetic fields in photospheric quiet Sun regions" @default.
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• W3106016122 doi "https://doi.org/10.1051/0004-6361:20078654" @default.
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