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Cite Publication Date: Jan 1, 1994 | |
 Citations: 1 |
Affiliation: Helen Dowling Instituut, University of Oslo
We review the formation of infrared solar spectral lines from highly excited levels in neutral atoms. The lines of Mg I and H I are the most interesting ones. We explain the NLTE processes by which they are affected and we study the sensitivity of the Mg I 12 μm lines to granulation and to flux tubes.
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