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Observation
and modeling of selected manganese lines in solar spectrum
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| Figure 1. The
average over solar disk spectrum near the Mn I 543.2 nm spectral
line (a) and the Mn I 543.2 nm spectral line profiles for different
heliocentric angles (b)
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Figures 2. Center-to-limb variation of the observed
and calculated (circles - with hyperfine components, squares - without
hyperfine components) parameters of the Mn I 543.2 nm spectral line
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| Telescopes Instrumentation |
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| Activities80-cm Telescope |
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