Solar Mn I 5432/5395 Åline formation explained
- J. G. Doyle
- D. Jevremović
- C. I. Short
- P. H. Hauschildt
- W. Livingston
- I. Vince
DOIAbstract
We present a solution for the long standing problem concerning the "chromospheric"behaviour of the Mn
We present a solution for the long standing problem concerning the "chromospheric"behaviour of the Mn
Context.The Mn line at 553 nm shows strong spectral features in both intensity and polarization prof...
Taking into account effects of hyperfine structure, we calculated the synthetic solar spectrum for w...
Manganese (Mn) is a key Fe-group element, commonly employed in stellar population and nucleosynthesi...
We present a solution for the long standing problem concerning the "chromospheric"behaviour of the ...
Context.We present a detailed NLTE analysis of 39 $\ion{Mn}{i}$ lines in the solar spectrum. The inf...
There is a long-standing debate why the Mn i 5394.7 Å line in the solar irradiance spectrum brighten...
There is a long-standing debate why the Mn i 5394.7 Å line in the solar irradiance spectrum brighten...
Abstract. On the basis of NLTE profile calculations obtained by employing the radiative transfer cod...
Abstract. The Mn I 5394.7 A ̊ line is the only spectral line originating in the solar photosphere fo...
SUMMARY: Taking into account effects of hyperfine structure, we calculated the synthetic solar spect...
International audience<jats:p>Manganese (Mn) is a key Fe-group element, commonly employed in stellar...
The next generation of solar observatories aim to understand the magnetism of the solar chromosphere...
Two astrophysical problems are reviewed where non-LTE line formation for the selected atom...
Context. As a part of the long-term program at Kitt Peak National Observatory (KPNO), the Mn
International audienceThe magnetism in the quiet regions of the solar photosphere carries informatio...
Context.The Mn line at 553 nm shows strong spectral features in both intensity and polarization prof...
Taking into account effects of hyperfine structure, we calculated the synthetic solar spectrum for w...
Manganese (Mn) is a key Fe-group element, commonly employed in stellar population and nucleosynthesi...
We present a solution for the long standing problem concerning the "chromospheric"behaviour of the ...
Context.We present a detailed NLTE analysis of 39 $\ion{Mn}{i}$ lines in the solar spectrum. The inf...
There is a long-standing debate why the Mn i 5394.7 Å line in the solar irradiance spectrum brighten...
There is a long-standing debate why the Mn i 5394.7 Å line in the solar irradiance spectrum brighten...
Abstract. On the basis of NLTE profile calculations obtained by employing the radiative transfer cod...
Abstract. The Mn I 5394.7 A ̊ line is the only spectral line originating in the solar photosphere fo...
SUMMARY: Taking into account effects of hyperfine structure, we calculated the synthetic solar spect...
International audience<jats:p>Manganese (Mn) is a key Fe-group element, commonly employed in stellar...
The next generation of solar observatories aim to understand the magnetism of the solar chromosphere...
Two astrophysical problems are reviewed where non-LTE line formation for the selected atom...
Context. As a part of the long-term program at Kitt Peak National Observatory (KPNO), the Mn
International audienceThe magnetism in the quiet regions of the solar photosphere carries informatio...
Context.The Mn line at 553 nm shows strong spectral features in both intensity and polarization prof...
Taking into account effects of hyperfine structure, we calculated the synthetic solar spectrum for w...
Manganese (Mn) is a key Fe-group element, commonly employed in stellar population and nucleosynthesi...
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