Line formation mechanism of the C I solar infrared multiplet at 1069.5 NM

Details Line formation mechanism of the C I solar infrared multiplet at 1069.5 NM Line formation mechanism of the C I solar infrared multiplet at 1069.5 NM

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kfnt....7...38s&link_type=openurl

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 7, July-Aug. 1991, p. 38-47. In Russian.

Physics

Infrared Spectra, Photosphere, Solar Atmosphere, Solar Spectra, Atomic Energy Levels, Chromosphere, Line Spectra

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