1999/06/10 by Jorge Melendez, J. Meléndez · 1 citation
Chemistry · Engineering · Physics and Astronomy · #Absorption (acoustics) #Absorption spectroscopy #Astronomy #Astrophysics #Atomic and Molecular Physics #Atomic physics #Geometry #Hyperfine structure #Infrared #Infrared spectroscopy #Laser-induced spectroscopy and plasma #Line (geometry) #Optics #Physics #Spectral line #Spectroscopy and Laser Applications #astro-ph #physics.atom-ph
paper · pdf · doi:10.1046/j.1365-8711.1999.02674.x
published as Mon.Not.Roy.Astron.Soc. 307 (1999) 197 · 7 pages (including 9 figures). MNRAS (1999) accepted. PS version also available at http://www.iagusp.usp.br/~jorge/papers/hfsmnfinal.ps
arxiv created 1999/06/10 · openalex publication_date 1999/07/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Hyperfine interaction constants and hyperfine components of Mn i lines in the near-infrared J and H bands were obtained by fitting the solar spectrum. I identified the 17744-Å solar absorption line as resulting from Mn i, and I discarded the identifications of the 13281.65-Å and 16929.85-Å solar features as a result of Fe i and Mn i, respectively.