Cargando…

OH in the Solar Spectrum

Revised identifications of OH lines in the solar spectrum have been made from the detailed laborarory analyses of the A (2)Σ(+)−X(2)∏ bands. In the (0, 0), (1, 1), and (2, 2) bands a total of 175 solar lines are ascribed to OH unblended; 124 have OH as a partial contributor. Laboratory intensities a...

Descripción completa

Detalles Bibliográficos
Autores principales: Moore, Charlotte E., Broida, Herbert P.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: [Gaithersburg, MD] : U.S. Dept. of Commerce, National Institute of Standards and Technology 1959
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5287041/
https://www.ncbi.nlm.nih.gov/pubmed/31216137
http://dx.doi.org/10.6028/jres.063A.023
_version_ 1782504096694009856
author Moore, Charlotte E.
Broida, Herbert P.
author_facet Moore, Charlotte E.
Broida, Herbert P.
author_sort Moore, Charlotte E.
collection PubMed
description Revised identifications of OH lines in the solar spectrum have been made from the detailed laborarory analyses of the A (2)Σ(+)−X(2)∏ bands. In the (0, 0), (1, 1), and (2, 2) bands a total of 175 solar lines are ascribed to OH unblended; 124 have OH as a partial contributor. Laboratory intensities along the branches of the separate bands have been used as a guide in making the solar identifications.
format Online
Article
Text
id pubmed-5287041
institution National Center for Biotechnology Information
language English
publishDate 1959
publisher [Gaithersburg, MD] : U.S. Dept. of Commerce, National Institute of Standards and Technology
record_format MEDLINE/PubMed
spelling pubmed-52870412019-06-18 OH in the Solar Spectrum Moore, Charlotte E. Broida, Herbert P. J Res Natl Bur Stand A Phys Chem Article Revised identifications of OH lines in the solar spectrum have been made from the detailed laborarory analyses of the A (2)Σ(+)−X(2)∏ bands. In the (0, 0), (1, 1), and (2, 2) bands a total of 175 solar lines are ascribed to OH unblended; 124 have OH as a partial contributor. Laboratory intensities along the branches of the separate bands have been used as a guide in making the solar identifications. [Gaithersburg, MD] : U.S. Dept. of Commerce, National Institute of Standards and Technology 1959 1959-12-01 /pmc/articles/PMC5287041/ /pubmed/31216137 http://dx.doi.org/10.6028/jres.063A.023 Text en https://creativecommons.org/publicdomain/zero/1.0/ The Journal of Research of the National Bureau of Standards Section A is a publication of the U.S. Government. The papers are in the public domain and are not subject to copyright in the United States. Articles from J Res may contain photographs or illustrations copyrighted by other commercial organizations or individuals that may not be used without obtaining prior approval from the holder of the copyright.
spellingShingle Article
Moore, Charlotte E.
Broida, Herbert P.
OH in the Solar Spectrum
title OH in the Solar Spectrum
title_full OH in the Solar Spectrum
title_fullStr OH in the Solar Spectrum
title_full_unstemmed OH in the Solar Spectrum
title_short OH in the Solar Spectrum
title_sort oh in the solar spectrum
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5287041/
https://www.ncbi.nlm.nih.gov/pubmed/31216137
http://dx.doi.org/10.6028/jres.063A.023
work_keys_str_mv AT moorecharlottee ohinthesolarspectrum
AT broidaherbertp ohinthesolarspectrum