• español
  • English
  • français
  • Deutsch
  • português (Brasil)
  • italiano
    • español
    • English
    • français
    • Deutsch
    • português (Brasil)
    • italiano
    • español
    • English
    • français
    • Deutsch
    • português (Brasil)
    • italiano
    JavaScript is disabled for your browser. Some features of this site may not work without it.

    Browse

    All of UVaDOCCommunitiesBy Issue DateAuthorsSubjectsTitles

    My Account

    Login

    Statistics

    View Usage Statistics

    Share

    View Item 
    •   UVaDOC Home
    • SCIENTIFIC PRODUCTION
    • Departamentos
    • Dpto. Química Física y Química Inorgánica
    • DEP63 - Artículos de revista
    • View Item
    •   UVaDOC Home
    • SCIENTIFIC PRODUCTION
    • Departamentos
    • Dpto. Química Física y Química Inorgánica
    • DEP63 - Artículos de revista
    • View Item
    • español
    • English
    • français
    • Deutsch
    • português (Brasil)
    • italiano

    Export

    RISMendeleyRefworksZotero
    • edm
    • marc
    • xoai
    • qdc
    • ore
    • ese
    • dim
    • uketd_dc
    • oai_dc
    • etdms
    • rdf
    • mods
    • mets
    • didl
    • premis

    Citas

    Por favor, use este identificador para citar o enlazar este ítem:http://uvadoc.uva.es/handle/10324/42802

    Título
    Line Oscillator Strengths for the c4′ 1Σu +(4)–X1Σg +(0–7) Absorption Bands of N2
    Autor
    Velasco Sanz, Ana MaríaAutoridad UVA Orcid
    Lavín Puente, María del CarmenAutoridad UVA Orcid
    Año del Documento
    2020
    Editorial
    The American Astronomical Society
    Descripción
    Producción Científica
    Documento Fuente
    The Astrophysical Journal, 2020, Volume 899, Number 1
    Abstract
    Theoretical absorption oscillator strengths for rotational lines of the¢S+c441u()–S+X1g(0–7)bands of N2, which arerelevant to analyze the spectra of the atmospheres of the Earth, Titan, and Mars, are reported. The knowninteraction between the¢S+c441u()andP+c431u()Rydberg states and the¢S+b131u()valence state has been dealtwith through an appropriate rovibronic energy matrix. Deviations in the intensity distribution of the rotational linesfrom considerations based on Hönl–London factors have been found for each of the studied bands. Emissionbranching ratios for the above bands and lifetimes of the rotational levels of v=4 level of the c4´1u+ state are also reported
    Revisión por pares
    SI
    DOI
    10.3847/1538-4357/aba049
    Version del Editor
    https://iopscience.iop.org/article/10.3847/1538-4357/aba049
    Propietario de los Derechos
    © 2020.The American Astronomical Society
    Idioma
    eng
    URI
    http://uvadoc.uva.es/handle/10324/42802
    Tipo de versión
    info:eu-repo/semantics/acceptedVersion
    Derechos
    openAccess
    Collections
    • DEP63 - Artículos de revista [223]
    Show full item record
    Files in this item
    Nombre:
    LINE-OSCILLATOR-AAS21265_.pdf
    Tamaño:
    439.8Kb
    Formato:
    Adobe PDF
    Thumbnail
    FilesOpen
    Attribution-NonCommercial-NoDerivatives 4.0 InternacionalExcept where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivatives 4.0 Internacional

    Comentarios

    Universidad de Valladolid

    Powered by MIT's. DSpace software, Version 5.10