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
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´1u+ state are also reported
Revisión por pares
SI
Version del Editor
Propietario de los Derechos
© 2020.The American Astronomical Society
Idioma
eng
Tipo de versión
info:eu-repo/semantics/acceptedVersion
Derechos
openAccess
Aparece en las colecciones
Files in questo item
La licencia del ítem se describe como Attribution-NonCommercial-NoDerivatives 4.0 Internacional