A far wing lineshape for H2 broadened CH4 infrared transitions

Jean Michel Hartmann; Christian Boulet; Claude Brodbeck; Nguyen Van Thanh; Thierry Fouchet; Pierre Drossart

doi:10.1016/S0022-4073(01)00058-9

A far wing lineshape for H₂ broadened CH₄ infrared transitions

Jean Michel Hartmann
, Christian Boulet
, Claude Brodbeck
, Nguyen Van Thanh
, Thierry Fouchet
, Pierre Drossart

CNRS
Sorbonne Univ.

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

Résumé

A far wing corrective factor _X for CH₄ lines broadened by H₂ is proposed. It has been deduced from laboratory spectra measured in the v₃ band region at various temperatures between 100 and 300 K. Its quality is demonstrated by comparisons of synthetic spectra with laboratory experiments as well as with the spectrum of the jovian atmosphere observed by ISO.

langue originale	Anglais
Pages (de - à)	117-122
Nombre de pages	6
journal	Journal of Quantitative Spectroscopy and Radiative Transfer
Volume	72
Numéro de publication	2
Les DOIs	https://doi.org/10.1016/S0022-4073(01)00058-9
état	Publié - 15 janv. 2002

Accès au document

10.1016/S0022-4073(01)00058-9

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Contient cette citation

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title = "A far wing lineshape for H2 broadened CH4 infrared transitions",

abstract = "A far wing corrective factor X for CH4 lines broadened by H2 is proposed. It has been deduced from laboratory spectra measured in the v3 band region at various temperatures between 100 and 300 K. Its quality is demonstrated by comparisons of synthetic spectra with laboratory experiments as well as with the spectrum of the jovian atmosphere observed by ISO.",

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AU - Hartmann, Jean Michel

AU - Boulet, Christian

AU - Brodbeck, Claude

AU - Van Thanh, Nguyen

AU - Fouchet, Thierry

AU - Drossart, Pierre

PY - 2002/1/15

Y1 - 2002/1/15

N2 - A far wing corrective factor X for CH4 lines broadened by H2 is proposed. It has been deduced from laboratory spectra measured in the v3 band region at various temperatures between 100 and 300 K. Its quality is demonstrated by comparisons of synthetic spectra with laboratory experiments as well as with the spectrum of the jovian atmosphere observed by ISO.

AB - A far wing corrective factor X for CH4 lines broadened by H2 is proposed. It has been deduced from laboratory spectra measured in the v3 band region at various temperatures between 100 and 300 K. Its quality is demonstrated by comparisons of synthetic spectra with laboratory experiments as well as with the spectrum of the jovian atmosphere observed by ISO.

UR - https://www.scopus.com/pages/publications/0037079637

U2 - 10.1016/S0022-4073(01)00058-9

DO - 10.1016/S0022-4073(01)00058-9

M3 - Article

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SN - 0022-4073

VL - 72

SP - 117

EP - 122

JO - Journal of Quantitative Spectroscopy and Radiative Transfer

JF - Journal of Quantitative Spectroscopy and Radiative Transfer

IS - 2