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dc.contributor.authorGamache, R.R.
dc.contributor.authorVispoel, B.
dc.contributor.authorRey, M.
dc.contributor.authorTyuterev, V.
dc.contributor.authorBarbe, A.
dc.contributor.authorNikitin, A.
dc.contributor.authorPolyansky, O.L.
dc.contributor.authorTennyson, J.
dc.contributor.authorYurchenko, S.N.
dc.contributor.authorCsászár, A.G.
dc.contributor.authorFurtenbacher, T.
dc.contributor.authorPerevalov, V.I.
dc.contributor.authorTashkun, S.A.
dc.date2022
dc.date.accessioned2022-03-15T14:14:29Z
dc.date.available2022-03-15T14:14:29Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/9882
dc.descriptionInternal vibrational and rotational partition functions are calculated for nine molecules that are abundant in the terrestrial atmosphere and some are also observed in planetary and exoplanet atmospheres. These molecules are often observed in non-local thermodynamic equilibrium (NLTE) conditions. Calculations are made for all isotopologues of these molecules for which data are available, generally for the temperature range T = 1–5000 K. The methods of calculation of the vibrational and rotational partition functions, Qv and Qr, respectively, the convergence, and the uncertainties for each isotopologue are discussed. Finally, a FORTRAN program, NLTE_TIPS_2021.FOR, to recall the NLTE partition sums is discussed.
dc.languageeng
dc.titlePartition sums for non-local thermodynamic equilibrium conditions for nine molecules of importance in planetary atmospheres
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeNLTE
dc.subject.freePartition sums
dc.subject.freePlanetary and exoplanet atmospheres
dc.source.titleIcarus
dc.source.volume378
dc.source.pageA114947
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/j.icarus.2022.114947
dc.identifier.scopus


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