Method of averaged energy differences of coupled states and other approaches for calculation line broadening parameters of HD16O transitions

Air-broadening coefficients of the water isotopologue HD16O up to J = 50 for P, Q and R branches calculated using different methods are presented. For partially labeled lines (“good” quantum numbers: J, symmetry and level number) we combined three methods for calculating half-widths: J-dependence and JJ’-dependence up to J=15 and averaging coefficients calculated using a previously developed semi-empirical method for high J (15-50). For lines with full assignments based on normal modes v1, v2, v3, Ka, Kc we used: (a) an analytical model (approximation) which depends on use of rotational quantum numbers J and Ka for both the upper and lower levels; and (b) a method based on the estimate of the averaged energy differences between coupled states. The comparison of calculated data with broadening coefficients from HITRAN-2008 and available experimental data is presented. The resulting broadening coefficients can be used to calculate spectra of water vapor with hundreds millions of weak lines with reasonable accuracy. The line list VTT [Voronin, Tennyson, Tolchenov, MNRAS, 2010], supporting programs, files for calculations of spectra HD16O and estimation of broadening coefficient are made freely available also in electronic form via http://www.exomol.com.

[1]  R. Tolchenov,et al.  Potential energy surface of HDO up to 25,000 cm-1. , 2008, The Journal of chemical physics.

[2]  Nina Lavrentieva,et al.  Collisional Line Broadening and Shifting of Atmospheric Gases: A Practical Guide for Line Shape Modelling by Current Semi-classical Approaches , 2010 .

[3]  R. Tolchenov,et al.  A high accuracy computed line list for the HDO molecule , 2010 .

[4]  Eric Villard,et al.  HDO and H2O vertical distributions and isotopic ratio in the Venus mesosphere by Solar Occultation at Infrared spectrometer on board Venus Express , 2008 .

[5]  P. Bernath,et al.  IUPAC Critical Evaluation of the Rotational-Vibrational Spectra of Water Vapor. Part II. Energy Levels and Transition Wavenumbers for HD16O, HD17O, and HD18O , 2010 .

[6]  V. Zuev,et al.  Statistical Models of the Temperature and Gaseous Components of the Atmosphere , 1987 .

[7]  C. J. Tsao,et al.  Line-widths of pressure-broadened spectral lines , 1962 .

[8]  V. M. Devi,et al.  Diode laser measurements of air and nitrogen broadening in the ν2 bands of HDO, H216O, and H218O , 1986 .

[9]  Harry Partridge,et al.  The determination of an accurate isotope dependent potential energy surface for water from extensive ab initio calculations and experimental data , 1997 .

[10]  V. Starikov Analytical representation of half-width for molecular ro-vibrational lines in the case of dipole–dipole and dipole–quadrupole interactions , 2009 .

[11]  R. Tolchenov,et al.  A new ab initio ground-state dipole moment surface for the water molecule. , 2008, The Journal of chemical physics.

[12]  A Search for Very Low Mass Stars and Brown Dwarfs in the Young σ Orionis Cluster , 1999, astro-ph/9903217.

[13]  Nina N. Lavrentieva,et al.  Line broadening estimate from averaged energy differences of coupled states , 2014, Other Conferences.

[14]  A. D. Bykov,et al.  Semi-empiric approach to the calculation of H2O and CO2 line broadening and shifting , 2004 .

[15]  Jonathan Tennyson,et al.  DVR3D: a program suite for the calculation of rotation-vibration spectra of triatomic molecules , 2004, Comput. Phys. Commun..

[16]  D. Robert,et al.  Short range force effects in semiclassical molecular line broadening calculations , 1979 .

[17]  L. Kedziora-Chudczer,et al.  Modelling the spectra of planets, brown dwarfs and stars using vstar , 2011, 1109.3748.

[18]  R. Barber,et al.  Water in planetary and cometary atmospheres: H2O/HDO transmittance and fluorescence models , 2012 .

[19]  Gang Li,et al.  The HITRAN 2008 molecular spectroscopic database , 2005 .

[20]  J. Tennyson,et al.  Molecular line lists for modelling the opacity of cool stars , 2007 .

[21]  T. Y. Chesnokova,et al.  Estimate of the J′J″ dependence of water vapor line broadening parameters , 2010 .

[22]  V. I. Starikov,et al.  Self- and air-broadening coefficients of HD16O spectral lines , 2012 .

[23]  K. Shine,et al.  Calculation of solar radiative fluxes in the atmosp here: the effect of updates in spectroscopic data , 2003 .

[24]  Anna Fedorova,et al.  The 1.10- and 1.18-μm nightside windows of Venus observed by SPICAV-IR aboard Venus Express , 2011 .

[25]  Laurence S. Rothman,et al.  The HITRAN molecular spectroscopic database: edition of 2000 including updates through 2001 , 2003 .