The HITRAN molecular spectroscopic database: edition of 2000 including updates through 2001

By L. Rothman, A. Barbe, D. Benner, L. Brown, C. Camy‐Peyret, M. Carleer, Kelly Chance, C. Clerbaux, V. Dana, V. Devi and 21 more. 2003

1,252 citations recorded by the source corpus.

Subfields: Atmospheric Science, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/a5f98e1bb6e640fe0043e90163f37bae41c0e643

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Citations in the corpus

Total internal partition sums for 166 isotopologues of 51 molecules important in planetary atmospheres: Application to HITRAN2016 and beyond (2017, methodology): “[16] provided TIPS for the 40 molecules and 95 isotopologues/isotopomers on the HITRAN2000 database [21] with an additional 13 rare isotopologues/ isotopomers of ozone and carbon dioxide.”
Description of the NCAR Community Atmosphere Model (CAM 3.0) (2004, methodology): “The hybrid coordinate is more general in concept than the modified σ scheme of Sangster [1960], which is used in the GFDL SKYHI model. However, the hybrid coordinate is normally specified in such a way that the two coordinates are identical. The following description uses the same general developmen”
Einstein A-coefficients and statistical weights for molecular absorption transitions in the HITRAN database (2006, methodology): “Section 2 describes the motivation that led to the replacement of the weighted square of the transition moment, R, that was present in the previous edition of HITRAN [2] by the Einstein Acoefficient.”
Oxygen compounds in Titan's stratosphere as observed by Cassini CIRS (2007, methodology): “The measured spectra are fitted using an optimal estimation method that minimises a cost function ( Rodgers, 1976 ).”
Retrieval of stratospheric temperatures from Atmospheric Infrared Sounder radiance measurements for gravity wave studies (2009, neutral): “…pressure uncertainty for the hydrostatic build-up of 5% (corresponding to 400 m uncertainty of the geopotential heights) will cause a retrieval error of 0.3 to 0.9 K. Fourth, a 5% uncertainty in the carbon dioxide spectroscopic data [Rothman et al., 2003] causes retrieval errors of 0.1 to 0.4 K.”
Habitable Moist Atmospheres on Terrestrial Planets near the Inner Edge of the Habitable Zone around M Dwarfs (2017, methodology): “Absorption by water vapor is based on the HITRAN2000 line database (Rothman et al. 2003) and incorporates the Clough, Kneizys, and Davies (CKD) 2.4 prescription for the continuum (Clough et al. 1989).”
An atomic and molecular database for analysis of submillimetre line observations (2004, background): “The JPL1 catalog (Pickett et al. 1998), HITRAN2 database (Rothman et al. 2003), and the CDMS3 catalogue (Müller et al. 2001) contain energy levels and transition strengths for a large number of molecular species.”
Atomic and Molecular Opacities for Brown Dwarf and Giant Planet Atmospheres (2006, methodology): “In x 2.1, we discuss the species with data obtained from the HITRAN (Rothman et al. 2003, 2005) and GEISA (JacquinetHusson et al. 1999, 2003, 2005) databases, together with other sources.”