Extended Analysis of Line Positions and Intensities of Ozone Bands in the 2900–3400 cm−1 Region

Михайленко, С.Н.; Barbe, A.; Tyuterev, Vladimir G.

doi:10.1006/jmsp.2002.8597

Cited by 26 publications

(10 citation statements)

References 15 publications

(14 reference statements)

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“…were calculated using Hamiltonian parameters [89]. The transition moment parameters for the cold bands listed in this table (2590 -3400 cm -1 spectral range) are given in…”

Section: O 3 (Molecule 3)mentioning

confidence: 99%

The HITRAN 2008 molecular spectroscopic database

Rothman

Gordon

Barbé

et al. 2009

Journal of Quantitative Spectroscopy and Radiative Transfer

3,305

2,123

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“…were calculated using Hamiltonian parameters [89]. The transition moment parameters for the cold bands listed in this table (2590 -3400 cm -1 spectral range) are given in…”

Section: O 3 (Molecule 3)mentioning

confidence: 99%

The HITRAN 2008 molecular spectroscopic database

Rothman

Gordon

Barbé

et al. 2009

Journal of Quantitative Spectroscopy and Radiative Transfer

3,305

2,123

View full text Add to dashboard Cite

“…associated with the upper states {(0 1 2), (1 1 1), (2 1 0), (0 0 3), (1 0 2), (2 0 1), (1 3 0), (3 0 0)} have been calculated using the Hamiltonian parameters for the upper states from Ref. [79]. The transition moment parameters for the cold bands (2590-3400 cm À 1 spectral range) of these states are given in Ref.…”

Section: O 3 (Molecule 3)mentioning

confidence: 99%

“…The transition moment parameters for the cold bands (2590-3400 cm À 1 spectral range) of these states are given in Ref. [79]. The calculations of the main part of the hot bands line intensities have been done with the transition moments given in Refs.…”

Section: O 3 (Molecule 3)mentioning

confidence: 99%

The 2009 edition of the GEISA spectroscopic database

Jacquinet-Husson

Crépeau

Armante

et al. 2011

Journal of Quantitative Spectroscopy and Radiative Transfer

320

133

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The updated 2009 edition of the spectroscopic database GEISA (Gestion et Etude des Informations Spectroscopiques Atmosphé riques; Management and Study of Atmospheric Spectroscopic Information) is described in this paper. GEISA is a computer-accessible system comprising three independent sub-databases devoted, respectively, to: line parameters, infrared and ultraviolet/visible absorption cross-sections, microphysical and optical properties of atmospheric aerosols. In this edition, 50 molecules are involved in the line parameters sub-database, including 111 isotopologues, for a total of 3,807,997 entries, in the spectral range from 10 À 6 to 35,877.031 cm À 1. The successful performances of the new generation of hyperspectral sounders depend ultimately on the accuracy to which the spectroscopic parameters of the optically active atmospheric gases are known, since they constitute an essential input to the forward radiative transfer models that are used to interpret their observations. Currently, GEISA is involved in activities related to the assessment of the capabilities of IASI (Infrared Atmospheric Sounding Interferometer; http://smsc.cnes.fr/IASI/index.htm) on board the METOP European satellite through the GEISA/IASI database derived from GEISA. Since the Metop-A (http://www.eumetsat.int) launch (19 October 2006), GEISA is the reference spectroscopic database for the validation of the level-1 IASI data. Also, GEISA is involved in planetary research, i.e., modeling of Titan's atmosphere, in the comparison with observations performed by Voyager, or by ground-based telescopes, and by the instruments on board the Cassini-Huygens mission. GEISA, continuously developed and maintained at LMD (Laboratoire de Mé té orologie Dynamique, France) since 1976, is implemented on the IPSL/CNRS (France) ''Ether'' Products and Services Centre WEB site (http://ether.ipsl.jussieu.fr), where all archived spectroscopic data can be handled through general and user friendly associated management software facilities. More than 350 researchers are registered for on line use of GEISA.

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“…There are both systematic biases and multiplicative biases that favour the MART-based retrieval. For both OSIRIS retrievals, all O 3 cross sections were taken from Bogumil et al [59], while the HITRAN 2004 infrared line parameters were based on original work by Mikhailenho et al [60] and De Backer-Barilly et al [61]. 7e, the slope of the linear fit is 1.3, illustrating a clear multiplicative bias of higher monthly Table 1.…”

Section: O 3 Comparisonsmentioning

confidence: 99%

Comparison of OSIRIS stratospheric NO₂ and O₃ measurements with ground-based Fourier transform spectrometer measurements at the Toronto Atmospheric Observatory

Taylor¹,

Strong²,

McLinden³

et al. 2007

Can. J. Phys.

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Stratospheric NO 2 and O 3 retrieved from measurements of limb-scattered sunlight made by the Optical Spectrograph and InfraRed Imager System (OSIRIS) are compared with like observations made by a ground-based infrared Fourier Transform Spectrometer at the Toronto Atmospheric Observatory (TAO-FTS). Two different versions of OSIRIS NO 2 are compared (DOAS version 3.0 and MART version 2.0) with partial column concentrations retrieved from the TAO-FTS. Two OSIRIS O 3 versions are also compared (Triplet version 3.0 and MART version 2.0) with O 3 retrieved from the TAO-FTS.To accommodate the most coincidences, comparisons are based on monthly mean stratospheric partial columns covering 16-50 km. All coincident monthly means display high correlations: 0.82-0.97. The monthly mean NO 2 at TAO compared with the monthly mean NO 2 from OSIRIS shows an average difference of less than ∼3% with standard deviations up to 6%. The OSIRIS NO 2 observations show a multiplicative bias of ∼0.8-0.9 and a systematic difference of 5-10% greater then those of the TAO-FTS. O 3 differences are less than 5%, on average, with standard deviations ranging from 2% to 2.8%. There is a pronounced multiplicative bias of OSIRIS compared with the TAO-FTS ranging from 0.55 to 0.73. The systematic O 3 differences are less than 5% larger for OSIRIS. These small differences meet the standards outlined in the Integrated Global Observing Strategy and confirm the quality of the OSIRIS data for studying stratospheric ozone and nitrogen chemistry.

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Extended Analysis of Line Positions and Intensities of Ozone Bands in the 2900–3400 cm−1 Region

Cited by 26 publications

References 15 publications

The HITRAN 2008 molecular spectroscopic database

The HITRAN 2008 molecular spectroscopic database

The 2009 edition of the GEISA spectroscopic database

Comparison of OSIRIS stratospheric NO₂ and O₃ measurements with ground-based Fourier transform spectrometer measurements at the Toronto Atmospheric Observatory

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Extended Analysis of Line Positions and Intensities of Ozone Bands in the 2900–3400 cm−1 Region

Cited by 26 publications

References 15 publications

The HITRAN 2008 molecular spectroscopic database

The HITRAN 2008 molecular spectroscopic database

The 2009 edition of the GEISA spectroscopic database

Comparison of OSIRIS stratospheric NO2 and O3 measurements with ground-based Fourier transform spectrometer measurements at the Toronto Atmospheric Observatory

Contact Info

Product

Resources

About

Comparison of OSIRIS stratospheric NO₂ and O₃ measurements with ground-based Fourier transform spectrometer measurements at the Toronto Atmospheric Observatory