Systematization of Sources of Data on Spectral Line Parameters for the CO2 Molecule and Its Isotopologues in the W@DIS Information System
- Authors: Kozodoev A.V.1, Privezentsev A.I.1, Fazliev A.Z.1, Filippov N.N.2
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Affiliations:
- V.E. Zuev Institute of Atmospheric Optics, Siberian Branch
- St. Petersburg State University
- Issue: Vol 31, No 2 (2018)
- Pages: 201-215
- Section: Optical Models and Databases
- URL: https://journals.rcsi.science/1024-8560/article/view/188368
- DOI: https://doi.org/10.1134/S1024856018020082
- ID: 188368
Cite item
Abstract
Spectral line profiles are used to process experimental spectra when solving the inverse problem of computing the collisional parameters of the profiles [1]. The difference in their shapes is due to different physical conditions (hard/soft collisions, high/low pressures, etc.). Numerous different profiles are used in the study of the spectral line parameters of carbon dioxide, methane, methyl halides, and other molecules. The diversity of the line profiles used in the systematization of spectral line parameters adds complexity to the structures of data available in information systems and to the structures of individuals involved in ontological descriptions of the spectral line properties, which characterize the line profiles. A brief classification of spectral line profiles and their parameters is given, and the results of the systematization of spectral data relating to different line profiles used in processing carbon dioxide spectra are presented. The line profiles available in the library are described, and a system is built for importing spectral line parameters derived from the solution of the direct and inverse problems. Computer software for an automatic description of the properties of the solutions imported has been developed. The basic properties of the spectral data compiled in the W@DIS information system provide a description of the outcome of the imported data quality assessment.
About the authors
A. V. Kozodoev
V.E. Zuev Institute of Atmospheric Optics, Siberian Branch
Email: faz@iao.ru
Russian Federation, Tomsk, 634055
A. I. Privezentsev
V.E. Zuev Institute of Atmospheric Optics, Siberian Branch
Email: faz@iao.ru
Russian Federation, Tomsk, 634055
A. Z. Fazliev
V.E. Zuev Institute of Atmospheric Optics, Siberian Branch
Author for correspondence.
Email: faz@iao.ru
Russian Federation, Tomsk, 634055
N. N. Filippov
St. Petersburg State University
Email: faz@iao.ru
Russian Federation, Peterhof, St. Petersburg, 198504
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