Электронная библиотека (репозиторий) Томского государственного университета

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Add   New accurate theoretical line lists of 12CH4 and 13CH4 in the 0-13400 cm-1 range: Application to the modeling of methane absorption in Titan's atmosphere
Authors: Nikitin, Andrei V. | Bézard, Bruno | Rannou, Pascal | Coustenis, Athena | Tyuterev, Vladimir G. | Rey, Michaël
Source: Icarus. 2018. Vol. 303. P. 114-130
Type: статьи в журналах
Date: 2018
Description: The spectrum of methane is very important for the analysis and modeling of Titan’s atmosphere but its insufficient knowledge in the near infrared, with the absence of reliable absorption coefficients, ... More
Add   CH3CN self-broadening coefficients and their temperature dependences for the Earth and Titan atmospheres
Authors: Dudaryonok, Anna S. | Lavrentieva, Nina N. | Buldyreva, Jeanna V.
Source: Icarus. 2015. Vol. 250. P. 76-82
Type: статьи в журналах
Date: 2015
Description: Theoretical self-broadening coefficients and associated temperature dependences for methyl cyanide lines in parallel (ΔK = 0) bands are reported for large ranges of rotational quantum numbers (0 ⩽ J ⩽ ... More
Add   Linewidths and temperature exponents of CH3CN-N2
Authors: Buldyreva, Jeanna V. | Lavrentieva, Nina N. | Dudaryonok, Anna S.
Source: Proceedings of SPIE. 2015. Vol. 9680 : 21st International Symposium Atmospheric and Ocean Optics: Atmospheric Physics, June 22-26, 2015, Tomsk, Russian Federation. P. 96800A-1-96800A-7
Type: статьи в журналах
Date: 2015
Description: Calculations of nitrogen-broadening coefficients and their temperature exponents for methyl cyanide lines at the room temperature using semi-empirical method are presented. They were performed for wid ... More
Add   Ab initio and multipolar characterisation of the induced dipole surface for CH4-CH4: Application to dipole-forbidden absorption in the Titan's atmosphere
Authors: Buryak, I. A. | Kalugina, Yulia N. | Vigasin, A. A.
Source: Journal of molecular spectroscopy. 2013. Vol. 291. P. 102-107
Type: статьи в журналах
Date: 2013
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