Электронная библиотека (репозиторий) Томского государственного университета
Perevalov, Valery I. | Campargue, Alain | Mondelain, Didier

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Source: Journal of Quantitative Spectroscopy and Radiative Transfer. 2019. Vol. 229. P. 40-49
Type: статьи в журналах
Date: 2019
Description: In spite of being a greenhouse gas with a large global warming potential, the absorption spectrum of nitrous oxide in the near infrared is insufficiently characterized. In the present work, the spectr ... More
Source: Journal of molecular spectroscopy. 2019. Vol. 362. P. 84-89
Type: статьи в журналах
Date: 2019
Description: The room temperature absorption spectrum of 17O enriched carbon dioxide is investigated by high sensitivity cavity ring down spectroscopy (CRDS) between 5695 and 5850 cm−1. About 1100 lines are measur ... More
Source: Journal of Quantitative Spectroscopy and Radiative Transfer. 2018. Vol. 217. P. 73-85
Type: статьи в журналах
Date: 2018
Description: The very weak absorption spectrum of the minor isotopologues of carbon dioxide near 1.74 µm (5702–5879 cm−1) is studied by high sensitivity cavity ring down spectroscopy (CRDS) with an 18O enriched sa ... More
Source: Journal of Quantitative Spectroscopy and Radiative Transfer. 2018. Vol. 207. P. 95-103
Type: статьи в журналах
Date: 2018
Description: The very weak absorption spectrum of natural CO2 near 1.74 µm (5702–5879 cm−1) is studied at high sensitivity. The investigated region corresponds to a transparency window of very weak opacity which i ... More
Source: Journal of molecular spectroscopy. 2018. Vol. 354. P. 54-59
Type: статьи в журналах
Date: 2018
Description: The 1.74 µm spectral region corresponds to a very weak absorption interval of carbon dioxide (or “transparency window”) of particular importance to sound the deep atmosphere and the surface of Venus. ... More
Source: Journal of Quantitative Spectroscopy and Radiative Transfer. 2016. Vol. 184. P. 233-240
Type: статьи в журналах
Date: 2016
Description: The absorption of carbon dioxide is very weak near 2.3 µm which makes this transparency window of particular interest for the study of Venus’ lower atmosphere. As a consequence of the weakness of the ... More
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