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Titlebook: Weakly Interacting Molecular Pairs: Unconventional Absorbers of Radiation in the Atmosphere; Claude Camy-Peyret,Andrei A. Vigasin Conferen

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發(fā)表于 2025-3-21 19:46:25 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱Weakly Interacting Molecular Pairs: Unconventional Absorbers of Radiation in the Atmosphere
編輯Claude Camy-Peyret,Andrei A. Vigasin
視頻videohttp://file.papertrans.cn/1022/1021370/1021370.mp4
叢書(shū)名稱NATO Science Series: IV:
圖書(shū)封面Titlebook: Weakly Interacting Molecular Pairs: Unconventional Absorbers of Radiation in the Atmosphere; Claude Camy-Peyret,Andrei A. Vigasin Conferen
描述The Advanced Research Workshop entitled “Weakly Interacting Molecular Pairs: Unconventional Absorbers of Radiation in the At- sphere” was held in Abbaye de Fontevraud, France, from April 29 to May 3, 2002. The meeting involved 40 researchers from 14 countries. The goal of this meeting was to address a problem that the scienti?c community is aware of for many years. Up now, however, the so- tion for this problem is far from satisfactory. Pair e?ects are called unconventional in the title of this meeting. In speci?c spectral domains and/or geophysical conditions they are recognized to play a dominant role in the absorption/emission properties of the atmosphere. Water vapor continuum absorption is among the most prominent examples. Permanently improving accuracy of both laboratory studies and ?eld observations requires better knowledge of the spectroscopic features - tributable to molecular pairs which may form at equilibrium. The Workshop was targeted both to clarify the pending questions and, as far as feasible, to trace the path to possible answers since the underlying phenomena are yet incompletely understood and since a reliable theory is often not available. On the other hand, t
出版日期Conference proceedings 2003
關(guān)鍵詞Absorption; atmosphere; cluster; collision; molecule; scattering; spectra; spheric; squall
版次1
doihttps://doi.org/10.1007/978-94-010-0025-3
isbn_softcover978-1-4020-1596-0
isbn_ebook978-94-010-0025-3Series ISSN 1568-1238
issn_series 1568-1238
copyrightSpringer Science+Business Media Dordrecht 2003
The information of publication is updating

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Theoretical Study of Interaction Potential and Pressure Broadening of Spectral Lines for the He–CH3Fperturbation theory (SAPT), with CH3F kept rigid. A global 3D fit on the . points in Jacobi coordinates have been done for the dynamics. Good agreement is observed between present pressure broadening coefficients and experimental data of De Lucia and collaborators (J. Chem. Phys. 97 (1992) 4723).
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發(fā)表于 2025-3-22 05:14:29 | 只看該作者
Theoretical Study of Interaction Potential and Pressure Broadening of Spectral Lines for the He–CH3Fperturbation theory (SAPT), with CH3F kept rigid. A global 3D fit on the . points in Jacobi coordinates have been done for the dynamics. Good agreement is observed between present pressure broadening coefficients and experimental data of De Lucia and collaborators (J. Chem. Phys. 97 (1992) 4723).
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發(fā)表于 2025-3-22 09:27:27 | 只看該作者
Clustering, Saturated Vapors, and the Atmosphere: The (H2O)n, H2O?N2, and H2O?O2 Casesvapor. Consequences for the atmosphere are discussed. Some preliminary (U)MP2 FC/6-311G** results on the H.O?N. and H.O?O. hetero-dimers are reported. The G1 calculations for the (O.). system are presented for the first time too.
6#
發(fā)表于 2025-3-22 13:09:11 | 只看該作者
Clustering, Saturated Vapors, and the Atmosphere: The (H2O)n, H2O?N2, and H2O?O2 Casesvapor. Consequences for the atmosphere are discussed. Some preliminary (U)MP2 FC/6-311G** results on the H.O?N. and H.O?O. hetero-dimers are reported. The G1 calculations for the (O.). system are presented for the first time too.
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發(fā)表于 2025-3-22 17:26:34 | 只看該作者
Collision-Induced Absorption in The CO2 Fermi Triad for Temperatures from 211K to 296 Kly masked by the .. wing absorption. Dimeric features are clearly seen on top of the structureless profiles. Integrated intensities of the Fermi-triad components are deter- mined as a function of temperature.
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發(fā)表于 2025-3-22 23:20:34 | 只看該作者
Collision-Induced Absorption in The CO2 Fermi Triad for Temperatures from 211K to 296 Kly masked by the .. wing absorption. Dimeric features are clearly seen on top of the structureless profiles. Integrated intensities of the Fermi-triad components are deter- mined as a function of temperature.
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