Broadening parameters of the H2O–He collisional system for astrophysical applications
| Parent link: | Journal of Molecular Spectroscopy: Scientific Journal Vol. 321.— 2016.— [P. 50-58] |
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| Müşterek Yazar: | |
| Diğer Yazarlar: | , , , |
| Özet: | Title screen The water vapor line broadening γ and shift δ coefficients in the ν1 + ν2, ν2 + ν3, ν1 + ν3, 2ν3, 2ν1, 2ν2 + ν3, and ν1 + 2ν2 vibrational bands were obtained from the analysis of the H2O-He absorption spectra, recorded in the region from 5000 to 7500 cm−1 with the spectral resolution of 0.01 cm−1 using a Bruker IFS 125HR FTIR spectrometer. The vibrational bands 2ν3 and ν1 + 2ν2 were investigated for the first time. The calculations ofγ and δ were performed in the framework of the semi-classical method. The rotational contributions as well as the contributions connected with the accidental resonances were taken into account in the used H2O-He interaction potential. The analytical representation of the broadening coefficients γ at planetary temperatures was introduced and discussed. Режим доступа: по договору с организацией-держателем ресурса |
| Dil: | İngilizce |
| Baskı/Yayın Bilgisi: |
2016
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| Konular: | |
| Online Erişim: | http://dx.doi.org/10.1016/j.jms.2016.01.009 |
| Materyal Türü: | Elektronik Kitap Bölümü |
| KOHA link: | https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=648434 |
MARC
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| 200 | 1 | |a Broadening parameters of the H2O–He collisional system for astrophysical applications |f T. M. Petrova [et al.] | |
| 203 | |a Text |c electronic | ||
| 300 | |a Title screen | ||
| 320 | |a [References: p. 58 (30 tit.)] | ||
| 330 | |a The water vapor line broadening γ and shift δ coefficients in the ν1 + ν2, ν2 + ν3, ν1 + ν3, 2ν3, 2ν1, 2ν2 + ν3, and ν1 + 2ν2 vibrational bands were obtained from the analysis of the H2O-He absorption spectra, recorded in the region from 5000 to 7500 cm−1 with the spectral resolution of 0.01 cm−1 using a Bruker IFS 125HR FTIR spectrometer. The vibrational bands 2ν3 and ν1 + 2ν2 were investigated for the first time. The calculations ofγ and δ were performed in the framework of the semi-classical method. The rotational contributions as well as the contributions connected with the accidental resonances were taken into account in the used H2O-He interaction potential. The analytical representation of the broadening coefficients γ at planetary temperatures was introduced and discussed. | ||
| 333 | |a Режим доступа: по договору с организацией-держателем ресурса | ||
| 461 | |t Journal of Molecular Spectroscopy |o Scientific Journal | ||
| 463 | |t Vol. 321 |v [P. 50-58] |d 2016 | ||
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| 701 | 1 | |a Petrova |b T. M. |g Tatjyana Mikhaylovna | |
| 701 | 1 | |a Solodov |b A. M. |g Aleksandr Mikhaylovich | |
| 701 | 1 | |a Solodov |b A. A. |g Aleksandr Aleksandrovich | |
| 701 | 1 | |a Starikov |b V. I. |c physicist |c Professor of Yurga technological Institute of Tomsk Polytechnic University, doctor of physical and mathematical Sciences |f 1955- |g Vitaly Ivanovich |3 (RuTPU)RU\TPU\pers\34163 |9 17703 | |
| 712 | 0 | 2 | |a Национальный исследовательский Томский политехнический университет |b Юргинский технологический институт (филиал) |b Кафедра информационных систем |3 (RuTPU)RU\TPU\col\18893 |9 27242 |
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| 856 | 4 | |u http://dx.doi.org/10.1016/j.jms.2016.01.009 | |
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