On the improvement of the rotational structure analysis of 13CH3D ground vibrational state
Author:
Affiliation:
1. Laboratory of Molecular Spectroscopy, Physics Department, National Research Tomsk State University , Tomsk, 634050, Russia
2. Department of Physics, University of Oulu , P. O. Box 3000, FIN-90014 University of Oulu, Finland
Publisher
Informa UK Limited
Subject
Physical and Theoretical Chemistry,Condensed Matter Physics,Molecular Biology,Biophysics
Link
https://www.tandfonline.com/doi/pdf/10.1080/00268976.2013.798437
Reference41 articles.
1. The abundances of CH4, CH3D, NH3, and PH3 in the troposphere of Jupiter derived from high-resolution 1100-1200/cm spectra
2. The tropospheric gas composition of Jupiter's north equatorial belt /NH3, PH3, CH3D, GeH4, H2O/ and the Jovian D/H isotopic ratio
3. The composition of Saturn's atmosphere at northern temperate latitudes from Voyager IRIS spectra - NH3, PH3, C2H2, C2H6, CH3D, CH4, and the Saturnian D/H isotopic ratio
4. The spectrum of Saturn from 1990 to 2230 cm−1: Abundances of AsH3, CH3D, CO, GeH4, NH3, and PH3
5. Titan's atmosphere from Voyager infrared observations
Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Investigation of the High-Resolution Fourier Spectrum of the ν3+ν4 Band of the 13CH3D Molecule;Russian Physics Journal;2017-01
2. Calculation of the Vibrational-Rotational Energy Structure of Molecules with Tetrahedral Symmetry of the Type XY 4;Russian Physics Journal;2014-11
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