Vibrational energies of CO2
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http://doi.org/10.17632/pxw2s9g3mk.1
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资源简介：
Title of program: VIBOCO
Catalogue Id: ABWC_v1_0
Nature of problem
Atmospheric temperature profiles and pressure values for planetary atmospheres can be determined using infrared spectra. Carbon dioxide bands observed in the spectra of planets are conveniently used for such calculations. Consequently, theoretical energy levels of this molecule, including various isotopic species, are required.
Versions of this program held in the CPC repository in Mendeley Data
ABWC_v1_0; VIBOCO; 10.1016/0010-4655(75)90040-5
This program has been imported from the CPC Program Library held at Queen's University Belfast (1969-2018)
程序标题：VIBOCO
目录编号：ABWC_v1_0
问题性质：行星大气层的气温剖面和压力值可通过红外光谱进行测定。行星光谱中观察到的二氧化碳谱带便于此类计算。因此，包括各种同位素物种在内的该分子的理论能量级是必需的。
Mendeley数据中CPC存储库中保存的此程序版本：ABWC_v1_0；VIBOCO；10.1016/0010-4655(75)90040-5
该程序已从贝尔法斯特女王大学（1969-2018年）所持有的CPC程序库中导入。
提供机构：
Mendeley Data
