@inproceedings{oai:jaxa.repo.nii.ac.jp:00020412,
 author = {佐藤, 毅彦 and 今村, 剛 and 空華, 智子 and Satoh, Takehiko and Imamura, Takeshi and Sorahana, Satoko},
 book = {Proceedings of the ISAS lunar and planetary symposium},
 month = {},
 note = {The 41st ISAS Lunar and Planetary Symposium (August 6-8, 2008. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)), We have performed radiative transfer computations to reproduce emissions observed in the near-infrared "windows" of CO2 atmosphere of Venus. Different databases of molecular absorption parameters (HITEMP, CDSD 296 K and 1000 K) are tested to evaluate appropriateness of given line list and absorption parameters. It is found that none of these can reproduce the observations with sufficient accuracy. Merging of a few databases for simulation of Venus atmosphere is probably needed., Physical characteristics: Original contains color illustrations, 資料番号: AA0064291033},
 pages = {143--146},
 publisher = {宇宙航空研究開発機構宇宙科学研究本部, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)},
 title = {Comparison of CO2 absorption databases with application to Venus near-infrared "Window" spectra},
 volume = {41},
 year = {2009}
}