@article{oai:jaxa.repo.nii.ac.jp:00031159,
 author = {春日, 敏測 and 海老塚, 昇 and 阿部, 新助 and 矢野, 創 and 渡部, 潤一 and 杉本, 雅俊 and 藤野, 宣知 and Kasuga, Toshihiro and Ebizuka, Noboru and Abe, Shinsuke and Yano, Hajime and Watanabe, Junichi and Sugimoto, Masatoshi and Fujino, Noritomo},
 journal = {The Institute of Space and Astronautical Science repot. S.P.: Proceedings of the 2002 International Science Symposium on the Leonid Meteor Storms},
 month = {Mar},
 note = {Spectroscopic observations were carried out at Mauna Kea, Hawaii and Nobeyama Radio Observatory, Japan, during the strong activity of the Leonid meteor shower in 2001. By using intensified HDTV camera equipped with a reflective grating and UV lens covering 300 to 850 nm wavelength range, the first detection of spectra under 350 nm was succeeded on the ground-based observation. Discovery of OH emission in the meteor gave a new concept on the early earth. In this paper, the observational system developed by the group is described., 資料番号: AA0046133021},
 pages = {159--163},
 title = {High definition TV spectra of the 2001 Leonids in visible ultraviolet region},
 volume = {15},
 year = {2003}
}