@article{oai:jaxa.repo.nii.ac.jp:00031512,
 author = {牧野, 忠男 and 関口, 宏之 and 山本, 博聖 and MAKINO, T. and SEKIGUCHI, H. and YAMAMOT, H.},
 issue = {3_B},
 journal = {東京大学宇宙航空研究所報告},
 month = {Sep},
 note = {我々は近年Balloon. Rocketを用いて近赤外域(1～2μ)で夜間大気光OH,O_2をPbSにより観測している。我々のデータによるとOHの近赤外域での発生高度は85～90kmにピークをもち厚さは10km, O_2 (1.27μ)もピークは～90kmで厚さは10kmである。日没後の時間変化はOH (3 - 1, 4 - 2)(6 - 4, 7 - 5)とも夜間は一定の割合で減少し続け,J.S.T., 04:00の強度は地上での日没6時間後(JST 23:00)の約30%であった。, The nightglow emissions of OH and O_2 have been observed in the near infrared region (1-2μ) by balloons and rockets. The data show that the height of the maximum emission rate and the effective thickness of emission layer for OH are 85-90 km and 10 km respectively, and for O_2, 90 km and 10 km respectively. The intensities of OH (3-1,4-2) and (6-4,7-5) bands show a steady decrease during the night; the OH intensity at 04:00 JST is about 30 % of that at 23:00 JST. 6 hours after local ground sunset., 資料番号: SA0124420000},
 pages = {527--535},
 title = {夜光OH, O_2の近赤外域での測定},
 volume = {10},
 year = {1974}
}