@article{oai:jaxa.repo.nii.ac.jp:00032100,
 author = {西, 恵三 and 東, 康一 and 山口, 朝三 and 末元, 善三郎 and NISHI, Keizo and HIGASHI, Koichi and YAMAGUCHI, Asami and SUEMOTO, Zenzaburo},
 issue = {2_B},
 journal = {東京大学宇宙航空研究所報告},
 month = {May},
 note = {The absolute intensity and the centre-to-limb variations of the sun in the vacuum ultraviolet region were observed by the K-10-6 rocket flown from Uchinoura, Japan, on September 1, 1971, 1110 JST. The nose cone of the rocket was controlled to point the direction of the sun by a jet system within about ±20'. A trichrometer was used for the measurements, and the measured wavelengths were 1,629 A, 1,684 A, and 1,739 A. The spatial and spectral resolutions were 1'.3 and 8.3 A respectively. The obseaved results were compared with some solar models, and our results seem to fit best to the HSRA (Harvard Smithsonian Reference Atmosphere)., 資料番号: SA0125212000},
 pages = {359--376},
 title = {太陽真空紫外領域スペクトルの絶対測定および中心周縁強度変化の観測(K-10-6号機による)},
 volume = {9},
 year = {1973}
}