@article{oai:jaxa.repo.nii.ac.jp:00031685,
 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 = {4_B},
 journal = {東京大学宇宙航空研究所報告},
 month = {Dec},
 note = {The centre-to-limb variations of the sun in the vacuum ultraviolet region were observed by a scanning spectrometer mounted in the K-10-11 rocket flown from Uchinoura, Japan, on September 24, 1975, 1400 JST. The nose cone of the rocket was controlled to point the direction of the sun by a jet system (CN) within about 20. The spatial and spectral resolutions of the spectrometer were 50" and 3.3 Å respectively. The observed results were consistent with our privious one (1630Å～1740Å) and those obtained by the French group (1740Å～2000Å), but differ from the HSRA model (about 1700Å～2000Å)., 資料番号: SA0124690000},
 pages = {959--973},
 title = {太陽真空紫外領域に於ける中心周縁強度変化の観測(K-10-11号機による)},
 volume = {12},
 year = {1976}
}