@article{oai:jaxa.repo.nii.ac.jp:00032688,
 author = {横田, 俊昭 and 佐々木, 進 and 河島, 信樹 and 星, 雅之 and 堤井, 信力 and YOKOTA, T. and SASAKI, SUSUMU and KAWASHIMA, NOBUKI and HOSHI, M. and TEI, S.},
 journal = {宇宙科学研究所報告},
 month = {Nov},
 note = {Spectroscopic observation is one of the powerful tools to study the atmospheric compositions of the planets, the roles of the atom and ion in the aurora, and to sense the circumstances of the earth. If two dimensional and multi-channel spectroscopically resolved images are obtained at the same time, the determination of the physical parameters will become much more useful. Spectroscopically resolved multi-channel image camera, proposed in this report, has been planned as following aims; (1) real time data acquisition of the object such as the aurora, airglow, planets and earth by observing the spatially resolved multi-channel spectra at the same time, (2) easy to handle and to change the wave length even after launching. The performances of the prototype which consists of the transmitting grating monochrometer and CCD area sensor have been tested. All controls of the system as well as the data processing have been performed by using the micro-computer. This spectroscopically resolved multi-channel image camera has the following characteristics; (a) the view angle is about 30°and 23°for horizontal and vertical direction, respectively, (b) the spectral sensitivity is in the range from 4000 to 7000 A with spectral resolution of 32A, (c) four maximum spectral images are taken at the same time, and (d) the optical dynamic range is greater than 30 dB at 6328 A., 資料番号: SA0166155000},
 pages = {1--18},
 title = {多チャンネル分光型画像カメラの開発},
 volume = {41},
 year = {1986}
}