@article{oai:kumadai.repo.nii.ac.jp:00024920,
 author = {三島, 嶽志 and Mishima, Takeyuki and Maeda, Kengo and 桃井, 凡夫 and Momoi, Tsuneo and Onomichi, Mitsukazu and Yamashita, Tairi and 三島, 嶽志 and Mishima, Takeyuki and Maeda, Kengo and 前田, 健悟 and 桃井, 凡夫 and 尾道, 三一 and 山下, 太利},
 journal = {熊本大学教育工学センター紀要},
 month = {Feb},
 note = {application/pdf, 論文(Article), Since the motions of the astronomical objects is subject to time and position, it is difficult for teachers to obtain and prepare the necessary data in print.
A microcomputer, however, can simulate the motion and immediately gives it to them.
Hence, we have attempted to provide elementary and junior high school teachers with the resources about the motion of the sun by the microcomputer.
In this paper, the following are given:(1)the variation of the sun's altitude with time, (2)the motion of the sun at different seasons, (3)the motion of the sun at different locations, (4)changes of the time and azimuth at rise of the sun in a year, (5)Changes of the altitude of southing and length of day in a year, and　(6)the altitude and azimuth of a constellation.},
 pages = {35--40},
 title = {マイクロコンピュータの特性を生かした教師用資料 : 太陽の動きを中心として},
 volume = {1},
 year = {1984},
 yomi = {ミシマ, タケユキ and モモイ, ツネオ and ミシマ, タケユキ and マエダ, ケンゴ}
}