@article{oai:jaxa.repo.nii.ac.jp:00033068,
 author = {福西, 浩 and 藤井, 良一 and 国分, 征 and 遠山, 文雄 and FUKUNISHI, H. and FUJII, R. and KOKUBUN, S. and TOHYAMA, F.},
 journal = {宇宙科学研究所報告. 特集: 宇宙観測研究報告},
 month = {Jan},
 note = {The Akebono (EXOS-D) satellite carries a triaxial fluxgate magnetometer with ring core sensors mounted on a 5-m mast. The magnetometer has four automatically switchable ranges from ±1024 to ±65536nT (full scale) and resolution commensurate with a 16-bit A/D converter in each range (0.031 to 2nT). The rate of sampling is 32 vectors per second. The characteristics of high sensitivity and high time resolution enable us to observe small-scale field-aligned currents embedded in large-scale field-aligned currents. Intense small-scale field-aligned currents are frequently observed in region 1,region 2 and cusp currents and also in the polar cap region. These currents usually consist of pairs of upward and downward field-aligned currents., 資料番号: SA0166927000},
 pages = {99--112},
 title = {あけぼの衛星による沿磁力線電流の観測},
 volume = {25},
 year = {1990}
}