@article{oai:nipr.repo.nii.ac.jp:00008113,
 author = {長井, 嗣信 and 河野, 毅 and NAGAI, Tsugunobu and KOHNO, Tsuyoshi},
 journal = {南極資料},
 month = {Feb},
 note = {P(論文), 本論文では,磁気圏嵐時の静止衛星軌道における高エネルギー粒子のフラックス変動について報告する.3つの静止衛星の同時観測により,夕方側で粒子の減少がみえる時に,真夜中から朝側にかけては,粒子の増加がみられることを明確に示した.また,地磁気じょう乱が引き続いて起きている時には,比較的大きなしかも孤立して起きた磁気圏嵐の時とやや異なる粒子フラックスの変動がみられることを2日間の例を使い示した., This article reports the results of studying the behavior of the energetic particle flux obtained at synchronous orbit during substorms. The multi-satellite study has clearly showed that the evening particle flux decrease contrasts with the behavior in the midnight-morning side, where the energetic particle flux increases at the substorm expansion onset. Two-days' examples indicate that the flux behavior during the periods of the continued geomagnetic activities seems to be somewhat different from that for the relatively large and isolated events.},
 pages = {23--34},
 title = {静止衛星軌道における高エネルギー粒子の観測(a.入射粒子とオーロラ)(第2回極域における電離圏磁気圏総合観測シンポジウム : Part I)},
 volume = {68},
 year = {1980},
 yomi = {ナガイ, ツグノブ and コウノ, ツヨシ}
}