@article{oai:nipr.repo.nii.ac.jp:00008131,
 author = {林, 幹治 and HAYASHI, Kanji},
 journal = {南極資料},
 month = {Feb},
 note = {P(論文), その発生が磁気圏の外部の環境に強く依存しているPc 3-5について,静止軌道上ならびに地上の極光帯での経度方向の多点観測に基づいた解析がなされ,経度方向の波数5-15 (1/2π rad)の波が正午付近を起点に朝方,夕方の方向へL-shellに沿って伝わっていることが示された.さらにplasmapauseの内側のPc 4についてほぼ磁気子午面に沿った多点観測により磁力線の局所的共鳴の実例が示された.さらに磁気圏内部に発生原因を持つPc 1,P_1脈動その他について最近の観測結果,現況を述べる., Pc 3-5 geomagnetic pulsations which are currently considered to be generated in the magnetosheath and resonated to a matched period of toroidal oscillations in the magnetosphere have added an advanced recognition of azimuthal wave characteristics propagating from the noon meridian in the magnetosphere. based upon multipoint observations both along the geostationary orbit and along the auroral zone on the ground. Examples supporting a local field line resonance model are found for Pc 4 within the plasmasphere. Another class of micropulsations which are generated within the magnetosphere associated with ring-current proton and auroral zone disturbances are also reviewed.},
 pages = {215--231},
 title = {磁気圏ULF波動(d.磁気圏内のULF波動)(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 = {ハヤシ, カンジ}
}