@article{oai:nipr.repo.nii.ac.jp:00008038,
 author = {佐藤, 夏雄 and 福西, 浩 and 巻田, 和男 and SATO, Natsuo and FUKUNISHI, Hiroshi and MAKITA, Kazuo},
 journal = {南極資料},
 month = {Feb},
 note = {P(論文), 地磁気子午面に沿って約270km離れた昭和基地とみすほ基地において,地磁気,地磁気脈動,オーロラ,ELF・VLF波動,オーロラ等の同時観測を行った.この論文ては,ELF波動の強度比およびスペクトル構造の相互についての解析結果を報告する.その結果は,1)周波数-時間スペクトルは非常に似ている.2)発生周波数の強度比はみすほ基地ては低周波数帯域が強く,昭和基地では高周波数帯域が強い.3)QPエミッションの周期は全く同してある., Simultaneous observations of ELF・VLF emissions, magnetic variations, cosmic noise absorption and auroras have been carried out at Syowa and Mizuho Stations since June 1976. Mizuho Station is located at a distance of ～270 km poleward on the same magnetic meridian as that of Syowa. From the ELF emission data observed at both the stations, the following results were obtamed 1) Frequency-time spectra of ELF chorus emissions were quite similar at both the stations. However, it ls found that the intensity in the lower frequency range (<15 kHz) is greater at Mizuho than at Syowa, and veisa in the higher frequency range 2) The period of QP emissions was same at both the stations},
 pages = {134--145},
 title = {ELF波動のみずほ-昭和基地同時観測},
 volume = {64},
 year = {1979},
 yomi = {サトウ, ナツオ and フクニシ, ヒロシ and マキタ, カズオ}
}