日本地球惑星科学連合2015年大会

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セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM28] 磁気圏-電離圏ダイナミクス

2015年5月28日(木) 16:15 〜 18:00 302 (3F)

コンビーナ:*三好 由純(名古屋大学太陽地球環境研究所)、長谷川 洋(宇宙航空研究開発機構宇宙科学研究所)、中野 慎也(情報・システム研究機構 統計数理研究所)、田中 良昌(国立極地研究所)、堀 智昭(名古屋大学太陽地球環境研究所 ジオスペース研究センター)、座長:田中 良昌(国立極地研究所)

17:45 〜 18:00

[PEM28-17] 日本経度帯のプラズマ圏密度季節変化:地上磁場にFLR同定2点法を適用した長期間連続測定

*河野 英昭1山田 哲郎2北川 雄一郎3Boris Shevtsov4Sergey Khomutov4Igor Poddelskiy4吉川 顕正1group MAGDAS/CPMN5 (1.九州大学大学院理学研究院地球惑星科学部門、2.九州大学理学部地球惑星科学科、3.九州大学大学院理学府地球惑星科学専攻、4.IKIR FEB RAS, Russia、5.九州大学国際宇宙天気科学・教育センター)

In this paper we have applied the cross-phase method and the amplitude-ratio method to the MAGDAS/CPMN ground magnetometers MGD (Magadan) and PTK (Paratunka, Kamchatka), located in the Russian Far East along the 210MM (Magnetic Meridian), and identified FLR (field-line resonance) events. MGD is located at (53.6, 219.1) magnetic latitude and longitude [deg], and PTK is located at (46.2, 226.2). Their L values are 2.9 and 2.1. We have identified the FLR events by using both visual inspection and an automatic-identification computer code.

Although the two magnetometers are separated by about seven degrees in magnetic latitudes, which is larger than the typical separation (about 1-2 degrees) for which the cross-phase and amplitude-ratio methods are efficient, but we could identify more than a hundred FLR events a year from the MGD/PTK-pair data, and the FLR events had a fairly continuous coverage from January to December.

In this paper we estimate the plasmaspheric density from thus obtained FLR frequencies, and examine their seasonal dependence. The result suggests a weak, but marginally significant seasonal dependence with maxima in winter and minima in summer. More details will be discussed at the presentation.