日本地球惑星科学連合2015年大会

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インターナショナルセッション(口頭発表)

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-EM09] Dynamics in magnetosphere and ionosphere

2015年5月27日(水) 11:00 〜 12:45 302 (3F)

コンビーナ:*中野 慎也(情報・システム研究機構 統計数理研究所)、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)、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:三好 由純(名古屋大学太陽地球環境研究所)

11:15 〜 11:30

[PEM09-02] Long-term trends in ionospheric parameters measured by the EISCAT radars

*Lindis merete BJOLAND1Vasyl BELYEY1Unni pia LOVHAUG1HOZ, Cesar LA1 (1.Department of Physics and Technology, University of Tromso)

Incoherent scatter radar measurements are an important source for studies of ionospheric plasma parameters. Data from the EISCAT Svalbard Radar (ESR), which covers the polar cap and cusp, and the UHF and VHF radars, which cover the auroral zone, can be used to obtain information about the electron density, electron- and ion temperature, and line-of-sight plasma velocity from an altitude of about 50 and up to above 1600 kilometers. As the ESR radar has been operational since 1996 and the UHF and VHF radars since the early 1980s, the accumulated database covers more than one solar cycle in the polar cap and cusp and several solar cycles in the auroral zone.

Results from the study of long-term trends in the ionospheric parameters both from the ESR and UHF/VHF will be shown and a comparison with the IRI-model will be discussed.