日本地球惑星科学連合2014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-EM06_30PM1] Study of coupling processes in Sun-Earth system with large radars and large-area observations

2014年4月30日(水) 14:15 〜 16:00 312 (3F)

コンビーナ:*山本 衛(京都大学生存圏研究所)、小川 泰信(国立極地研究所)、野澤 悟徳(名古屋大学太陽地球環境研究所)、橋口 浩之(京都大学生存圏研究所)、座長:Tsunoda Roland(Center for Geospace Studies SRI International)

15:00 〜 15:15

[PEM06-09] Thermospheric neutral density observations using the EISCAT incoherent scatter radars

*KOSCH Michael1VICKERS Hannah2OGAWA Yasunobu3 (1.Physics Dept., Lancaster University, Lancaster, UK、2.Institute for Physics and Technology, University of Tromso, Norway、3.National Institute of Polar Research, Tachikawa, Japan)

キーワード:Thermospheric density, Incoherent scatter radar

We exploit a recently-developed technique, based on ion-neutral coupling, to estimate the thermospheric neutral density at ~350 km using measurements of ionospheric plasma parameters made by the EISCAT radars. The passive version of the technique is applied to a 13-year long data set from the EISCAT Svalbard Radar (ESR). Here we show that the thermospheric density in the polar cap is decreasing, consistent with satellite drag estimates at lower latitudes. The active version of the technique requires the EISCAT Heater to artificially induce ion up-flow by heating the electrons, with observations from the EISCAT UHF radar. Here we show that ion up-flow is consistent with the plasma pressure gradient, and we extract the thermospheric neutral density. At an altitude of ~500 km, where neutral composition is not always pure atomic oxygen, problems with the technique are discussed.