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)

15:15 〜 15:30

[PEM06-10] 3D ionospheric electron density determination in Scandinavia with TomoScand and EISCAT 3D

*AMM Olaf1NORBERG Johannes1VIERINEN Juha2ROININEN Lassi3LEHTINEN Markku3NAKAMIZO Aoi1 (1.Finnish Meteorological Institute, Arctic Research Unit, Helsinki, Finland、2.Haystack Observatory, Massachusetts Institute of Technology, Westford, Massachusetts, USA、3.Sodankyla Geophysical Observatory, University of Oulu, Finland)

キーワード:ionospheric tomography, ionospheric electron density, ground-based observations, EISCAT 3D

The TomoScand network for ionospheric tomography in Scandinavia consists of a network of newly designed Beacon receivers and an extensive, dense array of GPS receivers. A novel tomographic inversion technique allows for a multi-frequency analysis for reconstruction of ionospheric electron densities, and is also able to include information of a multitude of ground-based measurements into the inversion, such as data from ionosondes, from the EISCAT radar, and from the magnetometers of the MIRACLE network in Scandinavia. We present the current status of the TomoScand network, and show latest inversion results on 2D profiles in meridional direction, together with test results that allow to evaluate the performance of the inversion technique. Further, we discuss the future development into a full 3D inversion scheme, and how the TomoScand network can be used as a "partner instrument" for the upcoming EISCAT 3D radar.