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-EM08] Progress in Physics of the Inner Magnetosphere

2015年5月26日(火) 16:15 〜 18:00 302 (3F)

コンビーナ:*Danny Summers(Dept of Math and Stats,Memorial University of Newfoundland)、海老原 祐輔(京都大学生存圏研究所)、三好 由純(名古屋大学太陽地球環境研究所)、座長:Danny Summers(Dept of Math and Stats,Memorial University of Newfoundland)

16:35 〜 16:50

[PEM08-08] Data assimilation of ionospheric magnetic field perturbations into a global magnetospheric model.

*Dmitri KONDRASHOV1Slava MERKIN2 (1.University of California, Los Angeles、2.John Hopkins University, USA)

キーワード:data assimilation, ionosphere, MHD, magnetosphere

Ionosphere is tightly coupled with the magnetosphere and is the only region of geospace where in situ observations approaching global scale are possible. This capability is owing to the emergence of new datasets of key ionospheric measurements with global spatial and high-frequency temporal coverage, such as AMPERE (Active Magnetosphere and Planetary Electrodynamics Response Experiment) magnetic field data measured onboard Iridium satellites. We are reporting first results for assimilation of low-altitude ionospheric measurements of magnetic field perturbations into a Lyon-Fedder-Mobarry (LFM) global magnetospheric model coupled with Rice-Convection Model (RCM).

We adopt optimal interpolation approach and rely on quasi-steady, linear approximation between equatorial magnetospheric pressure and field-aligned currents in the ionosphere. This approximation is estimated numerically by perturbing the LFM-RCM model and by considering only large-scale modes from Fourier decomposition of the ionospheric magnetic field and equatorial magnetospheric pressure.

The developed methodology was validated by using so called "fraternal-twins" model-based assimilation tests. The numerical LFM-RCM model with one set of parameters is used to generate synthetic observations, while model with differing set of parameters is used for assimilation and to calculate magnetospheric pressure corrections to be applied in order to reproduce synthetic observations.