日本地球惑星科学連合2018年大会

講演情報

[EE] ポスター発表

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-EM13] 太陽地球系結合過程の研究基盤形成

2018年5月20日(日) 15:30 〜 17:00 ポスター会場 (幕張メッセ国際展示場 7ホール)

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(名古屋大学宇宙地球環境研究所、共同)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)

[PEM13-P01] GPS-TEC電離圏3Dトモグラフィー;スーパーコンピュータによる大量データ解析

*山本 衛1水野 遼1斎藤 享2齊藤 昭則3 (1.京都大学生存圏研究所、2.電子航法研究所、3.京都大学大学院理学研究科)

キーワード:GPS-TEC、電離圏トモグラフィー、並列処理

Measurement of ionospheric total electron content (TEC) by using ground-based GPS receivers is now widely used, which we refer to as GPS-TEC. In Japan, there is one of the densest network of GPS receivers that is named as GEONET (GNSS Earth observation network system) operated by Geospatial Information Authority of Japan (GSI). We have developed three-dimensional (3D) tomography analysis based on the constrained least-squares fitting method, and applied it to the GPS-TEC data from GEONET. We started the real-time analysis with 15 minutes interval and about five minutes latency since March 2016. In this paper we report that we analyzed most of GEONET data since 1996 by using the supercomputer of Kyoto University. We assign one core of the supercomputer to one-day analysis (15-minute interval from 200 GPS receivers). By utilizing about 2000 core of the supercomputer syste, we achieved that processing time for one-year data was about 30 hours only. The results are statistically validated through comparisons with ionosondes and COSMIC occultation measurements. The maximum density from the 3D tomography showed good agreement with the foF2 parameter from ionosondes. We also found that the F2-peak of the 3D tomography density profile is lower in density, and higher in altitude compared with corresponding parameters from the COSMIC occultation measurements.