日本地球惑星科学連合2015年大会

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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-EM10] Study of coupling processes in solar-terrestrial system

2015年5月28日(木) 14:15 〜 16:00 A01 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*山本 衛(京都大学生存圏研究所)、野澤 悟徳(名古屋大学太陽地球環境研究所)、小川 泰信(国立極地研究所)、橋口 浩之(京都大学生存圏研究所)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)、座長:小川 泰信(国立極地研究所)

14:30 〜 14:45

[PEM10-19] Temporal change of the precise EIA asymmetry in Thailand-Indonesia sector observed by a beacon receiver network

*Kornyanat WATTHANASANGMECHAI1Mamoru YAMAMOTO1Akinori SAITO2Tatsuhiro YOKOYAMA3 (1.Research Institute for Sustainable Humanosphere, Kyoto University、2.Department of Geophysics, Graduate School of Science, Kyoto University、3.National Institute of Information and Communications Technology)

キーワード:EIA, asymmetry, geomagnetic disturbances, penetrating electric field, rapid evolution

To reveal a temporal change of the equatorial ionization anomaly (EIA) asymmetry, a multipoint satellite-ground beacon experiment was conducted along the meridional plane of the Thailand-Indonesia sector. The observation includes one station near the magnetic equator and four stations at the off-equator latitudes. GRBR-TECs from 97 polar-orbit satellite passes in March 2012 were analyzed in this study. Successive passes captured the rapid evolution of the EIA asymmetry especially during the geomagnetic disturbances. The penetrating electric field during geomagnetic disturbed days is not the cause of an asymmetry. Such rapid evolution of the EIA asymmetry was not seen during the nighttime when meridional wind mainly controlled the asymmetric structures. The EIA asymmetry had a quasi 3-day variation at 21 LT, which probably suggests the forcing from the lower atmosphere. Precise capturing of the crests’ locations and the asymmetry evolution enhances an understanding of the temporal change of the EIA asymmetry in local scale. It leads to a future local modeling of the TEC prediction in Southeast Asia.