*ChaoYen Chen1,2、Tiger J. Y. Liu1,2,3 (1.Institute of Space Science, National Central University, Taiwan、2.Center for Astronautical Physics and Engineering, National Central University, Taiwan 、3.Center for Space and Remote Sensing Research, National Central University, Taiwan)
セッション情報
[E] 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-EM14] Recent Advances in Ionosphere Observation and Modeling for Monitoring and Forecast
2019年5月26日(日) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 8ホール)
コンビーナ:Yang-Yi Sun(China University of Geosciences)、LIN CHIYEN(Center for Astronautical Physics and Engineering, National Central University, TAIWAN)、MINYANG CHOU(National Cheng Kung University)
Over the past few decades, rapid developments in space technology have advanced the research of ionospheric space weather by increasing a great number of ground- and space-based observations. In the ground segment, the dense ground-based GNSS networks, radars, and airglow instruments have greatly extended the observational coverages. In the space segment, the extraordinary satellite missions with payloads onboard the satellites providing radio occultation soundings of vertical electron density structure and in-situ observations of airglow, temperature, neutral winds, and electron density contribute to the understanding of middle and upper atmospheric dynamics. With the large amount and diversity of datasets, theoretical and empirical models can be validated and implemented for inclusion of new thermosphere and ionosphere phenomena. Furthermore, remarkable breakthrough of data assimilation techniques advances the ionosphere monitoring and forecast. The recent innovations in observations and models reinterpret the studies of ionospheric space weather. The purpose of this session is to solicit studies providing observations, theoretical and empirical modeling and data assimilation on the multiple scales of ionospheric phenomena, from global morphology to small-scale irregularities and traveling ionospheric disturbances. Studies on magnetically quiescent and disturbed conditions will be both addressed.
*Chi-Kuang Chao1、Yi-Wun Chen1 (1.Graduate Institute of Space Science, National Central University)
*FU-YUAN CHANG1、JANN-YENQ Liu1、Chi-Kuang Chao1 (1.National Central University)
*Tsung-Che Tsai1,2、Hau-Kun Jhuang3、Lou-Chuang Lee3,4,5、Yi-Ying Ho4 (1.National Center for High-Performance Computing, National Applied Research Laboratories, Hsinchu, Taiwan、2.Department of Civil Engineering, National Chiao Tung University, Hsinchu, Taiwan.、3.Department of Geoscience, National Taiwan University, Taipei, Taiwan.、4.Institute of Earth Science, Academia Sinica, Nankang, Taipei, Taiwan.、5.Institute of Space Science, National Central University, Jhongli, Taiwan.)
*Oksana Mandrikova1、Yurii Polozov1、Bogdana Mandrikova1,2 (1.Institute of Cosmophysical Research and Radio Wave Propagation, Far Eastern Branch of the Russian Academy of Sciences、2.Saint Petersburg Electrotechnical University "LETI")
*TsungYu Wu1、JANN-YENQ Liu1 (1.Institute of Space Science, NCU, Taiwan)
*行松 彰1,2 (1.国立極地研究所、2.総合研究大学院大学)
*Hau-Kun Jhuang1、Tsung-Che Tsai2,3、Lou-Chuang Lee1,4,5、Yi-Ying Ho4 (1.Department of Geosciences, National Taiwan University, Taipei, Taiwan、2.National Center for High-performance Computing, National Applied Research Laboratories, Hsinchu, Taiwan、3.Department of Civil Engineering, National Chiao Tung University, Hsinchu, Taiwan、4.Institute of Earth Science, Academia Sinica, Nankang, Taipei, Taiwan、5.Institute of Space Science, National Central University, Jhongli, Taiwan)