*Chi-Kuang Chao1,2 (1.Graduate Institute of Space Science, National Central University、2.Center for Astronautical Physics and Engineering, National Central University)
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-EM20] Recent Advances in Ionosphere Observation and Modeling through New Observation Opportunities
コンビーナ:CHIYEN LIN(Center for Astronautical Physics and Engineering, National Central University, TAIWAN)、Yen-Jung Wu(Space Sciences Laboratory, University of California, Berkeley)、Yang-Yi Sun(China University of Geosciences)、Charles Lin(Department of Earth Sciences, National Cheng Kung University)
Rapid developments in space technology are advancing our understanding of ionospheric space weather by increasing a great number of ground- and space-based observations over the recent decades. 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, such as FORMOSAT-7/COSMIC-2, ESA-SWARM NASA-ICON and -GOLD, providing a variety of observations all over the world such as airglow, temperature, neutral winds, current, ion drifts, plasma density that contribute to the understanding of middle and upper atmospheric dynamics. Increasing ground based observations are also important for coordinations with these satellite missions.
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 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 from magnetically quiescent to storm conditions as well as influences from lower atmosphere will also be solicited.
Pei-Cii Hong1、*Chi-Kuang Chao1,2 (1.Graduate Institute of Space Science and Engineering, National Central University、2.Center for Astronautical Physics and Engineering, National Central University)
*陳 佳宏1、Lin Charles1、齊藤 昭則2、山本 衛3、斎藤 享4 (1.台湾国立成功大学地球科学学科、2.京都大学大学院理学研究科地球物理学教室、3.京都大学生存圏研究所、4.国立研究開発法人海上・港湾・航空技術研究所 電子航法研究所)
*Yu-Chen Cheng1、Charles Lin1、Shih-Ping Chen1、Min-Yang Chou2 (1.Department of Earth Science, National Cheng Kung University, Tainan, Taiwan、2.COSMIC Program Office, University Corporation for Atmospheric Research Boulder, CO, USA)
*Pin-Hsuan Cheng1、Charles Lin1、Hanli Liu2 (1.Department of Earth Sciences, National Cheng Kung University、2.University Corporation For Atmospheric Research)
*Jia-Ting Lin1、Charles Lin1、CHIYEN LIN2,3、P. K. Pedatella1、Nicholas M Pedatella4,5 (1.Department of Earth Sciences, National Cheng Kung University, Taiwan、2.Center for Astronautical Physics and Engineering, National Central University, Taoyuan, Taiwan、3.Graduate Institute of Space Science, National Central University, Taoyuan, Taiwan、4.High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO, USA、5.COSMIC Program Office, University Corporation for Atmospheric Research, Boulder, CO, USA)
*Wen-Hao Yeh1、Cheng-Yung Huang1、Kun-Lin Chen1、Tzu-Pang Tseng2、Hsu-Hui Ho3、Jing-Mei Wu4、Jyun-Ying Huang3、Hsiu-Wen Li4、Ching-Chieh Lin3 (1.National Space Organization, National Applied Research Laboratories, Taiwan、2.Geoscience Australia, Australia、3.Taiwan Analysis Center for COSMIC, Central Weather Bureau, Taiwan、4.GPS Science and Application Research Center, National Central University, Taiwan)
*Yang-Yi Sun1 (1.China University of Geosciences (Wuhan))
*Tam Dao1,2、Minh Huy Le3、Brett A Carter1、Que Le2 (1.SPACE Research Centre, School of Science, RMIT University, Australia、2.Department of Physics, International University, Vietnam、3.Institute of Geophysics, Vietnam Academy of Science and Technology (VAST), Vietnam)