宇宙惑星科学(P)
セッション小記号太陽地球系科学・宇宙電磁気学・宇宙環境(EM)
セッションIDP-EM20
タイトル和文Recent Advances in Ionosphere Observation and Modeling through New Observation Opportunities
英文Recent Advances in Ionosphere Observation and Modeling through New Observation Opportunities
タイトル短縮名和文Ionosphere New Observation Opportunities
英文Ionosphere New Observation Opportunities
代表コンビーナ氏名和文LIN CHIYEN
英文CHIYEN LIN
所属和文Center for Astronautical Physics and Engineering, National Central University, TAIWAN
英文Center for Astronautical Physics and Engineering, National Central University, TAIWAN
共同コンビーナ 1氏名和文Yen-Jung Wu
英文Yen-Jung Wu
所属和文Space Sciences Laboratory, University of California, Berkeley
英文Space Sciences Laboratory, University of California, Berkeley
共同コンビーナ 2氏名和文Yang-Yi Sun
英文Yang-Yi Sun
所属和文China University of Geosciences
英文China University of Geosciences
共同コンビーナ 3氏名和文Lin Charles
英文Charles Lin
所属和文Department of Earth Sciences, National Cheng Kung University
英文Department of Earth Sciences, National Cheng Kung University
発表言語E
スコープ和文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.
英文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.
発表方法口頭および(または)ポスターセッション