日本地球惑星科学連合2019年大会

講演情報

[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)

[PEM14-P01] The Daytime and Nighttime Mapped Whistler Plasmapause Observed by DEMETER

*ChaoYen Chen1,2Tiger 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)

キーワード:Plasmapause position, Whistler, DEMETER satellite

This paper investigates the plasmapause positions in the ionosphere by measurement of the whistler count probed by DEMETER (Detection of Electro-Magnetic Emissions Transmitted from Earthquake Regions) satellite in the daytime at 1030 LT (local time) and the nighttime at 2230 LT during 2005-2010. The whistler finds the plasmapause position which can be clearly allocated in both daytime and nighttime. We examine the nighttime/daytime plasmapause in various longitudes, solar activities, seasons, and geomagnetic actives. Results show that the daytime plasmapause appears in the equatorward side of the nighttime one. Both the daytime and nighttime plasmapause are sensitive to solar activity, which move equatorward form the low to high solar activity in the study period. The seasonal variation of the plasmapause are rather random and insignificant. During magnetic disturbed condition, the plasmapause tend to move equatorward.