Session Details
[P-EM06]Mesosphere-Thermosphere-Ionosphere Coupling in the Earth's Atmosphere
Tue. May 26, 2015 6:15 PM - 7:30 PM JST
Tue. May 26, 2015 9:15 AM - 10:30 AM UTC
Tue. May 26, 2015 9:15 AM - 10:30 AM UTC
Convention Hall 2F
Convener:*Huixin Liu(Earth and Planetary Science Division, Kyushu University SERC, Kyushu University), Yuichi Otsuka(Solar-Terrestrial Environment Laboratory, Nagoya University), Libo Liu(Institute of Geology and Geophysics, Chinese Academy of Sciences), Atsuki Shinbori(Research Institute for Sustainable Humanosphere (RISH), Kyoto University)
The whole atmosphere concept is the key for the next breakthrough in solar-terrestrial science. This international session focuses on physical/chemical processes occurring in the mesosphere, thermosphere, and ionosphere (MTI) from both the poles to the equatorial region. Both quiet and disturbed states in response to lower atmospheric forcing or solar forcing are important for understanding the MTI system and its coupling to other regions. We invite presentations of observations with ground-based and/or space-borne instruments, theoretical studies, numerical simulations, and development of data analysis systems for various kinds of atmospheric variations in the MTI system.
[PEM06-P01]Observation of Ozone concentration relation to meteors echo duration distributions by a forward scattering radar
*Waleed MADKOUR1, Masa-yuki YAMAMOTO1, Satoshi MIZUMOTO1 (1.Kochi University of Tech.)
[PEM06-P02]Simultaneous observations of polar mesosphere winter echoes (PMWE) and Cosmic Noise Absorption (CNA) by the PANSY radar
*Takanori NISHIYAMA1, Kaoru SATO2, Takuji NAKAMURA1, Masaki TSUTSUMI1, Toru SATO3, Masashi KOHMA2, Koji NISHIMURA1, Yoshihiro TOMIKAWA1, Mitsumu K. EJIRI1, Takuo TSUDA4 (1.National Institute of Polar Research, 2.Department of Earth and Planetary Science, The University of Tokyo, 3.Department of Communications and Computer Engineering, Kyoto University, 4.Department of Communication Engineering and Informatics, University of Electro-Communications)
[PEM06-P03]Gravity wave activity in a wide height range of 65-110km over Syowa st. (69S), Antarctica
*Masaki TSUTSUMI1 (1.National Institute of Polar Research)
[PEM06-P04]Variability of the Equatorial Ionization Anomaly on seasonal and day to day time scales
*Shin han CHIEN1, Loren CHANG1, Huixin LIU2 (1.Institute of Space Science, National Central University, Jhongli City, Taiwan, 2.Earth and Planetary Science Division, Kyushu University SERC, Kyushu University)
[PEM06-P05]Topside Ionospheric Plasma Temperatures Retrieved From FORMOSAT-3/COSMIC Observations
*Jack C. WANG1, Loren C. CHANG1, Jann-yenq LIU1 (1.Graduate Institute of Space Science, National Central University, Taiwan)
[PEM06-P06]Development of real-time three-dimensional GPS-TEC tomography
*Shota SUZUKI1, Mamoru YAMAMOTO1, Chieh-Hung Chen2, Susumu SAITO3, Gopi Seemala1, Akinori SAITO4 (1.Research Institute for Sustainable Humanosphere, Kyoto University, 2.Department of Earth and Environmental Sciences, National Chung Cheng University, Taiwan, 3.Department of Geophysics, Graduate School of Science, Kyoto University, 4.Navigation Systems Department, Electronic Navigation Research Institute)
[PEM06-P07]Performance evaluation of low-cost airglow camera for mesospheric gravity wave measurements
*Shin SUZUKI1, Kazuo SHIOKAWA1 (1.Solar-Terrestrial Environment Laboratory, Nagoya University)
[PEM06-P08]The FORMOSAT-3/COSMIC Radio Occultation Data Assimilated to NCAR/TIE-GCM to study the horizontal winds in the ionosphere
*Ming-quey CHEN1, Yung-chih SU1, Shih-hao CHAO1 (1.Grad. Inst. of Space Science, National Central Univ., Taiwan)
[PEM06-P09]Periodic variations in the thermospheric density
*Huixin Liu1, Hiroyuki Tsubosaki1 (1.Kyushu University, Japan)
[PEM06-P10]Evaluation of EEJ variation due to Ultra Fast Kelvin Waves using the Kyushu-GCM and the Quasi-3D dynamo model
*Kenshi GOYA1, Saburo MIYAHARA2, Ying-Wen CHEN3 (1.Dept. of Earth and Planetary Sci., Kyushu University, 2.Kyushu University, 3.JAMSTEC)
[PEM06-P11]The relationship between the electric field in the lower atmosphere and Sq variations
*Akihiro IKEDA1, G. Maria Cardinal2 (1.Kagoshima National College of Technology, 2.International Center for Space Weather Science and Education)