Sun. May 20, 2018 9:00 AM - 10:30 AM 304 (3F International Conference Hall, Makuhari Messe)

[EE] Oral
| P (Space and Planetary Sciences)
| P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM13] Study of coupling processes in solar-terrestrial system

convener:Mamoru Yamamoto(Research Institute for Sustainable Humanosphere, Kyoto University), Yasunobu Ogawa(National Institute of Polar Research), Satonori Nozawa(名古屋大学宇宙地球環境研究所, 共同), Akimasa Yoshikawa(Department of Earth and Planetary Sciences, Kyushu University), Chairperson:Yamamoto Mamoru, Nozawa Satonori

Sun. May 20, 2018 1:45 PM - 3:15 PM 304 (3F International Conference Hall, Makuhari Messe)

[EE] Oral
| P (Space and Planetary Sciences)
| P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM13] Study of coupling processes in solar-terrestrial system

convener:Mamoru Yamamoto(Research Institute for Sustainable Humanosphere, Kyoto University), Yasunobu Ogawa(National Institute of Polar Research), Satonori Nozawa(名古屋大学宇宙地球環境研究所, 共同), Akimasa Yoshikawa(Department of Earth and Planetary Sciences, Kyushu University), Chairperson:Yoshikawa Akimasa, Yamamoto Mamoru

Sun. May 20, 2018 9:00 AM - 10:30 AM 303 (3F International Conference Hall, Makuhari Messe)

[EE] Oral
| P (Space and Planetary Sciences)
| P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM15] Dynamics in magnetosphere and ionosphere

9:15 AM - 9:30 AM

[PEM15-02] Red line aurora in the dayside cusp for northward IMF

*Satoshi Taguchi¹, Yushin Oda¹, Keisuke Hosokawa² (1.Department of Geophysics, Graduate School of Science, Kyoto University, 2.Department of Communication Engineering and Informatics, University of Electro-Communications)

Mon. May 21, 2018 3:30 PM - 5:00 PM Poster Hall (International Exhibition Hall7, Makuhari Messe)

[EE] Poster
| P (Space and Planetary Sciences)
| P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM15] Dynamics in magnetosphere and ionosphere

[PEM15-P04] Characteristic distance between mesoscale auroral brightenings along the equatorward boundary of the cusp

*Satoshi Kose¹, Satoshi Taguchi¹, Keisuke Hosokawa² (1.Department of Geophysics, Graduate School of Science, Kyoto University, 2.Department of Communication Engineering and Informatics, University of Electro-Communications)

[PEM15-P05] Spatial structures of polar rain during the period of poleward moving cusp auroras

*Kohei Takasu¹, Satoshi Taguchi¹, Yushin Oda¹, Keisuke Hosokawa² (1.Department of Geophysics, Graduate School of Science, Kyoto University, 2.Department of Communication Engineering and Informatics, University of Electro-Communications)

[PEM15-P06] Plasma flow enhancements preceding a large-scale moving cusp aurora

*Yunosuke Nagafusa¹, Satoshi Taguchi¹, Yasunobu Ogawa², Keisuke Hosokawa³ (1.Graduate School of Science, Kyoto University, 2.National Institute of Polar Research, 3.Department of Communication Engineering and Informatics, University of Electro-Communications)

Mon. May 21, 2018 5:15 PM - 6:30 PM Poster Hall (International Exhibition Hall7, Makuhari Messe)

[EE] Evening Poster
| P (Space and Planetary Sciences)
| P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM15] Dynamics in magnetosphere and ionosphere

[PEM15-P04] Characteristic distance between mesoscale auroral brightenings along the equatorward boundary of the cusp

*Satoshi Kose¹, Satoshi Taguchi¹, Keisuke Hosokawa² (1.Department of Geophysics, Graduate School of Science, Kyoto University, 2.Department of Communication Engineering and Informatics, University of Electro-Communications)

[PEM15-P05] Spatial structures of polar rain during the period of poleward moving cusp auroras

*Kohei Takasu¹, Satoshi Taguchi¹, Yushin Oda¹, Keisuke Hosokawa² (1.Department of Geophysics, Graduate School of Science, Kyoto University, 2.Department of Communication Engineering and Informatics, University of Electro-Communications)

[PEM15-P06] Plasma flow enhancements preceding a large-scale moving cusp aurora

*Yunosuke Nagafusa¹, Satoshi Taguchi¹, Yasunobu Ogawa², Keisuke Hosokawa³ (1.Graduate School of Science, Kyoto University, 2.National Institute of Polar Research, 3.Department of Communication Engineering and Informatics, University of Electro-Communications)

Tue. May 22, 2018 5:15 PM - 6:30 PM Poster Hall (International Exhibition Hall7, Makuhari Messe)

[JJ] Evening Poster
| P (Space and Planetary Sciences)
| P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM18] Physics and Chemistry in the Atmosphere and Ionosphere

[PEM18-P09] Local modeling of the thermosphere-ionosphere dynamics in the polar region

*Ooigawa Tomokazu¹, Hiroyuki Shinagawa², Satoshi Taguchi¹ (1.Department of Geophysics, Graduate School of Science, Kyoto University, 2.National Institute of Information and Communications Technology)

Satoshi Taguchi

Convener, Chairperson

[P-EM13] Study of coupling processes in solar-terrestrial system

[P-EM13] Study of coupling processes in solar-terrestrial system

Speaker, Author, Co-Author

[P-EM15] Dynamics in magnetosphere and ionosphere

[PEM15-02] Red line aurora in the dayside cusp for northward IMF

[P-EM15] Dynamics in magnetosphere and ionosphere

[PEM15-P04] Characteristic distance between mesoscale auroral brightenings along the equatorward boundary of the cusp

[PEM15-P05] Spatial structures of polar rain during the period of poleward moving cusp auroras

[PEM15-P06] Plasma flow enhancements preceding a large-scale moving cusp aurora

[P-EM15] Dynamics in magnetosphere and ionosphere

[PEM15-P04] Characteristic distance between mesoscale auroral brightenings along the equatorward boundary of the cusp

[PEM15-P05] Spatial structures of polar rain during the period of poleward moving cusp auroras

[PEM15-P06] Plasma flow enhancements preceding a large-scale moving cusp aurora

[P-EM18] Physics and Chemistry in the Atmosphere and Ionosphere

[PEM18-P09] Local modeling of the thermosphere-ionosphere dynamics in the polar region