[P-EM28_29AM2] Magnetosphere-Ionosphere Coupling

12:15 PM - 12:30 PM

[PEM28-06] Comparing the ionospheric plasma drift obtained from the global MHD simulation and that measured by SuperDARN radars

*Satoko SAITA¹, Shigeru FUJITA², Akira KADOKURA³, Takashi TANAKA⁴, Akira sessai YUKIMATU³, Yoshimasa TANAKA³, Shinichi OHTANI⁵, Ken T. MURATA⁶, Tomoyuki HIGUCHI⁷ (1.Research Organization of Information and Systems, 2.Meteorological College, 3.National Institute of Polar Research, 4.International Center for Space Weather Science and Education, Kyushu University, 5.Johns Hopkins University Applied Physics Laboratory, 6.National Institute of Information and Communications Technology, 7.The Institute of Statistical Mathematics)

Tue. Apr 29, 2014 2:15 PM - 4:00 PM 413 (4F)

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

[P-EM28_29PM1] Magnetosphere-Ionosphere Coupling

3:30 PM - 3:45 PM

[PEM28-12] Inversion method for estimating the helium ion density distribution in the plasmasphere based on IMAGE/EUV data

*Shin'ya NAKANO¹, Mei-ching FOK², Pontus C. BRANDT³, Tomoyuki HIGUCHI¹ (1.The Institute of Statistical Mathematics, 2.NASA Goddard Space Flight Center, 3.The Johns Hopkins University Applied Physics Laboratory)

Wed. Apr 30, 2014 4:15 PM - 5:00 PM 211 (2F)

Oral
| Symbol S (Solid Earth Sciences)
| S-TT Technology & Techniques

[S-TT60_30PM2] Creating future of solid Earth science with high performance computing (HPC)

4:15 PM - 4:30 PM

[STT60-08] Cloud Services to Release Techniques of Data Assimilation

*Hiromichi NAGAO¹, Tomoyuki HIGUCHI² (1.Earthquake Research Institute, The University of Tokyo, 2.The Institute of Statistical Mathematics)