[EE] Oral
P (Space and Planetary Sciences) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment
Thu. May 24, 2018 10:45 AM - 12:15 PM 303 (3F International Conference Hall, Makuhari Messe)
convener:ALEXEI DMITRIEV(Institute of Space Science, National Central University, Jungli City, Taiwan), Yoshizumi Miyoshi(Institute for Space-Earth Environmental Research, Nagoya University), Chairperson:Miyoshi Yoshizumi(ISEE, Nagoya University)
Time intervals of declining solar activity are dominated by so-called recurrent storms. They are produced mainly by high speed streams (HSS) of the solar wind coming from coronal holes. A HSS is preceded by a co-rotating interaction region (CIR), where the fast stream interacts with slow solar wind. Recurrent magnetic storms are weak but they cause intense chorus activity, which leads to the acceleration of the magnetospheric electrons up to relativistic energies. These effects are comprehensively investigated now by the Van Allen and ERG space missions. Strong variations of interplanetary electric field in HSSs and precipitation of magnetospheric particles at middle and high latitudes disturb the ionosphere, thermosphere and atmosphere for several days or even weeks. This results in significant energy deposition, which is even greater than strong but short transient storms produced by CMEs. The role of recurrent storms in disturbances of the ionosphere, thermosphere and atmosphere has been under intense investigation during the last several years. Presentation of recent experimental results from space missions, such as modern Van Allen Probes, ERG, COSMIC, Swarm etc., ground-based networks as well as prediction of models on these subjects are encouraged.
10:45 AM - 11:00 AM
*Ryuho Kataoka1, Yoshizumi Miyoshi2 (1.National Institute of Polar Research, 2.ISEE, Nagoya University)
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11:00 AM - 11:15 AM
Oksana Mandrikova1, *Nadezhda Fetisova1, Yury Polozov1 (1.Institute of Cosmophysical Research and Radio Wave Propagation, Far Eastern Branch of the Russian Academy of Sciences)
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11:15 AM - 11:30 AM
*Konstantin Ratovsky1, Irina Medvedeva1, Maxim Klimenko2,3, Nikolay Chirik2,3, ALEXEI DMITRIEV4,5, Alla Suvorova4,5 (1.Institute of Solar-Terrestrial Physics SB RAS, 2.West Department of Pushkov IZMIRAN, RAS, 3.Immanuel Kant Baltic Federal University, 4.National Central University, 5.Moscow State University)
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11:30 AM - 11:45 AM
*Yi Chung Chiu1, Loren Chang1, Yi Duann1, ALEXEI DMITRIEV1, Irina Medvedeva2, Konstantin Ratovsky2 (1.Institute of Space Science, National Central University, 2.Russian Academy of Sciences, Russian Federation)
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11:45 AM - 12:00 PM
*Wen Yi1,4,2, Xianghui Xue1,4,5, Iain Reid3,2, Joel Younger3,2, Andrew Spargo2, Damian Murphy6, Tingdi Chen1,4, Xiankang Dou1 (1.CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, 2.School of Physical Sciences, University of Adelaide, Adelaide, 3.ATRAD Pty Ltd., Thebarton, South Australia, Australia, 4.Mengcheng National Geophysical Observatory, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China, 5.Synergetic Innovation Center of Quantum Information and Quantum Physics, University of Science and Technology of China, Hefei, China, 6.Australian Antarctic Division, Kingston, Tasmania, Australia)
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12:00 PM - 12:15 PM
*Irina Medvedeva1, Konstantin Ratovsky1 (1.Institute of Solar-Terrestrial Physics SB RAS)
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