日本地球惑星科学連合2018年大会

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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-EM11] Effects of recurrent storms: from the heliosphere to the atmosphere

2018年5月24日(木) 10:45 〜 12:15 303 (幕張メッセ国際会議場 3F)

コンビーナ:DMITRIEV ALEXEI(Institute of Space Science, National Central University, Jungli City, Taiwan)、三好 由純(名古屋大学宇宙地球環境研究所)、座長:三好 由純(名古屋大学宇宙地球環境研究所)

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.

11:15 〜 11:30

*Konstantin Ratovsky1Irina Medvedeva1Maxim Klimenko2,3Nikolay Chirik2,3ALEXEI DMITRIEV4,5Alla 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)

11:45 〜 12:00

*Wen Yi1,4,2Xianghui Xue1,4,5Iain Reid3,2Joel Younger3,2Andrew Spargo2Damian Murphy6Tingdi Chen1,4Xiankang 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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