日本地球惑星科学連合2019年大会

講演情報

[J] 口頭発表

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-EM19] 太陽物理学の最前線

2019年5月26日(日) 15:30 〜 17:00 A03 (東京ベイ幕張ホール)

コンビーナ:今田 晋亮(名古屋大学宇宙地球環境研究所)、横山 央明(東京大学大学院理学系研究科)、清水 敏文(宇宙航空研究開発機構宇宙科学研究所)、勝川 行雄(自然科学研究機構国立天文台)、座長:今田 晋亮

15:30 〜 15:45

[PEM19-01] 太陽-ジオスペース結合過程の理解に向けて:第25太陽活動周期の課題

★招待講演

*三好 由純1今田 晋亮1 (1.名古屋大学宇宙地球環境研究所)

キーワード:太陽-ジオスペース結合、第25活動周期

One of the major goals of solar-terrestrial physics is to understand how the transfer of Sun and solar wind energy into the Geospace and vice versa. In the last decade, there have been several flagship missions in Geospace; NASA/THEMIS, Van Allen Probes, and MMS, and JAXA/Arase, making important contributions to our understandings of how the Geospace responds on variations of Sun and solar wind. Solar atmosphere is also observed and monitored by modern satellite, such as Hinode, and Solar Dynamics Observatory. The present solar cycle (cycle 24) is one of the weakest cycles in these 100 years. Existing missions successfully observe several abnormal phenomena during weak solar cycle, such as extremely low-density solar wind, strong asymmetry for solar polar magnetic field, or relatively weak geomagnetic activities. For example, large flux enhancements of the outer belt associated with huge magnetic storms have not observed in cycle 24. Further, a lot of cycle prediction studies suggest that next solar cycle (cycle 25) is also as weak as cycle 24. There are also several preexisting and under-preparing missions which will be flagship missions during solar cycle 25. In this presentation, we briefly review highlights from these missions and discuss what subjects are important for the next decade, i.e, the 25th solar cycle to understand coupling process between Sun and Earth.