日本地球惑星科学連合2021年大会

講演情報

[E] ポスター発表

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-EM08] 宇宙天気・宇宙気候

2021年6月5日(土) 17:15 〜 18:30 Ch.03

コンビーナ:片岡 龍峰(国立極地研究所)、A Antti Pulkkinen(NASA Goddard Space Flight Center)、草野 完也(名古屋大学宇宙地球環境研究所)、坂口 歌織(情報通信研究機構)

17:15 〜 18:30

[PEM08-P09] Simultaneous observation of cosmic rays with muon detector and neutron monitor at the Syowa station in the Antarctic

*加藤 千尋1、宗像 一起1、門倉 昭2、片岡 龍峰2、三宅 晶子3、Evenson Paul4、浅野 駿太1 (1.信州大学、2.国立極地研究所、3.茨城工業高等専門学校、4.University of Delaware)

キーワード:宇宙線、大気効果

Since 2018.2, simultaneous observation of cosmic ray muon and neutron is continued. The operation is quite stable and its duty cycle is higher than 94%. These detectors are showing their usefulness by responding to, for example, a peculiar CME event in August 2018. There is another interesting event in September 2019. A Sudden Stratospheric Warming (SSW) was observed and muon counts responded to the SSW. This response is caused by that muon counts on the ground are affected by high altitude temperature. Temperature effect on CR muon now can be corrected with high altitude temperature data. There is, however, some matter of research about how the method works. This event seems to be valuable to improve correction method. We describe a character of muon and neutron data accumulated during the last three years and discuss potential use in studying atmospheric effect on CR muon and neutron count rates.