日本地球惑星科学連合2023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-EM09] Space Weather and Space Climate

2023年5月25日(木) 13:45 〜 15:00 101 (幕張メッセ国際会議場)

コンビーナ:片岡 龍峰(国立極地研究所)、Antti A Pulkkinen(NASA Goddard Space Flight Center)、Mary Aronne中村 紗都子(名古屋大学宇宙地球環境研究所)、Chairperson:Mary Aronne中村 紗都子(名古屋大学宇宙地球環境研究所)

14:15 〜 14:30

[PEM09-15] Statistical analyses for the relationship between solar activities and aurora candidates in ancient Chinese historical records

*Po-Han Lee1Jann-Yenq Liu1,2,3、Yuh-Ing Chen4 (1.Department of Space Science and Engineering, National Central University, Taiwan、2.Center for Astronautical Physics and Engineering, National Central University, Taoyuan City, TAIWAN、3.Center for Space and Remote Sensing Research, National Central University, Taoyuan City, TAIWAN、4.Graduate Institute of Statistics, National Central University, Taoyuan City, TAIWAN)


キーワード:aurora, solar activity

Continuous observations at specified locations and chronicling of astronomical phenomena provide unique opportunities to reveal the ancient space weather. In this study, 508 aurora candidates in Chinese official historical records during 511-1912 are converted into quantitative data with its color, location, and appearance time. Statistic results show that aurora candidates were observed significantly during high solar activity periods, especially that in the red color. However, the relationship between solar activities and aurora candidates of white, blue, as well as the other colors are not significant with 95% confidence intervals. White aurora candidates were observed nearly equally across four seasons. By contrast, only 13% of red aurora candidates occurred in summer; and most of the blue aurora candidates were in summer and autumn. The red aurora candidates mainly appeared at middle latitudes, similar to the middle latitude aurora, while white and blue aurora candidates are under study. In summary, the statistical results on the historical records of all aurora candidates show that auroras, especially the red one, appear more frequent during high solar activity periods.