日本地球惑星科学連合2018年大会

講演情報

[JJ] 口頭発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS10] 古気候・古海洋変動

2018年5月23日(水) 15:30 〜 17:00 A07 (東京ベイ幕張ホール)

コンビーナ:岡崎 裕典(九州大学大学院理学研究院地球惑星科学部門)、磯辺 篤彦(九州大学応用力学研究所)、北村 晃寿(静岡大学理学部地球科学教室、共同)、佐野 雅規(早稲田大学人間科学学術院)、長谷川 精(高知大学理工学部)、岡 顕(東京大学大気海洋研究所)、加 三千宣(愛媛大学沿岸環境科学研究センター)、座長:佐野 雅規

15:45 〜 16:07

[MIS10-14] 14Cデータに見られる宇宙線イベント

★招待講演

*三宅 芙沙1 (1.名古屋大学宇宙地球環境研究所)

キーワード:放射性炭素、14Cスパイク、単年宇宙線イベント

Cosmic rays falling on the Earth mainly come from outside the solar system (Galactic Cosmic Ray: GCR ) and the sun (Solar Cosmic Ray: SCR). Incoming cosmic rays interact with the atmosphere, whence cosmic rays produce cosmogenic nuclides such as 14C. Carbon-14 is oxidized to form 14CO2 shortly thereafter its production, and is incorporated in tree-rings. Therefore, 14C contents in tree rings would be a proxy of past cosmic ray intensities.

Several past cosmic ray increase events including the AD 775 event have been detected as a rapid increase of 14C contents in tree rings, namely “14C spike”. It is considered that an origin of these events is an extreme Solar Proton Event (SPE) originated from large solar flares and coronal mass ejections. An existence of 14C spikes is important not only to understand the solar activities but also to offer an annual time marker in 14C data which can be applied to an annual radiocarbon dating and a dendrochronology. Recently, such application studies have been performed, e.g. annual age determination of a volcanic eruption of Mt. Baitoushan (AD 946) and historical wood sample of a Switzerland chapel using the AD 775 event.

In this presentation, I will introduce detected rapid 14C increase events, their origins, and application studies of 14C spikes.