日本地球惑星科学連合2019年大会

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[J] Eveningポスター発表

セッション記号 M (領域外・複数領域) » M-AG 応用地球科学

[M-AG41] 福島原発事故により放出された放射性核種の環境動態

2019年5月26日(日) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 8ホール)

コンビーナ:高橋 嘉夫(東京大学大学院理学系研究科地球惑星科学専攻)、北 和之(茨城大学理学部)、恩田 裕一(筑波大学アイソトープ環境動態研究センター)、津旨 大輔(一般財団法人 電力中央研究所)

[MAG41-P01] 放射光X線を用いた福島第一原子力発電所1号機由来の不溶性セシウム粒子中のウラン-ジルコニウム粒子の発見

*三浦 輝1栗原 雄一2山本 政儀3坂口 綾4田中 万也2桧垣 正吾5高橋 嘉夫5 (1.電力中央研究所、2.原子力研究開発機構、3.金沢大学、4.筑波大学、5.東京大学)

キーワード:福島原発事故、不溶性セシウム粒子、放射光X線分析

Introduction: A large amount of radiocesium (Cs) was emitted into environment by the Fukushima Nuclear Power Plant (FDNPP) accident in March, 2011. Adachi et al. (2013) reported glassy water-insoluble microparticles including radiocesium, called as radiocesium-bearing microparticles (Type-A particles). Based on the 134Cs/137Cs ratio calculated by Nishihara et al. (2012), Type-A particle is thought to be emitted from Unit 2 or 3 of FDNPP (Higaki et al., 2017; Miura et al., 2018). Abe et al. (2014) detected uranium (U) in Type-A particle by synchrotron radiation measurement. In addition, Ochiai et al. (2018) reported that Type-A particle has UO2 with zirconium (Zr). In contrast, Ono et al. (2017) reported new particles called as Type-B particles emitted from Unit 1. Type-B particle is different from Type-A particle in size, shape, Cs concentration and so on. We measured some Type-A and Type-B particles to clarify chemical condition of U by synchrotron radiation measurement. Difference in chemical condition of U in each particle may represent the difference of generating process or condition of each reactor unit at the accident.

Method: In this study, we collected Type-A and B particles from road dusts and non-woven fabric cloths from Fukushima by a wet separation method. After measurement of radioactivity with a high-purity germanium semiconductor detector, scanning electron microscope and energy dispersive X-ray spectroscopy analyses were performed to confirm that separated particles were Type-A or Type-B particles. X-ray fluorescence (XRF) mapping and X-ray adsorption near edge structure (XANES) measurement were performed at BL37XU (SPring-8, Hyogo). Bent Crystal Laue Analyzer (BCLA) was used to detect U peaks, because energy of U Lα emission is close to energies of rubidium Kα and strontium Kα emissions.

Results: We could detect U in Type-A and B particles using BCLA which decreased background contribution about one tenth. U-enriched area in the Type-B particle was about several microns, which is much bigger than U nano-particle in Type-A particle reported by Ochiai et al. (2018). This difference in size possibly suggested that U particle in Type-B particle was derived from melt in contrast to that in Type-A particle possibly produced from vapor. XANES measurement showed the presence of U(IV) in Type-B particle but also U(VI) in Type-A and B particles, which suggested U(VI)O2 fuel was oxidized possibly due to its exposure to air at the surface of the particles. In the spots of detecting U, we also detected Zr which is used for fuel cladding tube. It is needed to identify chemical-states of Zr and U as a future study.