日本地球惑星科学連合2015年大会

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セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS24] ガスハイドレートと地球環境・資源科学

2015年5月27日(水) 18:15 〜 19:30 コンベンションホール (2F)

コンビーナ:*戸丸 仁(千葉大学理学部地球科学科)、八久保 晶弘(北見工業大学環境・エネルギー研究推進センター)、森田 澄人(独立行政法人 産業技術総合研究所 地圏資源環境研究部門)

18:15 〜 19:30

[MIS24-P03] 画像解析法による砂の粒度分析について

*木村 匠1伊藤 拓馬2金子 広明1皆川 秀紀1 (1.産業技術総合研究所メタンハイドレート研究センター貯留層特性解析チーム、2.産業技術総合研究所メタンハイドレート研究センター貯留層特性解析チーム(現・地球環境産業技術研究機構))

キーワード:粒度分析, 画像解析法, レーザー回折法, 砂, リングせん断

Grain size is a fundamental property of earth materials. However, no two of the many techniques yield a consistent measurement of this property; thus, elucidating the relationships among different methods is valuable for understanding what constitutes grain size. This study compares the grain size distributions analyzed by optical microscopy/digital image (Morphologi G3 instrument (Malvern Ltd; the UK)) and those analyzed by laser diffraction. In most of the investigated samples, the size distributions obtained by both methods were very similar. However, a shift toward a coarser grain-size distribution was observed in the optical microscopy analysis of finer sand samples, and the frequency distribution was broadened. The fractions of sand and silt size fractions were also consistent between the two methods, but optical microscopy indicated a smaller clay size fraction than the laser diffraction method. The median particle size (30–200 μm) was similar in both methods. The standard deviation was lower in the optical microscopy method than that in the laser diffraction method. We conclude that optical microscopy is a useful technique for determining the grain size distribution. Additionally, we investigated the particle shape and particle size in the experimental fault formed by ring-shearing test. This study is financially supported by METI and Research Consortium for Methane Hydrate Resources in Japan (the MH21 Research Consortium).