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 S (固体地球科学) » S-VC 火山学

[S-VC46] 火山噴火のダイナミクスと素過程

2015年5月25日(月) 09:00 〜 10:45 304 (3F)

コンビーナ:*小園 誠史(東北大学大学院理学研究科地球物理学専攻)、鈴木 雄治郎(東京大学地震研究所)、奥村 聡(東北大学大学院理学研究科地学専攻地球惑星物質科学講座)、座長:奥村 聡(東北大学大学院理学研究科地学専攻地球惑星物質科学講座)

10:15 〜 10:30

[SVC46-13] デジタル画像解析を援用した降下火山灰の形状・流速同時測定の試行

*服部 康男1中尾 圭佑1須藤 仁1 (1.電力中央研究所)

キーワード:沈降速度, 可視化流速計測, 室内実験, 火山灰輸送-堆積モデル

Accurate descriptions of terminal velocity of ash-fall are practical interest in volcanic ash risk assessment on critical infrastructure (e.g. Wardman et al. 2012). Numerical simulations with an ash transport- and deposition-model, which has a capability to estimate spatial- and temporal-distributions of ash concentration and deposition, have become a powerful tool of the risk assessment (e.g. Folch 2012). Such simulations give the solution of governing equations on ash transport processes with numerical procedures. The governing equations include some empirical formulas with assumptions. Also for the estimation of terminal velocity of ash-fall, many empirical formulas have been already reported, but there exists considerable scattering of calculations among them (e.g Folch 2012).

In the present study, we examined a measurement for shape and velocity of ash-fall by employing a digital image analysis technique. We configured the experimental setup based on a shadowgraph particle measurement system of Dantec Dynamics to deal with non-spherical particles. The particles were illuminated by high-intensity pulsed lasers, Nd: YAG laser, with an optical diffuser. A CCD camera was placed in front of the light source, and the camera was equipped with a long-distance microscope lens to obtain visualized images of small particles. We carried out a trial measurement for sedimentation of corrected ash and discussed the optimization of measurement parameters and relationship between shape and velocity of ash-fall in a laboratory test. More details will be presented in the presentation, and we believe that our study must be helpful to develop the numerical simulations for evaluation of volcanic ash risk.

The authors wish to express our gratitude to Mr. Y. Futawatari of Dantec Dynamics, Ltd., Mr. T. Sato and Mr. K. Ota for helpful comments on the design of the optical setup, and to Mr. K. Toshida, Dr. D. Miura and Dr. S. Takeuchi for fruitful discussions on this study.