日本地球惑星科学連合2014年大会

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セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT38_30PM1] 地球構成物質のレオロジーと物質移動

2014年4月30日(水) 14:15 〜 16:00 511 (5F)

コンビーナ:*大内 智博(愛媛大学地球深部ダイナミクス研究センター)、桑野 修(独立行政法人海洋研究開発機構)、清水 以知子(東京大学大学院理学系研究科地球惑星科学専攻)、座長:辻野 典秀(岡山大学・地球物質科学研究センター)

15:30 〜 15:45

[SIT38-P05_PG] 強磁場プロセスを用いた配向性フォルステライト多結晶体の創製

ポスター講演3分口頭発表枠

*小泉 早苗1平賀 岳彦1鈴木 達2目 義雄2 (1.東京大学地震研究所、2.物質・材料研究機構)

キーワード:フォルステライト, 多結晶体, 磁場, 配向, CPO

It is well known that the crystallographic preferred orientation (CPO) of minerals is commonly produced in the Earth's interior. Thus, it is important to understand the physical properties of the mineral aggregates that exhibit CPO. However, silicate minerals are often feeble magnetic and have small anisotropic susceptibilities so that it is difficult to apply a magnetic field effectively to rotate the mineral particles. Tendency of finer particles to spontaneously agglomerate due to strong attractive interactions (van der Waals forces) add further difficulty. We used a technique of slip casting in a high magnetic field (12T) to align certain crystallographic axis of mineral particles. For the particles to rotate easily in the solvent under a strong magnetic field, we improve the method of deflocculating. To control the surface potential of the particles, we applied various types of polymer modification. Vacuum sintering of the powders that were composed of the aligned particles was expected to produce a polycrystalline material aggregate that exhibits CPO. The resultant materials were characterized by X-ray powder diffraction (XRD), secondary electron microscope (SEM) and Electron Backscatter Diffraction (EBSD).
The specimen exposed to a strong magnetic field exhibits preferential A-axis alignment to the magnetic direction. Those synthetic specimens allow us to examine the effect of CPO on the physical properties of the earth's materials in future room experiments.