Three dimensional simulation of fluid flow in X‐ray CT images of porous media

A numerical scheme is developed in order to simulate fluid flow in three dimensional (3‐D) microstructures. The governing equations for steady incompressible flow are solved using the semi‐implicit method for pressure‐linked equations (SIMPLE) finite difference scheme within a non‐staggered grid system that represents the 3‐D microstructure. This system allows solving the governing equations using only one computational cell. The numerical scheme is verified through simulating fluid flow in idealized 3‐D microstructures with known closed form solutions for permeability. The numerical factors affecting the solution in terms of convergence and accuracy are also discussed. These factors include the resolution of the analysed microstructure and the truncation criterion. Fluid flow in 2‐D X‐ray computed tomography (CT) images of real porous media microstructure is also simulated using this numerical model. These real microstructures include field cores of asphalt mixes, laboratory linear kneading compactor (LKC) specimens, and laboratory Superpave gyratory compactor (SGC) specimens. The numerical results for the permeability of the real microstructures are compared with the results from closed form solutions. Copyright © 2004 John Wiley & Sons, Ltd.     

Room temperature solid-state detectors for Gamma ray burst spectroscopy

We have evaluated several solid state detectors which offer excellent energy resolution at room temperature for soft X-rays. For soft X-rays (< 1 keV to 20 keV), silicon P-intrinsic-N (PIN) and avalanche-mode photodiodes (APD's) have been studied. Using commercially available charge sensitive pre-amplifiers, these photodiodes provide 1 keV resolution without cooling. Their detection efficiencies are limited to about 20 keV and 15 keV, respectively. To overcome this constraint, we have studied thick (1.5 mm) PIN detectors made by Micron Semiconductor Ltd., U.K., as well as compound semiconducting materials with high Z constituents such as CZT and PbI₂. PbI₂ allows high detection efficiencies of photons up to 100 keV with detectors 100–300 microns thick. These new detectors offer the capability to study the low-energy spectral evolution of Gamma ray bursts (GRBs). A matrix of these detectors could be used as an image plane detector with moderate spatial resolution for imaging.     

湖南黄金洞金矿毒砂中Au赋存状态的电子探针研究

本文利用ＪＸＡ－８８００Ｍ超大型电子探针，以湖南黄金洞金矿含金毒砂为研究对象。利用金特征Ｘ－射线扫描方法和微区含金含量，对不可见金赋存状态的研究方法和温试条件进行了探索，先观察背散射电子图像，排除金在含金矿物毒砂中呈显显微颗粒存在的可能性，继而用ＬｉＦ晶体测定金Ｌ＝８８．７６Ｌａｌ峰位，然后逐渐放大倍数（ｘ３００，ｘ１０００，ｘ５０００，ｘ３００００，ｘ２０００００）进行金特征，Ｘ－射线连续测量，，结果发现金元素总 是均匀分布在重砂中，从而证实了金呈品格金形式存在的推测。     

冬季青藏高原大气热状况分析Ⅱ：年际变化

通过诊断3套再分析资料的非绝热加热场,研究冬季青藏高原上空大气的热力特征.结果表明,与夏季为强热源的特征不同,冬季高原上空不是欧亚大陆上最强的冷源中心.冬季高原上空整体是偏弱的冷源,在高原西侧及东南地区上空甚至出现非绝热加热正值区,这一分析对以往研究提出的高原是冷源的特性给出了修正.各种非绝热加热分量的诊断表明,冬季高原上空这种总的非绝热加热分布主要是由于高原主体的长波辐射冷却较周边地区弱,以及西侧至东南地区凝结潜热释放造成的.为了说明再分析的非绝热加热资料对冬季高原上空大气的这种热力特征描述的可信性,文中还利用了地表辐射能量、TRMM及PREC/L降水、垂直速度等资料进一步辅助分析,证实了由于高原位势较高造成大气整层温度偏低,向外长波辐射偏少,以及高原地势的隆起造成局地较强的上升运动,高原西侧至东南角降水大值区潜热偏大,最终造成高原上空总非绝热加热负值偏小.最后理想高原隆起的水球试验结果说明,冬季,高原的存在减弱了陆地上空的冷却效应,因而其上为弱冷源,再次证实了资料分析的结果.