X射线岩石CT的历史与现状

采用X射线CT技术无损探测岩石内部结构和裂纹演化过程 ,起源于 2 0世纪 80年代后期 ,由最初对CT图像的认识逐步深化为对岩石裂纹演化规律的分析和应用研究。基于室内岩石试件扫描断面的CT图像 ,目前在岩石变形破坏过程的实时监测、加荷条件多样化、裂纹演化规律性、裂纹宽度的定量测量、岩石裂纹三维图像重建、损伤演化与损伤变量分析、CT成果应用研究等方面取得了一系列进展。岩石CT面临的主要问题是如何获得各种试验条件下精确的CT图像及其成果的应用研究。岩石CT的生命力在于自身理论、技术发展和在相关领域的应用程度     

X射线荧光光谱法直接测定地质样品中多种痕量元素

采用低压聚乙烯镶边垫底的粉末压饼法制样,Ｘ射线荧光光谱法直接测定了地质样品中痕量元素Ａｓ、Ｇａ、Ｓｃ、Ｌａ、Ｙ、Ｃｅ、Ｗ、Ｍｏ、Ｓｎ、Ｃｏ和Ｐｂ。讨论了背景校正、谱线重叠校正、基体效应校正和仪器漂移校正等问题。利用理论α系数代替经验系数,使方法具有较高的准确度和较低的检出限。所测１１个元素的检出限在（０．３０～２．０２）×１０－６水平,精度（ＲＳＤ,ｎ＝１１）在０．９５％～１３．０％。方法经国家一级标准物质分析验证,结果与标准值相符。     

混合相中硅线石和莫来石的X射线衍射定性定量分析

对混合相中硅线石和莫来石的Ｘ射线衍射定性,定量分析表明,选取硅线石的ｄ（３３２）Ｓ峰,莫来石的ｄ（３３１）Ｍ峰或硅线石的ｄ（２２０）Ｓ峰,莫来石的ｄ（２２０）Ｍ峰放慢扫描速度,可定性分析硅线石和莫来石;选取硅线石的ｄ（３３２）Ｓ峰,莫来石的ｄ（３３１）Ｍ峰,采用计算机拟合分峰改进自清洗法,可定量分析硅线石和莫来石。经电子探针验证,实验方法准确,可行。     

2210多协议路由器的配置及应用

介绍了IBM2210路由器的特点,配置方法及其在9210工程中的应用     

广西气象计算机网络的建设和发展

介绍广西气象计算机网络的过去,现状和将来发展方向.     

应用XRF分析仪快速分析铁精矿中的Si、 S、K和TFe含量

论述了快速分析铁精矿中Si、S、K和TFe含量的现场X射线荧光技术，其分析精度、准确度均符合化学分析的误差标准，满足实际生产要求。     

气象电报收集、分发系统在业务中的应用

全省气象电报收集、分发系统是负责收集全省各观测站的气象资料，及时处理并分发到北京、香港、澳门等各个服务单位，它有易操作，报文处理迅速，易维护等特点，提高了电报的传输时效。     

Neutron Activation Analysis,Atomic Absorption and X‐Ray Fluorescence Spectrometry Review for 2006–2007

These mature analytical techniques do not show any change in publication level from the previous two years and AAS remains dominant in terms of the number of publications. The last two years have seen fewer technical improvements than in the previous review period. Some interesting papers dealing with uncertainty and quality assurance in INAA were published during 2006–2007. It is suggested that photon activation should be reconsidered because the source of electron accelerators has recently improved. A technique to preconcentrate Se for INAA determination has also been proposed. In the case of AAS, papers on analyte preconcentration continue to be more abundant than those relating to instrumental modification. Sample preparation for AAS is also active and ultrasound‐assisted leaching shows some promising applications. There were an unusual number of reviews concerned with AAS and those important to geological samples are cited here. A technique to preconcentrate Cr in water is presented and a new device to determine As and Se is showing some potential uses. Confocal X‐ray mapping continues to show interesting developments. One group developed a technique to perform XRF inside an oyster and an interesting application of μ‐XRF mapping of sediments is presented. Determination of platinum‐group elements (at μg g¹ concentrations) can be carried out very quickly with an improved XRF technique.     

The X‐ray‐infrared/submillimetre connection and the legacy era of cosmology

We review some recent results on the identification and characterisation of Active Galactic Nuclei (AGN) obtained by cross correlating X‐ray surveys with infrared and submillimetre surveys. We also look toward the scientific gains that could be achieved from an XMM‐Newton survey of the medium‐deep legacy fields that are being observed at ≈ 1–850 μm. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Using X‐ray observations to identify the particle acceleration mechanisms in VHE SNRs and “dark” VHE sources

Very high energy (VHE) γ‐ray observations have proven to be very successful in localizing Galactic acceleration sites of VHE particles. Observations of shell‐type supernova remnants have confirmed that particles are accelerated to VHE energies in supernova blast waves; the interpretation of the γ‐ray data in terms of hadronic or leptonic particle components in these objects relies nevertheless strongly on input from X‐ray observations. The largest identified Galactic VHE source class consists of pulsar wind nebulae, as detected in X‐rays. Many of the remaining VHE sources remain however unidentified until now. With X‐ray observations of these enigmatic “dark” objects one hopes to solve the following questions: What is the astrophysical nature of these sources? Are they predominantly electron or hadron accelerators? And what is their contribution to the overall cosmic ray energy budget? The paper aims to provide an overview over the identification status of the Galactic VHE source population. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)