镍磷对陶瓷-金属结合剂性能与结构的影响

采用化学镀镍包覆陶瓷结合剂粉体的方法制备陶瓷-金属结合剂.结合强度测试仪、XRD、SEM等检测手段,研究了镍磷含量对陶瓷-金属结合剂性能与结构的影响.结果 表明:在镍磷含量20wt;的陶瓷-金属结合剂中,陶瓷熔融贯通一起成骨架,金属相与陶瓷相交错镶嵌紧密结合,陶瓷-金属结合剂具有较佳的力学性能,抗折强度和抗冲击强度分别为155.22 MPa和3.11 kJ/m2,相比陶瓷结合剂分别提高98.7;和87.3;;镍磷含量适当的陶瓷-金属结合剂磨具,既保留了陶瓷结合剂磨具的体系结构,又具有金属与陶瓷融合一体的结合剂性能,其各项性能得到改善.     

Multi-wavelength study of MGRO J2019+37

MGRO J2019+37,within the Cygnus region,is a bright extended source revealed by Milagro at 12-35 TeV.This source is almost as bright as the Crab Nebula in the northern sky,but is not confirmed by ARGO-YBJ around the TeV scale.Up to now,no obvious counterpart at low energy wavelengths has been found.Hence,MGRO J2019+37 is a rather mysterious object and its VHEγ-ray emission mechanism is worth investigating.In this paper,a brief summary of the multi-wavelength observations from radio toγ-rays is presented.All the available data from XMM-Newton and INTEGRAL at X-ray,and Fermi-LAT atγ-ray bands,are used to get constraints on its emission flux at low energy wavelengths.Then,its possible counterparts and the VHE emission mechanism are discussed.     

W-In体系溶质晶界偏聚行为的第一性原理计算

基于第一性原理构建了钨基合金体系的溶质偏聚模型,以W-In体系为例研究了不同浓度下溶质的晶界偏聚行为和成键特征,从电子结构层面揭示了W-In体系的键合作用,预测了W-In体系界面稳定性随溶质浓度的变化规律.结合键布居、电荷密度、差分电荷密度和态密度等电子结构分析,发现了W-In体系中溶质原子在偏聚过程中的键性转变特征,阐明了W-In键由晶粒内部的离子键过渡为晶界区域强共价键的微观机理.模型计算首次得到了W-In体系中溶质本征偏聚能随In浓度的非单调变化规律,结合键合作用和能量分析揭示了溶质浓度对本征偏聚能的影响机制.计算预测了W-In体系达到高热稳定性所需的最佳溶质浓度范围和应避开的溶质浓度范围.本研究为具有高温稳定性的钨基合金材料的设计与制备提供了理论基础和定量化指导.     

三维荧光光谱结合物理和数学分离研究溶解性有机质组成

采用分子排阻色谱和激发/多波段发射荧光检测器,结合三维荧光光谱和平行因子分析,研究了新、老填埋垃圾渗滤液中溶解性有机质( DOM)的组成。实验结果表明,两种渗滤液来源的DOM均含有类蛋白和类腐殖质物质。在新填埋垃圾渗滤液中,类蛋白物质有4种存在形态,包括大分子蛋白质形态、高/低分子量腐殖质结合态和多肽/氨基酸形态;在老填埋垃圾渗滤液DOM中,类蛋白物质只有两种形态,分别为大分子蛋白质形态和腐殖质结合态。相比于分子排阻色谱,三维荧光光谱结合平行因子分析能够分辨出腐殖质和非腐殖质结合态的类蛋白物质,但不能有效区分蛋白质和以多肽/氨基酸形态存在的类蛋白物质。结果表明,三维荧光光谱结合平行因子分析和分子排阻色谱,可以表征DOM中不同形态分布的类蛋白和类腐殖质物质。     

Performances and long-term stability of the LHAASO-KM2A prototype array

A prototype array for the LHAASO-KM2A, which consists of 42 detector units and fully overlaps the ARGO-YBJ experiment, was set up at the Yangbajing cosmic ray observatory and has been in stable operation since Octoter 2010. The resulting performances of the KM2A electromagnetic particle detector prototypes fully meet the design requirements. Through hybrid observation of cosmic ray showers with the ARGO-YBJ experiment, the performances and long-term stability of the prototype array are tested and the results are consistent with expectation. The cosmic ray moon shadow observed by the prototype array is also presented.     

Design and performances of electromagnetic particle detector for LHAASO-KM2A

In the Large High Altitude Air Shower Observatory (LHAASO) project, the one kilometer square extensive air shower array (KM2A) is the the largest detector array in terms of effective area. It consists of 5635 electromagnetic particle detectors (EDs) and 1221 muon detectors (MDs). Each ED is composed of 16 scintillator tiles readout by wavelength-shifting fibers that are bundled and attached by a 25 mm PMT. The design of the unit and its performances, such as photoelectron yield, time resolution and uniformity, are discussed in detail. An assembling scheme for the whole ED is established to guarantee the uniformity throughout all 16 tiles in a single ED and all EDs in mass production.