电弧离子镀NiCrAlY涂层高温氧化行为

采用电弧离子镀技术在铸造镍基合金上沉积ＮｉＣｒＡｌＹ涂层，涂层均匀、致密与基体结合良好。测定了Ｋ１７合金和ＮｉＣｒＡｌＹ涂层在９００～１７００℃的氧化动力学曲线，试验结果表明： Ｋ１７合金和 ＮｉＣｒＡｌＹ涂层在不同温度静态空气中氧化动力学曲线基本符合抛物线规律。９００℃和１０００℃时，Ｋ１７合金上沉积ＮｉＣｒＡｌＹ涂层后，明显改善了合金的抗氧化性。１１００℃时，涂层的保护作用降低。随着氧化温度升高，涂层和基体之间元素扩散能力增强，Ｔｉ从基体扩散到涂层表面形成氧化物是导致涂层抗氧化性降低的原因之一。氧化膜从涂层上剥落下来，也导致了涂层抗氧化能力降低。     

GCr15钢离子注入表面改性研究

对航空轴承用钢ＧＣｒ１５进行了硼离子、氮离子及其复合注入试验。利用扫描电镜和Ｘ射线衍射仪对注入层的组织结构进行了分析，并测试了注入层的硬度、耐磨性、耐蚀性。结果表明：ＧＣｒ１５离子注入层形成了多种弥散相和非晶相，表层的残余奥氏体含量也有所减少。表层的硬度、耐磨性以及耐蚀性经离子注入后明显增加。     

水反应金属燃料发动机三维两相燃烧数值模拟

用三维湍流N-S方程及颗粒轨道模型描述水反应金属燃料发动机内部喷雾两相湍流燃烧过程。通过耦合求解气液两相流模型方程,得到发动机燃烧流场。通过模拟Mg与水的反应,分析比较了一次和二次进水方案的不同流场特性。研究结果表明,二次进水方案更有利于火焰稳定和提高燃烧性能。     

阳极层推力器的研究现状与发展趋势

通过对阳极层推力器的工作原理、特点、羽流特性以及国内外阳极层推力器的研究现状与发展趋势的介绍和分析,指出了阳极层推力器是目前应用前景最好的电推进器之一,并且阳极层推力器正朝着更高功率和/或更高比冲的方向发展。随着空间技术的飞速发展,对高功率和/或高比冲的阳极层推力器的需求将越来越迫切,世界各国在这上面的投入也将越来越大。     

离子推力器羽流特性及其污染分析

介绍了与电推进系统有关的空间环境效应的形成原因及其对航天器性能、寿命等的影响。阐述了离子火箭发动机羽流内束离子、中性推进剂原子、交换电荷（CEX）离子和电子等主要成分与航天器相互作用的过程及机理。分析表明，离子推力器出口处的中性推进剂原子与高速束离子流碰撞后产生的CEX离子Xe^＋，以及带电离子轰击推力器组件特别是加速极所产生的金属CEX离子，是造成离子火箭发动机羽流污染的主要成分。在此基础上提出了若干防污染措施。     

电推进技术的研究应用现状及其发展趋势

简述了电推进的工作原理、基本分类以及各形式电推进(电热式、电磁式和静电式)的主要特点；重点论述了世界各国电推进技术的研制和应用现状，以及电推进技术的发展趋势和应用前景；最后简述了我国电推进技术的研究现状，并提出了加快我国电推进技术发展的建议。     

锂离子电池用正极材料LiNi_(1-x)Co_xO_2的研究

采用高温固相法分别在空气和氧气气氛下合成锂离子电池正极材料LiNi1-xCoxO2 (x =1 ,0 .8,0 .5,0 .2 ,0 ) ,用X射线衍射 (XRD)测定晶格结构和晶胞参数 ,并用CR2 0 2 5扣式电池及 1 8650型电池对材料充放电性能进行测试。试验结果表明 ,随着LiNi1-xCoxO2 中钴含量增加 ,晶胞参数a和c值依次减小 ,晶胞体积收缩。同时烧结气氛对材料结构和电化学性能影响极大 ,氧气气氛有助于LiNi1-xCoxO2 (x >0 )的生成     

The KACST muon detector and its application to cosmic-ray variations studies

A single channel cosmic ray muon detector was constructed and installed in Riyadh, central Saudi Arabia, for studying the variations in the cosmic ray (CR) muon flux. The detector has been in operation since July 2002. The recorded data correspond to muons that primarily have energies between 10 and 20 GeV. The detector will be used to continuously measure the intensity of the muon components of the cosmic rays, exploring its variations and possible correlations with environment parameters. The technical aspects of this detector will be presented. Some results obtained by the detector so far will be given. These include the modulation of the CR flux on different time scales (diurnal, 27-day, and long-term variations). Additionally, the effect of a severe dust storm on the muon count rate was investigated.     

Response of a pentagonal PZT element as a component of a 4π-real-time detector

The detector characteristics of a pentagonal element were studied by colliding it with hypervelocity micro-particles. A charge-sensitive amplifier was developed for the element of its capacitance ∼10 nF. The output amplitudes were expressed as a linear function of the momentum at collision. Empirical formulas obtained from on-ground experiments could be used for the calibration of the detector. The pentagonal element was potential to measure the momentum during collision from the output amplitude. A set of electrodes on the surface was used to confirm the measurement of the coordinates at collision. A possible application of this pentagonal element on a real-time dust detector was discussed.     

The Transition Between Fast and Slow Solar Wind from Composition Data

The transition between coronal hole associated fast solar wind and slow solar wind is studied using data from the high resolution mass spectrometer SWICS on ACE. We discuss the data in the framework of a recent theory about the global heliospheric magnetic field and conclude that the data are consistent with magnetic connections between field-lines in the fast and in the slow wind. This revised version was published online in June 2006 with corrections to the Cover Date.