电泳沉积-激光熔覆金属陶瓷复合涂层

提出以电泳沉积作为激光熔覆的粉末预置法,并与等离子喷涂等方法进行了比较,借鉴其他送粉技术许多新的工艺方法,对陶瓷涂层可能出现的裂纹、内应力等问题提出了增加金属粘结相,预热、缓冷等解决措施.     

SPACE CHEMISTRY RESEARCHES IN CHINA DURING 2000-2001

Over the past two years, significant progress in space chemistry has been made in China. The research fields include meteorites, pre-solar materials, science researches of the moon, effects of the space debris on space environment, and heterogeneity of the Earth. Chinese Lunar Exploration Project Some studies are also dedicated to one important space mission "Chinese Lunar Exploration Project". In this paper, the main achievements are outlined, and some concepts and hypotheses are briefly revised.     

神舟4号大气成分探测的新结果

神舟4号(SZ-4)大气成分探测器搭载在SZ-4留轨舱上于2002年12月30日发射入轨，在在轨运行的前3个多月中，正值地球南半球处于夏半球季节，并发生了多次中低强度的地磁扰动事件，SZ-4大气成分探测器测得了轨道舱运行高度上(330-362km附近)大气成分的响应变化和异常现象新结果．探测数据表明，中低强度的地磁扰动事件也能引起热层大气中主要成分O和N2的数密度值增高的响应变化．同样在进入地磁扰动峰期后较高纬度处出现了N2的异常增变和O的异常降变以及大气密度异常扰动的现象，但此期间所出现异常现象的地域与SZ-3和SZ-2大气成分探测器探测结果相反，它仅位于南半球较高纬度地区．     

Changes in the Structure of Comet Nuclei Due to Radioactive Heating

The initial structure of a comet nucleus is most probably a homogeneous, porous, fine-grained mixture of dust and ices, predominantly water. The water ice is presumably amorphous and includes considerable fractions of occluded gases. This structure undergoes significant changes during the early evolution of the nucleus at large heliocentric distances, due to internal radiogenic heating. Structural changes occur mainly as a result of gas flow through the porous medium: the gas pressure that builds up in the interior is capable of breaking the fragile structure and altering the pore sizes and porosity. These effects are modeled and followed numerically, testing a large number of parameters. This revised version was published online in June 2006 with corrections to the Cover Date.     

烟火药水下燃烧的声辐射机理与实验研究

烟火药水下燃烧能够形成低频的水下声.法国烟火集团拉克鲁瓦防御公司研制出了一种"烟火--声电"声诱饵(1995),但是至今还没有进行深入的研究与报道.本文就烟火药水下燃烧的声辐射机理进行了探讨.结果显示,其所辐射的噪声主要包括喷注噪声和气泡噪声,进一步的分析发现主要以气泡噪声为主,喷注湍流噪声为辅.为了证明此观点,实验研究了具有脉动燃烧效应的烟火药水下燃烧时的声辐射特性.     

直流电弧喷射等离子体炬阳极喷嘴积碳现象的研究

采用高功率直流电弧等离子体喷射化学气相沉积工艺,制备了不同厚度的自支称金刚石厚膜.实验发现,等离子体炬阳极喷嘴积碳是沉积过程中最突出的问题之一.从理论和实验两个方面研究了阳极积碳产生的原因,并通过激光拉曼光谱分析了碳球的结构和成分.结果表明,碳球由金刚石层、混合层和最外面的石墨层构成.详细分析了甲烷浓度、冷却水温度、放电电弧的局部高温、阳极喷嘴的表面质量对积碳形成的影响,并提出了改进措施.     

功能分析与失效物理结合的可靠性预计方法

 可靠性预计是产品设计、研发过程中的重要工作,全面准确的可靠性预计可以评价产品的可靠性水平,也可以为设计提供信息,指导设计。全面分析总结当前电子设备可靠性预计相关技术方法,以当前基于失效物理(POF)技术的系统可靠性预计方法中,并未考虑产品功能组成关系的缺陷为突破点,建立了一种以失效物理分析为基础,综合考虑电路功能组成关系的电子设备可靠性预计方法。该方法从电路功能出发,通过灵敏度仿真和主成分分析两种方法,确定对电路性能起主要影响的关键单元,再通过失效物理分析或统计规律明确单元的失效概率分布,通过混合分布获得系统的分布,得到系统可靠性指标。最后以某航空机电产品的电源电路为案例,对本预计方法进行验证。     

Nickel Isotopic Composition and Nickel/Iron Ratio in the Solar Wind: Results from SOHO/CELIAS/MTOF

Using the Mass Time-of-Flight Spectrometer (MTOF)—part of the Charge, Elements, Isotope Analysis System (CELIAS)—onboard the Solar Heliospheric Observatory (SOHO) spacecraft, we derive the nickel isotopic composition for the isotopes with mass 58, 60 and 62 in the solar wind. In addition we measure the elemental abundance ratio of nickel to iron. We use data accumulated during ten years of SOHO operation to get sufficiently high counting statistics and compare periods of different solar wind velocities. We compare our values with the meteoritic ratios, which are believed to be a reliable reference for the solar system and also for the solar outer convective zone, since neither element is volatile and no isotopic fractionation is expected in meteorites. Meteoritic isotopic abundances agree with the terrestrial values and can thus be considered to be a reliable reference for the solar isotopic composition. The measurements show that the solar wind elemental Ni/Fe-ratio and the isotopic composition of solar wind nickel are consistent with the meteoritic values. This supports the concept that low-FIP elements are fed without relative fractionation into the solar wind. Our result also confirms the absence of substantial isotopic fractionation processes for medium and heavy ions acting in the solar wind.     

Isotopic Composition of the Solar Wind Inferred from In-Situ Spacecraft Measurements

The Sun is the largest reservoir of matter in the solar system, which formed 4.6 Gyr ago from the protosolar nebula. Data from space missions and theoretical models indicate that the solar wind carries a nearly unfractionated sample of heavy isotopes at energies of about 1 keV/amu from the Sun into interplanetary space. In anticipation of results from the Genesis mission’s solar-wind implanted samples, we revisit solar wind isotopic abundance data from the high-resolution CELIAS/MTOF spectrometer on board SOHO. In particular, we evaluate the isotopic abundance ratios ¹⁵N/¹⁴N, ¹⁷O/¹⁶O, and ¹⁸O/¹⁶O in the solar wind, which are reference values for isotopic fractionation processes during the formation of terrestrial planets as well as for the Galactic chemical evolution. We also give isotopic abundance ratios for He, Ne, Ar, Mg, Si, Ca, and Fe measured in situ in the solar wind.     

镁合金微弧氧化膜的相结构研究

针对镁合金微弧氧化膜层,对其相组成和品粒尺寸随工艺参数的变化规律进行了定件和定量分析,并考察了相组成对膜层耐蚀性能的影响.结果表明:不同工艺参数条件下制备的微弧氧化膜层均由镁铝尖晶石和方镁石两相组成,但两相的含量差别很大.当这两相含量的比值在0.6～1.0范围内时,膜层的耐蚀性明显提高.不同时间内制备的膜层中MgAl2O3晶粒尺寸都在40～50nm的范围内,随着氧化时间的增加,晶粒尺寸呈现先减小后增大的趋势.