氯离子和温度对铝合金在冷却液中腐蚀的影响

分别采用了动电位极化法、电化学阻抗法研究了不同温度下、不同氯离子浓度下防锈铝在模拟冷却液中的腐蚀行为,采用金相显微镜和扫描电镜对极化后防锈铝的表面特征进行了观察和记录。结果表明,氯离子吸附在防锈铝氧化膜表面,对氧化膜表面造成破坏。在一定温度下（30℃）,当氯离子浓度超过0.01mol/L时,中间产物吸附作用就会增强,阻抗谱中低频区出现感抗弧,点蚀萌生。随着氯离子浓度增高（超过0.01mol/L）,防锈铝的腐蚀加剧,耐腐蚀性能下降。随着温度的升高,阴极和阳极反应阻力变小,阳极金属铝的溶解和阴极氧还原速度增大,腐蚀速度增大。温度升高的同时,溶解氧含量下降,阴极反应受到抑制。与此同时扩散过程在整个腐蚀反应过程中的支配性降低,中间产物在氧化膜表面的吸附作用增强,从而导致低频容抗弧的出现。温度对点蚀形貌的影响主要体现在影响单个点蚀坑的几何大小,促进点蚀坑的生长。      

一种金属结构裂纹监测的薄膜传感器设计

针对金属结构服役过程中裂纹实时监测的需求,设计了一种基于电位法原理的裂纹监测薄膜传感器。首先,建立了该薄膜传感器的有限元模型并对传感器输出特性进行了仿真分析。仿真结果表明:通过分析各监测点之间的电位差变化可以判断裂纹扩展方向和长度。其次,应用离子镀技术在铝合金中心孔试件表面制备了薄膜传感器,薄膜传感器与基体表面结合良好。最后,进行了基于薄膜传感器的裂纹监测试验。实验结果表明:通过分析相邻两次监测数据的变化程度可以判断裂纹所处的扩展阶段。     

离子辅助沉积Al膜层增强Ti811钛合金高温微动疲劳抗力

为提高Ti811钛合金高温微动疲劳抗力,利用离子辅助沉积技术在Ti811钛合金表面制备Al膜层。对比研究多弧离子镀(MIP)和离子辅助多弧沉积(IAD)Al膜层的膜基界面成分分布、膜基结合强度、显微硬度、摩擦学性能。探讨IAD铝膜层对Ti811合金微动疲劳抗力的影响。结果表明,利用离子辅助多弧沉积技术可以获得膜基结合强度高、硬度低、减摩润滑性能好的Al膜层,该膜层能够显著提高Ti811钛合金350℃时的微动疲劳抗力。     

用~（11）B（p，α_0）~8Be核反应分析B~＋离子注入铜合金中的浓度分布

采用１１Ｂ（ｐ，α０）８Ｂｅ核反应分析了Ｂ＋注入锡青铜样品中的纵向浓度分布．该分布具有较宽的高浓度峰，表明样品表面可形成优良的改性层．讨论了提高核反应分析法深度分辨率的主要因素，指出减小入射质子束的能量分散度、提高探测系统的能量分辨率及增大Ｂ＋的能损因子，是提高深度分辨率的主要途径．     

Fabrication of Diamond-like Carbon Films by Ion Assisted Middle Frequency Unbalanced Magnetron Sputtering

Diamond-like carbon (DLC) films are deposited by the Hall ion source assisted by the mid-frequency unbalanced magnetron sput-tering technique. The effects of the substrate voltage bias, the substrate temperature, the Hall discharging current and the argon/nitrogen ratio on the DLC film’s performance were studied. The experimental results show that the film’s surface roughness, the hardness and the Young’s modulus increase firstly and then decrease with the bias voltage incrementally increases. Also when the substrate temperature rises, the surface roughness of the film varies slightly, but its hardness and Young’s modulus firstly increase followed by a sharp decrease when the temperature surpassing 120 ℃. With the Hall discharging current incrementally rising, the hardness and Young’s modulus of the film decrease and the surface roughness of the film on 316L stainless steel firstly decreased and then remains constant.     

The Mercury Atmospheric and Surface Composition Spectrometer for the MESSENGER Mission

The Mercury Atmospheric and Surface Composition Spectrometer (MASCS) is one of seven science instruments onboard the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft en route to the planet Mercury. MASCS consists of a small Cassegrain telescope with 257-mm effective focal length and a 50-mm aperture that simultaneously feeds an UltraViolet and Visible Spectrometer (UVVS) and a Visible and InfraRed Spectrograph (VIRS). UVVS is a 125-mm focal length, scanning grating, Ebert-Fastie monochromator equipped with three photomultiplier tube detectors that cover far ultraviolet (115–180 nm), middle ultraviolet (160–320 nm), and visible (250–600 nm) wavelengths with an average 0.6-nm spectral resolution. It will measure altitude profiles of known species in order to determine the composition and structure of Mercury’s exosphere and its variability and will search for previously undetected exospheric species. VIRS is a 210-mm focal length, fixed concave grating spectrograph equipped with a beam splitter that simultaneously disperses the spectrum onto a 512-element silicon visible photodiode array (300–1050 nm) and a 256-element indium-gallium-arsenide infrared photodiode array 850–1,450 nm. It will obtain maps of surface reflectance spectra with a 5-nm resolution in the 300–1,450 nm wavelength range that will be used to investigate mineralogical composition on spatial scales of 5 km. UVVS will also observe the surface in the far and middle ultraviolet at a 10-km or smaller spatial scale. This paper summarizes the science rationale and measurement objectives for MASCS, discusses its detailed design and its calibration requirements, and briefly outlines observation strategies for its use during MESSENGER orbital operations around Mercury.     

Launch and Early Operation of the MESSENGER Mission

On August 3, 2004, at 2:15 a.m. EST, the MESSENGER mission to Mercury began with liftoff of the Delta II 7925H launch vehicle and 1,107-kg spacecraft including seven instruments. MESSENGER is the seventh in the series of NASA Discovery missions, the third to be built and operated by The Johns Hopkins University Applied Physics Laboratory (JHU/APL) following the Near Earth Asteroid Rendezvous (NEAR) Shoemaker and Comet Nucleus Tour (CONTOUR) missions. The MESSENGER team at JHU/APL is using efficient operations approaches developed in support of the low-cost NEAR and CONTOUR operations while incorporating improved approaches for reducing total mission risk. This paper provides an overview of the designs and operational practices implemented to conduct the MESSENGER mission safely and effectively. These practices include proven approaches used on past JHU/APL operations and new improvements implemented to reduce risk, including adherence to time-proven standards of conduct in the planning and implementation of the mission. This paper also discusses the unique challenges of operating in orbit around Mercury, the closest planet to the Sun, and what specific measures are being taken to address those challenges.     

空间轨道单粒子翻转率预估方法研究

系统分析了国外单粒子翻转率预估方法，提出了一种适合国内现状的单粒子翻转率预估方法，计算了五个典型轨道上的单粒子翻转率和轨道翻转系数，为评价半导体器件抗单粒子效应的能力提供了依据。     

考夫曼离子推力器放电室数值模拟研究综述及展望

首先分析了影响考夫曼离子推力器放电性能的关键因素,然后按照仿真模型的维度对考夫曼离子推力器放电室数值模拟方法进行了分类综述和优缺点分析,并针对以流体方法为基础的各向异性界面问题进行了分析。在此基础上,概述了零维模型、二维模型和三维模型下针对放电室所取得的数值模拟研究结果。最后对考夫曼离子推力器放电室数值模拟研究进行了总结及展望。