表面活性剂对Ni-Co-PTFE复合电镀的影响

研究了表面活性剂对Ni-Co-PTFE复合电镀的影响情况，发现表面活性剂种类及其用量对该复合镀层中PTFE含量及镀层摩擦性能有显著的影响，其中以非离子表面活性剂与全氟阳离子表面活性剂组成的复合活性剂效果最好，其最佳用量为1g/L，获得的复合镀层微观表面结构致密，微粒分布均匀，摩擦系数最小，显微硬度HV0.1最大。     

Spacecraft optimal rendezvous controller design using simulated annealing

A new global approach for rendezvous Linear Quadratic controller design is presented in this paper. Instead of solving the algebraic Riccati equation, a continuous simulated annealing (SA) algorithm is used to design rendezvous LQ controller. Optimization of one automatic rendezvous controller with 18 design parameters is illustrated. The results show that the SA algorithm can locate the global solution effectively and robust, besides a great number of global solutions have been obtained by the SA. The SA has demonstrated better performance than other optimization algorithms such as floating-coded Genetic Algorithm, Simplex method and Powell algorithm.     

三角翼低速动态大攻角气动特性试验研究

对后掠角分别为X=60°、70°和80°尖前缘平板三角翼模型和一个前缘后掠角为（76° 40°）的双三角翼模型在低速风洞中作大攻角俯仰摩波运动，振幅am=30°、60°和90°，缩减频率K=0.01～0.12，基于根弦长雷诺数Re=2.76×10^5～8.23×10^5。进行了六分量动态气动载荷测量，动态流动显示和70°三角翼上翼面非定常压力测量，并分别与对应的静态试验结果比较。分析了运动参数包括缩减频率、振幅和Re数、后掠角对气流动态迟滞特性的影响。     

硅基内衬喷管扩张段烧蚀和温度场的耦合计算方法

本文叙述固体火箭喷管扩张段硅基内衬烧蚀和温度场的耦合计算方法.烧蚀采用非定常的液体层烧蚀模型;温度场计算采用圆柱坐标系下的一维径向瞬态导热模型,考虑材料在高温下形成的炭化层和热解层,而由烧蚀产生的边界移动问题用坐标变换的方法处理.利用烧蚀和导热计算方程组中二者的结合部,通过充分耦合,获得了更准确的预示计算结果.     

基于传递函数方法的局部覆盖环状CLD圆柱壳动力学分析

 采用传递函数方法对局部覆盖环状约束层阻尼（CLD）圆柱壳进行了动力学分析。基于Donnell薄壳简化，由Hamilton原理导出了局部覆盖CLD圆柱壳的运动方程和边界条件，通过Laplace变换并引入状态向量后，建立了系统的状态空间方程，利用传递函数方法求解方程得到了系统的固有频率、〖JP2〗损耗因子和频响曲线。算例分析结果验证了该方法的有效性和精确性，且更适于处理黏弹性材料具有频变特性的问题。讨论了CLD覆盖率和黏弹层厚度对系统固有频率和损耗因子的影响，为局部覆盖CLD圆柱壳的优化设计奠定了基础。     

受均匀内压作用的偏置孔边径向裂纹的应力强度因子的一种求解方法

本文利用一种新的混合法——光弹性实验与权函数解法相结合求解了孔壁受均匀内压作用偏置圆孔边径向裂纹的应力强度因子,该方法具有简单、经济、精度高等优点,对分析复杂应力场中圆孔边穿透裂纹问题,该方法同样适用,且优点更为突出.     

风洞中复杂流场三维速度LDV测量

本文将一台TSI 9100-7型两分量激光测速仪改进为可测三个速度分量的LDV系统,并用于测量风洞中椭球体模型、双三角翼模型大迎角下的复杂流场三维速度分量。流场横截面内的速度矢量分布与相同实验条件下的流态显示结果相符合,并对涡流场加以分析。     

MESSENGER: Exploring Mercury’s Magnetosphere

The MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) mission to Mercury offers our first opportunity to explore this planet’s miniature magnetosphere since the brief flybys of Mariner 10. Mercury’s magnetosphere is unique in many respects. The magnetosphere of Mercury is among the smallest in the solar system; its magnetic field typically stands off the solar wind only ∼1000 to 2000 km above the surface. For this reason there are no closed drift paths for energetic particles and, hence, no radiation belts. Magnetic reconnection at the dayside magnetopause may erode the subsolar magnetosphere, allowing solar wind ions to impact directly the regolith. Inductive currents in Mercury’s interior may act to modify the solar wind interaction by resisting changes due to solar wind pressure variations. Indeed, observations of these induction effects may be an important source of information on the state of Mercury’s interior. In addition, Mercury’s magnetosphere is the only one with its defining magnetic flux tubes rooted beneath the solid surface as opposed to an atmosphere with a conductive ionospheric layer. This lack of an ionosphere is probably the underlying reason for the brevity of the very intense, but short-lived, ∼1–2 min, substorm-like energetic particle events observed by Mariner 10 during its first traversal of Mercury’s magnetic tail. Because of Mercury’s proximity to the sun, 0.3–0.5 AU, this magnetosphere experiences the most extreme driving forces in the solar system. All of these factors are expected to produce complicated interactions involving the exchange and recycling of neutrals and ions among the solar wind, magnetosphere, and regolith. The electrodynamics of Mercury’s magnetosphere are expected to be equally complex, with strong forcing by the solar wind, magnetic reconnection, and pick-up of planetary ions all playing roles in the generation of field-aligned electric currents. However, these field-aligned currents do not close in an ionosphere, but in some other manner. In addition to the insights into magnetospheric physics offered by study of the solar wind–Mercury system, quantitative specification of the “external” magnetic field generated by magnetospheric currents is necessary for accurate determination of the strength and multi-polar decomposition of Mercury’s intrinsic magnetic field. MESSENGER’s highly capable instrumentation and broad orbital coverage will greatly advance our understanding of both the origin of Mercury’s magnetic field and the acceleration of charged particles in small magnetospheres. In this article, we review what is known about Mercury’s magnetosphere and describe the MESSENGER science team’s strategy for obtaining answers to the outstanding science questions surrounding the interaction of the solar wind with Mercury and its small, but dynamic, magnetosphere.     

窗函数递推T矩阵法

 引入数字信号处理中的窗函数, 应用于加法定理中, 解决了在入射波为TE 波时, 用递推T 矩阵法计算电大尺寸物体或多个散射体散射场时, 精度不高的问题。另外本文从积分方程出发, 推导出了总体T 矩阵的另一种表示形式, 最后给出的算例证明了引入窗函数的有效性和总体T 矩阵表达式的正确性。     

环氧／聚氨酯涂料的研究

采用环氧树脂来固化聚氨酯涂料，可使涂层具有良好的刚性和耐蚀性，本文研究了涂料各组分对于涂料涂层性能的影响，拟定了最佳配方工艺，并对其机理进行了阐述。