如何从"无为"到"无不为"--老子"道"的伦理精神探微

《老子》书文约义丰,曲折难懂。其“无为无不为”更是只能心知其意。笔者试图对从“无为”到“无不为”中间的逻辑环节作一个解读——把二者连接起来的是其中存在着一种成长性希冀,在中国传统文化中则体现为一种务虚精神,并且深深地影响到了中国人对生命和人的认识。     

某发动机低频不稳定燃烧的消除

根据发动机热试车出现的低频不稳定燃烧现象,分析了产品的故障模式,建立了相关零组件模型。对相关零件进行了改进设计,消除了发动机低频不稳定燃烧现象。     

捷联惯导系统大方位失准角下的非线性对准

采用欧拉角描述平台坐标系与导航坐标系间的失准角,推导了适用于捷联惯导系统的非线性误差方程,证明了该方法仅适用于方位误差角为大角度,而水平误差角为小量的情况。数学仿真表明:在方位误差角为大角度情况下,采用所推导的误差方程和非线性滤波技术能获得更高的估计精度。     

翼型伞气动特性风洞试验研究

文章介绍了在8m×6m低速风洞中对某冲压式翼型伞进行的试验研究。文中给出了有关的技术方法,并对典型的试验结果进行了讨论。这一国内首创的风洞试验技术,可为翼型伞设计提供利用其他试验手段难以得到的翼伞操稳特性气动参数。     

GNSS Satellite Autonomous Integrity Monitoring (SAIM) using inter-satellite measurements

Integrity is the ability of Global Navigation Satellite Systems (GNSS) to detect faults in measurements and provide timely warnings to users and operators when the navigation system cannot meet the defined performance standards, which is of great importance for safety of life critical applications. Compared with both Receiver Autonomous Integrity Monitoring (RAIM) and ground based GNSS Integrity Channel (GIC) methods which are widely adopted nowadays, the Satellite Autonomous Integrity Monitoring (SAIM) method can be used to monitor orbit/ephemeris and clock errors, and has advantages in monitoring orbit and clock quality and providing instantaneous responses when faults happen.     

Drag force on solar sails due to absorption of solar radiation

We consider a special relativistic effect, known as the Poynting–Robertson effect, on various types of trajectories of solar sails. Since this effect occurs at order v^?/c, where v^? is the transversal speed relative to the sun, it can dominate over other special relativistic effects, which occur at order v²/c². While solar radiation can be used to propel the solar sail, the absorbed portion of it also gives rise to a drag force in the transversal direction. For escape trajectories, this diminishes the cruising velocity, which can have a cumulative effect on the heliocentric distance. For a solar sail directly facing the sun in a bound orbit, the Poynting–Robertson effect decreases its orbital speed, thereby causing it to slowly spiral towards the sun. We also consider this effect for non-Keplerian orbits in which the solar sail is tilted in the azimuthal direction. While in principle the drag force could be counter-balanced by an extremely small tilt of the solar sail in the polar direction, periodic adjustments are more feasible.     

数控蒙皮横拉机运动分析与仿真控制

进行了某数控蒙皮横拉机的机构分析,开发了机构运动反解软件.并在UG软件中进行了机构的运动建模与计算机仿真.运动反解与计算机仿真的相互验证,确定运动反解软件的准确性.实现了拉形过程有限元模拟与拉形机作动筒伸缩控制的结合,为该设备的精确控制及效能发挥提供了技术基础.      

聚酰亚胺/无机氧化物复合薄膜的制备与耐原子氧性能

分别以锆酸四丁酯、钛酸四丁酯和正硅酸乙酯为氧化物前驱体,利用溶胶凝胶法制备了一系列聚酰亚胺/无机氧化物复合薄膜,在原子氧地面模拟设备中进行了原子氧暴露实验,原子氧累计通量约为3.1×10²⁰ atom/cm².分别考察了无机氧化物种类和含量对复合薄膜力学性能和耐原子氧性能的影响.结果表明,无机氧化物在聚酰亚胺基体中的分散形态对其力学性能影响很大;原子氧暴露后,聚酰亚胺薄膜表面分别形成了富锆、富钛和富硅的保护层,质量损失率减小,耐原子氧性能明显提高.     

Thermal cyclotron radiation from a hot coronal loop with helical magnetic field

The spectral and polarization properties of thermal cyclotron radio emission from a hot coronal loop with a current along the axis are computed. The magnetic field is supposed to have a component along the loop axis as well as a poloidal part due to the current, both components being of comparable magnitude. In this specific configuration a helical magnetic field is present with a remarkable minimum of its absolute value along the loop axis and a maximum at its periphery. The presence of one or two maxima of magnetic field value along the line of sight results in increasing optical thickness of the gyroresonance layers at appropriate frequencies in the microwave band and, therefore, in enhanced radio emission at those harmonics which are optically thin (for example,s=4). These cannot be observed in models with the commonly employed magnetic field configuration (longitudinal along the loop axis).We show that the frequency spectrum of thermal cyclotron radiation from a hot coronal loop with a helical magnetic field differs from that of the standards-component source (with smooth frequency characteristics and polarization corresponding toe-mode) in that plenty of fine structures (line-like features and cut-offs) are present and theo-mode is prevalent in some frequency intervals. The enhanced radio emission at high harmonics and the complicated form of frequency spectrum in the model considered imply that some microwave sources, which are poorly explained in traditional models of solar active regions, may be associated with helical magnetic fields in hot coronal loops. Computations allow one to indicate spectral and polarizational peculiarities of local sources testifying to the presence of a helical magnetic field.     

2198和5A90铝锂合金脉冲阳极氧化膜制备及耐蚀性

在18%(质量分数,下同)H_2SO_4+5%C_2H_2O_4水溶液中,采用脉冲(PC)电流对2198和5A90两种铝锂合金进行阳极氧化处理。用扫描电子显微镜(SEM)观察铝锂合金阳极氧化膜表面和截面形貌;用能谱仪(EDS)对其成分进行面扫描和线扫描;用动电位极曲线检测氧化膜在3.5%NaCl水溶液中的耐蚀性。结果表明:2198和5A90铝锂合金阳极氧化膜主要由Al的氧化物组成;2198合金氧化膜表面存在细小颗粒,厚度约为150μm;5A90合金氧化膜表面存在微孔,为后续封孔处理提供结构条件,厚度约为180μm;用脉冲方法在两种铝锂合金表面生成的较厚阳极氧化膜具有较高的耐蚀性。