含环向裂纹厚壁圆筒电磁止裂的应力场分析

以具有轴对称性质、端部带有半埋藏环形裂纹的厚壁圆筒为研究对象,通过对长厚壁圆筒内外环面均匀通入超强脉冲电流进行电磁热止裂。采用复变函数方法求解了脉冲放电瞬间裂纹尖端的温度场和热应力场。在一定的超强脉冲电流作用下,由于环形裂纹尖端的电流绕流热集中效应,裂尖温升超过了金属熔点,使裂尖处金属熔化在内部形成堆焊,钝化了裂尖,并且在裂纹前缘形成了热压应力,阻止了裂纹的扩展。在此基础上还讨论了在电载荷和机械载荷共同作用下裂纹前缘的应力场。     

双臂自由飞行空间机器人捕捉目标实验研究

本文主要介绍了在地面上模拟的空间微重力环境下双臂自由飞行空间机器人捕捉目标的实验。首先介绍了双臂自由飞行空间机器人地面实验平台，该实验平台由机器人模型、视觉系统、无线通讯系统、网络系统、操作台、运动规划系统、气浮系统七个子模块构成。其次简单介绍了双臂自由飞行空间机器人捕捉目标策略，最后介绍了基于该实验平台的几种实验。     

火箭电气系统电缆网热防护研究

简要介绍了箭上电气系统电缆网热防护技术应用现状，阐述了一体化热防护研究的必要性，提出了轻质电缆网的芯线、绝缘层、屏蔽层、插头和热防护层有效集成的总体方案。研制热防护材料，确定热防护层结构，试制一体化热防护电缆网，模拟热环境试验，研究表明：一体化热防护电缆网满足结构减重与轻柔、可靠性提高和总装周期缩短等总体指标要求。     

基于软件锁相环的电机速度控制系统

随着电力电子、微电子技术和控制技术的发展,一些场合对电机调速系统性能的要求越来越高,而锁相调速控制在稳速精度方面有其独特的优势。文章在改进的数字锁相环基础上,提出了软件锁相环电机速度控制系统,利用高性能微处理器实现了软件锁相环。     

Identification of high energy solar particle signals on the Mexico City neutron monitor database

We performed a search for ground level solar cosmic ray enhancements on the full five minute database of the Mexico City neutron monitor using wavelet filters and two different statistical tests. We present a detailed analysis of the time series of November 2, 1992, where we found a previously unreported increment matching the onset time of the impulsive phase of GLE 54, thus providing evidence of an effective detection of high energy solar cosmic rays.     

Prospects of using a permanent magnetic end effector to despin and detumble an uncooperative target

Space debris, such as defunct satellites and upper stages of rockets, becomes an uncooperative target after losing its attitude control and communication ability. In addition, tumbling motion can occur due to environmental perturbations and residual angular momentum prior to the object’s end-of-mission. To minimize the collision risk during docking and capturing of the tumbling target, a non-contact method based on the eddy current effect is put forward to transmit the control torque to the tumbling target. The main idea is to induce a controllable torque on the conducting surface of the tumbling target using a rotational magnetic field generated by a Halbach rotor. The radial and axial Halbach rotors are used to damp the spinning and nutation motions of the target, respectively. The normal and tangential force are evaluated concerning the relative pose between the chaser and the target. A simplified dynamic model of the nutation damping and despinning processes is developed and the influences of the asymmetrical principal moments of inertia and transverse angular velocity are discussed. The numerical simulation results show that the designed Halbach rotor stabilized the target attitude within an acceptable time. The electromagnetic nutation damping and despinning method provides new solutions for the development of on-orbit capture technology.     

Relationship of the diffuse aurora and SAR arc dynamics to substorms and storms

Investigation results of a diffuse aurora (DA) and stable auroral red (SAR) arc dynamics based on spectrophotometric observations at the Yakutsk meridian (199°E geomagnetic longitude) are presented. The relationship of an equatorward extension of DA in the 557.7 nm emission to a substorm growth phase during the magnetospheric convection intensification after the turn of IMF B_Z to the south is shown. The formation of SAR arc during the substorm expansion phase is investigated. The association of SAR arc dynamics with the development of asymmetric ring current (substorm injection) during the main phase of a storm is analyzed. It is shown how the pulsating precipitations of energetic ring current particles develop in the outer plasmasphere based on photometric observations.     

电源自动测试系统述评

综述了电源自动测试系统的测试原理、测试方法和测试依据，分析了电源自动测试系统的特点、现状和发展趋势。     

大功率LED混光照明恒流驱动电路的设计

在分析了大功率LED混光照明中LED光源特性的基础上,提出了三色LED恒流驱动电路的设计方案。驱动电路分别采用升压和降压拓扑结构,利用具有PWM实时调光功能的RT8452作为驱动控制芯片,通过改变外接PWM占空比即可调节LED亮度。实验证明,此驱动电路工作可靠,效率高,实现简单。     

A solar wind driven model of geosynchronous plasma moments

We describe a tabular specification model of the density and temperature of ions and electrons at geosynchronous orbit as a function of magnetic local time and solar wind parameters. This model can be used to provide boundary conditions for numerical ring current models. Unlike previous specification models of geosynchronous plasma moments, this model is parameterized by upstream solar wind conditions. We find that solar wind parameters are a better predictor of geosynchronous ion density than magnetospheric indices, and as upstream parameters they are often more appropriate as model inputs since they causally precede the model outputs. Of the upstream parameters that were tested, the best predictors of geosynchronous conditions were the solar wind flow pressure and the magnitude and Z-component of the interplanetary magnetic field.