一种飞机机轮轴承重负荷冲击试验机的设计

随着现代飞机性能要求的不断提高,对飞机机轮轴承提出了更高的要求,研制性能更佳的机轮轴承供机轮选用已是必然趋势,本文介绍了一种采用立式液压加载系统以及对滚式的被动驱动轴承外圈旋转方式的飞机机轮轴承重负荷冲击试验机,可模拟机轮轴承在机轮上承受的径向和轴向静载荷试验、动载荷谱滚转疲劳寿命试验、冲击载荷承载能力试验、刹车制动试验等受载工况试验。     

GH4169材料磨削后数控抛光表面完整性试验研究

针对航空发动机叶片材料GH4169高温合金,采用CBN砂轮磨削后进行羊毛毡轮数控抛光.首先,研究了抛光预压量对抛光轮寿命和工件表面粗糙度的影响,找到了抛光轮寿命的评价方法和优化的预压量;然后,研究了抛光深度对磨削后GH4169表面完整性的影响.结果表明:表面粗糙度Ra随抛光深度的增加先减小后稳定,表面显微硬度HV随抛光深度的增加呈显著下降趋势,进给方向表面残余正应力随深度增加先升高后下降,而垂直进给方向表面残余正应力先基本不变后下降.最终试验优选出了深度参数为2μm,预压量0.5～1.0mm.采用羊毛毡轮对GH4169磨削表面进行抛光,既能达到较小的表面粗糙度值(Ra=0.3μm),又可以有效维持CBN砂轮磨削形成的两个方向较大的表面残余应力.     

精确轨道航天器的姿态机动策略选择

航天器姿态控制一直是地面飞控的核心,尤其对于有精确轨道控制要求的航天器,姿态控制的策略选择直接关系任务成败。探月三期月地高速再入返回任务对再入角有着严格要求,为了实现返回器高精度再入,在系统介绍服务舱的姿态控制模式、控制方法和控制流程的基础上,提出了利用修改相平面参数和轮控调姿,以建立轨控姿态,从而减少姿控喷气,并提高轨控精度的方法。飞行结果表明,中途修正的控制精度从最初的分米量级提高至0.009m/s。高精度轨道控制使得提前32h再入角控制精度达到0.024°,较设计指标提高1个数量级。文中提及的轮控调姿方法可作为未来深空探测任务姿态控制的设计参考。     

Jitter reduction of a reaction wheel by management of angular momentum using magnetic torquers in nano- and micro-satellites

Nowadays, nano- and micro-satellites, which are smaller than conventional large satellites, provide access to space to many satellite developers, and they are attracting interest as an application of space development because development is possible over shorter time period at a lower cost. In most of these nano- and micro-satellite missions, the satellites generally must meet strict attitude requirements for obtaining scientific data under strict constraints of power consumption, space, and weight. In many satellite missions, the jitter of a reaction wheel degrades the performance of the mission detectors and attitude sensors; therefore, jitter should be controlled or isolated to reduce its effect on sensor devices. In conventional standard-sized satellites, tip-tilt mirrors (TTMs) and isolators are used for controlling or isolating the vibrations from reaction wheels; however, it is difficult to use these devices for nano- and micro-satellite missions under the strict power, space, and mass constraints. In this research, the jitter of reaction wheels is reduced by using accurate sensors, small reaction wheels, and slow rotation frequency reaction wheel instead of TTMs and isolators. The objective of a reaction wheel in many satellite missions is the management of the satellite’s angular momentum, which increases because of attitude disturbances. If the magnitude of the disturbance is reduced in orbit or on the ground, the magnitude of the angular momentum that the reaction wheels gain from attitude disturbances in orbit becomes smaller; therefore, satellites can stabilize their attitude using only smaller reaction wheels or slow rotation speed, which cause relatively smaller vibration. In nano- and micro-satellite missions, the dominant attitude disturbance is a magnetic torque, which can be cancelled by using magnetic actuators. With the magnetic compensation, the satellite reduces the angular momentum that the reaction wheels gain, and therefore, satellites do not require large reaction wheels and higher rotation speed, which cause jitter. As a result, the satellite can reduce the effect of jitter without using conventional isolators and TTMs. Hence, the satellites can achieve precise attitude control under low power, space, and mass constraints using this proposed method. Through the example of an astronomical observation mission using nano- and micro-satellites, it is demonstrated that the jitter reduction using small reaction wheels is feasible in nano- and micro-satellites.     

The statistical features of radio bursts with fine structure at 1.1–7.6 GHz

This work presents the spectral and temporal features of radio bursts with fine structures (FSs) at broad band from 1.1 to 7.6 GHz. Fifteen burst events are studied with high frequency and temporal cadence observation from the Solar Broadband Radio Spectrometer at three frequency bands. It is found that the amount and species of radio FS decrease with increasing frequency band; the pulsation, type III burst and continuum are most frequently recorded; almost in all the burst events, more radio FSs occur before the soft X-ray (SXR) maximum than after; at 1.1–2.06 GHz, all types of radio FSs have more before the SXR peak except fiber; at 2.6–3.8 GHz, pulsation, fiber and spike prefer to appear after the peak; the separation between neighboring emission lines of zebra pattern increases with increasing frequency and the magnetic field deduced from the whistler model is 29–86 G at 1.1–2.06 GHz and 89–268 G at 2.6–3.8 GHz.     

工程陶瓷磨削表面/亚表面损伤的产生及其控制

讨论了表面/亚表面裂纹和残余应力产生的原因及扩展机理,探讨了控制陶瓷磨削表面/亚表面损伤的途径,并指出了当前存在的问题及今后需要努力地方向.     

飞轮隔振平台组合系统的动力学建模

为分析隔振平台对星上飞轮扰动的衰减效果,研究了飞轮隔振平台组合系统的动力学建模问题.首先推导出含有静动不平衡量的飞轮加隔振平台组合系统的动力学模型.从模型中得出,飞轮和平台之间存在耦合;转子的静动不平衡会体现为飞轮的多项扰动力和扰动力矩.其次,对这些扰动项进行量级分析,并据此简化系统方程.最后利用数值仿真将简化模型与之前的完整模型作对比,验证了此简化模型的合理性;并通过初步的整星系统仿真,说明了隔振系统对航天器姿态稳定度的改善效果.     

几种新型去毛刺和光整加工设备

介绍第二届精密表面光整加工及去毛刺工艺技术国际学术会议论文交流中有关滚筒研磨技术和电解磁力研磨技术的新发展。     

航空发动机高压旋转涡轮盘腔流动与换热

在同模型实验参数范围内，且数值解和实验解基本吻合的前提下，对发动机原型参数进行数值模拟，求解了旋转系下流体流动与换热微分方程组，通过对气体域和固体域进行共扼计算，并将动量方程与能量方程福合求解。结果表明利用低参数下实验数据支持的数值计算程序对真实参数的模拟是合理的，对于复杂的非线性现象，数值外推法比传统实验外推更加准确。     

Spraying of Super Fine Powders With HVOF and Axial Plasma Thermal Spray Systems

The use of fine powders in thermal spray can lead to many advantages. These advantages include denser coatings, coatings with increased wear resistance, coatings with smoother surface finish, coatings that can be applied to internal surfaces, less expensive coatings. The use of fine powders also has an disadvantage that th ey can have poor flow characteristics. The paper will discuss a feeder that is able to feed fine powders to overcome this difficulty and the coating equipment, both axial plasma and HVOF systems, used to deposit these materials to produce smooth dense coatings.