便携式多功能校准仪在专用测试设备现场校准中的应用

航天工程专用测试设备具有系统复杂、参数多、不易移动的特点,常用校准方法复杂度高、效率低、成本高。为保证航天工程科研生产的顺利进行,专用测试设备的准确可靠及可溯源性越来越受到研制、生产和使用方的重视,并介绍了五种常用的专用测试设备校准方法。并针对目前常用校准方法的不足,提出将便携式多功能校准仪应用在专用测试设备现场校准的新方法,给出了不确定度分析。     

提高静压气浮陀螺加表K0、K1项精度的工艺研究

本文通过对影响静压气浮陀螺加表K0、K1项精度的因素分析,从加表及其重要组件的工作原理、结构特点、工艺过程等方面展开研究,总结出经过工艺试验及生产过程验证提高加表K0、K1项精度的关键技术,提高了加表验收合格率。     

用CST软件仿真替代部分卫星RM测试的可行性研究

环境减灾-1A、1B卫星采用CST-MWS软件完成了RM星仿真分析,快、好、省地完成了天线分系统设计验证任务。文章通过某卫星全向天线CST-MWS软件分析结果与RM测试结果的比较,表明软件分析结果的准确性满足RM验证的要求,验证了环境减灾-1A、1B卫星RM星仿真结果的正确性。进而也论证了软件仿真替代部分RM测试的可行性。     

天问一号着陆器大底分离安全性分析与验证

针对天问一号着陆器大底分离过程,建立大底分离动力学模型并分析分离安全性,基于分析结果设计了大底分离策略.利用大底分离动力学模型和近距离扰动气动模型,分析了分离过程的相对速度和姿态运动规律,根据大底与着陆器的正分离要求确定了大底分离的最小弹射速度.考虑到着陆器姿态运动影响分离安全性,对着陆器施加角速度阻尼控制并限制了最短...     

旋翼干扰下的直升机尾桨气动噪声计算研究

针对旋翼干扰下的直升机尾桨气动噪声计算问题,将CFD方法与Farassat 1A(F1A)公式相结合,提出了一种适用于旋翼干扰下的尾桨气动噪声数值计算方法。首先,应用所提出的方法进行了噪声的算例验证,并与参考文献结果进行了对比;然后,着重针对悬停和前飞状态旋翼干扰下的尾桨噪声及气动特性进行了计算分析,并与孤立尾桨状态进行了对比。计算分析结果表明:悬停状态下,旋翼干扰下的尾桨气动噪声水平显著大于孤立尾桨;而在前飞状态,由于旋翼尾迹对尾桨桨盘平面产生更强的气动干扰,这一现象会更加明显;同时,在旋翼干扰作用下,尾桨噪声的主传播方向也会发生明显变化。     

基于改进半阈值算法的电容层析成像滑油监测方法研究

针对航空滑油检测过程中电容层析成像（Electrical Capacitance Tomography,ECT）存在的病态性和欠定性问题,将稀疏正则化中基于L1/2正则化的半阈值迭代算法应用到ECT图像重建,加入L2范数的惩罚项,构造新的泛函模型,并在迭代过程中设计一种新的约束项以优化解向量。仿真实验采用Comsol5.3搭建系统模型,Matlab2014a处理采集数据。实验结果表明,与Landweber迭代算法相比,改进算法成像误差降低37.33%,相关系数提升33.67%;与半阈值迭代算法相比,改进算法成像误差和相关系数分别降低12.31%和提升11.86%,图像误差降低至0.24、相关系数提升至0.92,且成像时间依然保持在0.06s。实际滑油监测的实验系统采用现场可编程门阵列（Field Programmable Gate Array,FPGA）直接数字频率生成模块生成数字量的正弦激励信号,通过D/A转化为正负交流信号对测量电极进行激励。实验结果表明,基于ECT系统的改进半阈值迭代算法可以满足航空发动机滑油监测的实时性和准确性的要求。     

Scheme design of the CHANG’E-5T1 extended mission

Flight schemes for the CHANG’E-5T1 extended mission are investigated in this paper. In the flight scheme and trajectory design, the remaining propellant of the CHANG’E-5T1 mission is utilized. The CHANG’E-5T1 mission is firstly introduced with feasible flight goals derived based on the terminal trajectory and satellite status. The flight schemes are designed to include a lunar return and the libration points in the Sun-Earth/Moon and Earth-Moon systems, with an emphasis on the Earth-Moon triangle libration point thus far unexplored. Secondly, three schemes are proposed for the CHANG’E-5T1 extended mission with different flight goals. The direct libration point orbit transfer and injection method is adopted to solve the issue in the transfer trajectory design. Furthermore, an innovative concept is proposed to transfer from the Earth-Moon collinear libration point to the triangle point using the Sun-Earth/Moon libration point. Finally, the merits and drawbacks of the three schemes are discussed in terms of flight time, control energy and frequency, flight distance, and goal value. As a result, the scheme including a lunar return and the Earth-Moon L2 libration point is selected for the CHANG’E-5T1 extended mission. A flight to the Earth-Moon libration point is achieved, replicating the achievement of the ARTEMIS mission.     

会议筹备的0-1整数规划

在举行大型会议时,组委会需对宾馆预定、会议室安排,客车租用这三方面问题做出合理的安排,既要满足与会代表的要求,又要使租用会议室及租车费用尽可能少。针对此问题,建立了多目标规划模型,利用分层序列法,把目标按其重要性的序列:宾馆预定,会议室安排,客车租用依次求解,在前一目标最优解集内求下一个目标最优解,并利用LINGO软件求解。     

Assessment of the consequences of the Fengyun-1C breakup in low Earth orbit

On 11 January 2007, the People’s Republic of China conducted a successful anti-satellite test against one of their defunct polar-orbiting weather satellites. The target satellite, called Fengyun-1C, had a mass of 880 kg and was orbiting at an altitude of about 863 km when the collision occurred. Struck by a direct-ascent interceptor at a speed of 9.36 km/s, the satellite disintegrated, spreading the cataloged fragments between 200 and 4000 km, with the highest concentration near the breakup height. By the end of April 2008, 2377 pieces of debris, including the original payload remnant, had officially been cataloged by the US Space Surveillance Network. Of these, nearly 1% had reentered the Earth’s atmosphere. This deliberate act is the largest debris-generating event on record, and its consequences will adversely affect circumterrestrial space for many years.     

An inversion approach for lunar regolith layer thickness using optical albedo data and microwave emission simulation

An approach to inversion of the lunar regolith layer thickness by using multi-channel brightness temperature observation in passive microwave remote sensing is developed. To first make simulation of brightness temperature from the lunar layered media, the lunar regolith layer thickness (d) is proposed being constructed by available lunar DEM (digital elevation mapping) and on site measurements. The physical temperature distribution (T) over the lunar surface is also empirically assumed as a monotonic function of the latitude. Optical albedo of the lunar nearside from the telescopic observation is employed to construct the spatial distribution of the FeO+TiO₂ content (S) in the lunar regolith layer. A statistic relationship between the DEM and S of the lunar nearside is further extended to construction of S of the lunar farside. Thus, the dielectric permittivity (ε) of global lunar regolith layer can then be determined. Based on all these conditions (d,T,ε), brightness temperature of the lunar regolith layer in passive microwave remote sensing, which is planned for China's Chang-E lunar project, is numerically simulated by a parallel layering model using the strong fluctuation theory of random media.Then, taking these simulations with random noise as observations, an inversion method of the lunar regolith layer thickness is developed by using three- or two-channels brightness temperatures. When the S is low, and the four channels brightness temperatures in China's Chang-E project are well distinguishable, the regolith layer thickness and physical temperature of the underlying lunar rock media can be inverted by the three-channels approach. When the S becomes high that the brightness temperature at high frequency channels such as 19.35, 37 GHz are saturated, the regolith layer thickness is alternatively inverted only by the two-channels approach.Numerical simulation and inversion approach in this paper make an evaluation of the performance for lunar passive microwave remote sensing, and for future data calibration and validation.