大多普勒容限巴克码脉压

 本文介绍用补偿式非相干型旁瓣抑制滤波器(SSF)实现13位巴克码脉冲压缩旁瓣抑制的理论计算及实验结果。补偿式非相干型SSF采用最小二乘近似逆滤波方法设计,若子脉冲宽度为0.7μs,峰值旁瓣电平不超过-30dB,这种SSF的多普勒容限能达到-40kHz～+40kHz。理论计算及实验结果都表明,所设计的补偿式非相干型SSF的多普勒容限比具有同样长度冲激响应序列的R-G-ISSF有显著改善。     

基于电子数据存储技术的微机化遥测处理系统

通过对某一高码速率光纤遥测系统中数据格式、码速率、数据容量、数据存储宽度、数据存储速率等特点的研究，提出了一种基于大容量电子数据存储器的微机化遥测处理系统，对存储的大容量数据阵列中的帧码识别、分路控制方法进行了讨论，并对受干扰数据处理时帧同步码检测的检测门限和同步对策参数进行了分析，最后给出了整个微机化的大容量遥测数据处理系统的软硬件设计方法，通过在６．５ＭｂｐｓＰＣＭ系统下的运行实验表明，整个方     

Rapid design and optimization of low-thrust rendezvous/interception trajectory for asteroid deflection missions

Asteroid deflection techniques are essential in order to protect the Earth from catastrophic impacts by hazardous asteroids. Rapid design and optimization of low-thrust rendezvous/interception trajectories is considered as one of the key technologies to successfully deflect potentially hazardous asteroids. In this paper, we address a general framework for the rapid design and optimization of low-thrust rendezvous/interception trajectories for future asteroid deflection missions. The design and optimization process includes three closely associated steps. Firstly, shape-based approaches and genetic algorithm (GA) are adopted to perform preliminary design, which provides a reasonable initial guess for subsequent accurate optimization. Secondly, Radau pseudospectral method is utilized to transcribe the low-thrust trajectory optimization problem into a discrete nonlinear programming (NLP) problem. Finally, sequential quadratic programming (SQP) is used to efficiently solve the nonlinear programming problem and obtain the optimal low-thrust rendezvous/interception trajectories. The rapid design and optimization algorithms developed in this paper are validated by three simulation cases with different performance indexes and boundary constraints.     

On the observability of Mars entry navigation using radiometric measurements

A thorough observability analysis of the Mars entry navigation using radiometric measurements from ground based beacons is performed. This analysis involves the evaluation of the Fisher information matrix which is derived from the maximum likelihood estimation. A series of navigation cases with multiple beacons are investigated, and both range and range-rate measurements are considered. The determinant of Fisher information matrix is used to quantify the observability of navigation system, while the trace of Fisher information matrix is used to determine the lower-bound of estimation errors. For one and two beacon cases, the navigation system is unobservable. However, the eigenvectors of Fisher information matrix give the observable and unobservable component. When three or more beacon measurements are employed, the states of entry vehicle become observable. Some valuable analytic conclusions on the relationship between the geometric configuration of beacons and observability are obtained consequently. Finally, simulation results from two navigation examples indicate that our effort is useful for understanding and assessing the observability of the Mars entry navigation using radiometric measurements.     

An innovative navigation scheme of powered descent phase for Mars pinpoint landing

Pinpoint landing (within 100 m from the target) is essential for future Mars exploration missions. This paper deals with one aspect of the pinpoint landing architecture—the navigation performance improvement during the powered descent phase, and proposes an innovative navigation scheme to obtain the vehicle complete and accurate states. On the basis of dead reckoning relying on the Inertial Measurement Unit, measurements of the Integrated Doppler Radar are adopted to correct the vehicle velocity and altitude. Distance between the vehicle and one Mars Orbiter as well as their line-of-sight relative velocity is measured by a radio sensor, and integrated in the filter to correct the vehicle horizontal position. The innovative navigation system is based on an Extend Kalman Filter. Two observation schemes are developed. One considers measurements of the Integrated Doppler Radar and radio range measurement. Another further considers radio velocity measurement. The performance of the innovative navigation scheme is greatly influenced by the position of the Mars Orbiter with respect to the target. Stochastic analyses are performed to obtain optimal locations of Mars Orbiter. Finally, the innovative navigation scheme performances are assessed through stochastic simulations. Its performance improvements are demonstrated by comparison with the Integrated Doppler Radar only navigation scheme.     

电缆网阻值测试仪的设计与实现

随着单片机技术的发展及其在测试领域的广泛应用,早期采用的人工作业对电缆网性能测定的方法已经不再适用。本文介绍了一种基于单片机技术的电缆网阻值测试仪。从电缆网阻值测试仪的功能与设计要求出发,阐述了总体设计方案,说明了该套设备的工作原理,描述了系统的硬件实施和软件设计,并对整套设备进行了实验验证。结果表明：设备满足了用户要求,提高了测试效率。     

改进跨音速位势方法的讨论

 简要地回顾并讨论了传统位势方法之不足。对改进传统位势方法的两种必要的修正(熵修正和涡修正)的量级在小扰动条件下作了分析和估值。结果表明涡修正是更高阶小量,因而作为第一步修正可采用非等熵位势流来近似。采用熵修正激波算子来计及非等熵的激波突跃条件,并考虑了由熵修正带来的尾迹条件的变化。算例表明非等熵位势方法能得到预期的改进位势方法的效果。     

宽温域连续润滑的Ni3 Al 基自润滑复合材料

报道了一种从室温到1 000℃能够连续润滑的Ni3Al基自润滑复合材料.该材料选用高温强度和抗氧化性优异的Ni3Al金属间化合物为基体材料,利用多种高、低温固体润滑剂的复合和协同效应实现了宽温域连续润滑.本文介绍了利用真空热压烧结方法制备该自润滑复合材料的简要过程,研究了材料的高温力学性能,并在球盘式高温摩擦试验机(HT-1000型)和销盘式高速摩擦试验机上分别测试了不同温度和转速下Ni3Al基自润滑复合材料的摩擦磨损性能.结果表明,材料在1 000℃时具有优异的力学性能(压缩强度40～45 MPa)和自润滑性能(摩擦因数0.28 ～0.25),在高载和高速条件下具有稳定的更低的摩擦因数.     

太阳同步轨道卫星光学特性

为了分析太阳同步轨道卫星的光学特性,对FY-1卫星的可见光和红外波段光学信号进行了仿真计算和模拟试验验证.通过对外部辐射及内部热源的分析,计算了卫星的温度场,采用随机起伏表面算法模拟表面覆盖材料外表面,通过阴影遮挡判断及双向反射分布函数(BRDF, Bi-directional Reflectance Distribution Function)模型计算卫星对外部辐射的反射特性,编程计算得到在可见光0.4~1.0μm和红外8~14 μm,14~16 μm波段下卫星的光学特性.结果表明红外辐射亮度与表面温度相关,8~14 μm最大约90 W/(m²·sr)、14~16 μm最大约20 W/(m²·sr).空间可见光辐射强度具有明显的镜面反射效应,卫星主体峰值2 200 W/sr.通过地面模拟测量空间目标的温度和红外辐射验证了温度及红外辐射仿真计算模型,可见光辐射强度仿真计算结果与地面模型卫星测量结果误差在20%以内.     

一体化智能电磁流量计的研制

介绍了一种集传感器,转换器,积算仪器于一体的就地显示式智能电磁流量计,其研制中采用先进的单片微机芯片,实现在线多种信号采集和数据处理,并采用软件容错技术,大大提高了仪表的可靠性和测量准确度。