惯性敏感器与星敏感器之间在轨自主标定比较研究

惯性敏感器与星敏感器组合定姿是航天器高精度姿态确定的常用手段。通常将惯性敏感器的常值漂移作为扩展状态进行标定,而将星敏感器的常值偏差作为扩展状态进行估计也是可能的。本文对这两种方法的定姿精度进行了分析比较,给出了选用的准则。     

A robust star identification algorithm with star shortlisting

A star tracker provides the most accurate attitude solution in terms of arc seconds compared to the other existing attitude sensors. When no prior attitude information is available, it operates in “Lost-In-Space (LIS)” mode. Star pattern recognition, also known as star identification algorithm, forms the most crucial part of a star tracker in the LIS mode. Recognition reliability and speed are the two most important parameters of a star pattern recognition technique. In this paper, a novel star identification algorithm with star ID shortlisting is proposed. Firstly, the star IDs are shortlisted based on worst-case patch mismatch, and later stars are identified in the image by an initial match confirmed with a running sequential angular match technique. The proposed idea is tested on 16,200 simulated star images having magnitude uncertainty, noise stars, positional deviation, and varying size of the field of view. The proposed idea is also benchmarked with the state-of-the-art star pattern recognition techniques. Finally, the real-time performance of the proposed technique is tested on the 3104 real star images captured by a star tracker SST-20S currently mounted on a satellite. The proposed technique can achieve an identification accuracy of 98% and takes only 8.2?ms for identification on real images. Simulation and real-time results depict that the proposed technique is highly robust and achieves a high speed of identification suitable for actual space applications.     

热输入对AZ31镁合金FSP试样力学性能的影响

分别利用普通钢制垫板和自制的带有冷水通道的铜制垫板,对AZ31镁合金进行了搅拌摩擦加工。利用光学显微镜(OM)、SEM、显微硬度仪和拉伸设备,研究了被加工件厚度、搅拌头焊接速率和冷却条件对试样搅拌区力学性能的影响。研究表明:试样搅拌区从上层至中层和底层,再结晶晶粒尺寸依次减小。通过减小被加工件厚度、增大搅拌头焊接速率和加快冷却速率等方法,抑制了试样搅拌区晶粒长大。在搅拌头转速和焊接速率分别为800r/min和90mm/min的条件下,得到的搅拌区底部平均晶粒尺寸约为450nm,该区域显微硬度为96HV,与普通钢制垫板制备的试样相比,硬度提高了24HV,其屈服强度、抗拉强度和伸长率分别提高为原材料的1.27倍、1.6倍和2.2倍。     

考虑卫星轨道运动和像移影响的星敏感器星图模拟方法

星图模拟技术是星图识别算法和星敏感器性能测试的基础.提出一种新的高精度星图模拟方法.该方法分为三个步骤:首先,利用两行轨道数据(TLE,Two-Line Orbital Element)与简化常规/深空扰动的近似解模型(SGP4/SDP4)计算出卫星在轨运行参数,进而获得卫星姿态矩阵;然后,根据星敏感器的方位和俯仰角度,确定星敏感器视场中的导航星及星敏感器安装矩阵,利用小孔成像模型,获得导航星在星敏感器成像面的投影位置;最后,为更准确模拟实际星像点的灰度扩散,在考虑卫星运动引起的恒星像移的基础上,按照二维高斯分布规律置灰度值来模拟星像点像素.在此基础上,还详细分析了不同曝光时间下,恒星像移对恒星位置测量的影响.     

等通道转角挤压工艺制备超细化合金的研究与进展

等通道转角挤压技术（简称ECAP）是制备超细晶粒金属块材的最新研究领域之一。本文阐述了ECAP的研究目的与意义。说明了ECAP的原理，探讨了ECAP的国内外研究现状及进展，指出了ECAP急待解决的五大问题，具有较好的实用价值。     

Characteristics and accuracies of the GRACE inter-satellite pointing

For almost 10 years, the Gravity Recovery and Climate Experiment (GRACE) has provided information about the Earth gravity field with unprecedented accuracy. Efforts are ongoing to approach the GRACE baseline accuracy as there still remains an order of magnitude between the present error level of the gravity field solutions and the GRACE baseline. At the current level of accuracy, thorough investigation of sensor related effects is necessary as they are one of the potential contributors to the error budget. In the science mode operations, the twin satellites are kept precisely pointed with their KBR antennas towards each other. It is the task of the onboard attitude and orbit control system (AOCS) to keep the satellites in the required formation. We analyzed long time series of the inter-satellite pointing variations as they reflect the AOCS performance and characteristics. We present significant systematic effects in the inter-satellite pointing and discuss their possible sources. Prominent features are especially related to the magnetic torquer characteristics, star cameras’ performance and KBR antenna calibration parameters. The relation between the magnetic torquer attitude control and the Earth magnetic field, impact of the different performance of the two star camera heads on the attitude control and the features due to uncertainties in the calibration parameters relating the star camera frame to K-frame are discussed in detail. Proper understanding of these effects will help to reduce their impact on the science data and subsequently increase the accuracy of the gravity field solutions. Moreover, understanding the complexity of the onboard system is essential not only for increasing the accuracy of the GRACE data but also for the development of the future gravity field satellite missions.     

综合化飞行器管理计算机技术研究

目前国外新一代飞机的设计中,为进一步提高飞机的性能,同时降低系统费用,采用飞行器管理系统综合管理包括飞行控制、发动机控制、机电公共设备管理等飞机平台的功能.飞行器管理系统核心是飞行器管理计算机,细粒度可配置飞行器管理计算机不同于以往基于通道容错的计算机系统,它是基于模块级容错的计算机系统,细粒度可配置飞行器管理计算机设计利用综合化技术,通过采用通用的、标准的模块,提高系统的可靠性和可用性.它既要具有飞行控制系统的多余度安全,同时又需要满足发动机控制、机电管理等不同系统、不同余度配置的安全要求.另一方面飞行器管理计算机从系统结构、容错技术等方面要适应不断变化的微电子技术和计算机技术的发展,保持飞机平台具有相对的稳定性,更要具有灵活的系统配置能力.主要介绍了细粒度可配置飞行器管理计算机体系结构、软件要求、容错结构的实现.     

直角切削6061-T6铝合金剪切区力学行为及微观结构演化预测

力学行为是塑性变形微观过程的宏观表现,早期的金属切削理论模型没有考虑微观结构对切削力的影响。在考虑热力耦合效应的基础上建立了基于位错密度材料模型的6061-T6铝合金直角切削力预测模型,分析了不同切削参数下基于位错运动的塑性变形机制对切削力的影响。结合等分剪切区和非等分剪切区模型,构建了第一变形区多物理场计算方法,提出一种切屑形成过程中由塑性变形引起的微观结构演化解析模型。通过测量切削力和切屑内晶粒尺寸对模型的可行性进行了初步验证。结果表明：剪切区长度变长引起参与位错滑移的材料增多是切削深度增大导致切削力增大的主要原因。增大切削速度导致切削力的降低不是单一变量影响的结果,而是应变降低引起位错增殖数量减少和温度升高引起位错湮灭作用增加的共同作用结果。非等分剪切区模型正确反映了第一变形区温度和应力的分布特征,且与二维有限元模型分布相一致,建立的第一变形区微观结构演化解析模型能够预测切屑内位错密度和晶粒尺寸。     

大型固体发动机燃烧室立式贮存研究

为研究大型固体发动机对特殊立式贮存环境的适应性,开展了大型固体发动机立式贮存状态的受力分析以及立式贮存试验研究。基于大型固体发动机立式贮存环境条件的分析,综合考虑固化降温、充气内压等因素对发动机立式贮存的影响,开展了联合载荷作用下的计算分析。研究结果表明,发动机立式贮存状态相对初始状态前、后人工脱粘间隙都增大,前人工脱粘间隙增大较多,前人工脱粘开口部位轴向位移最大,中孔径向位移最大;发动机充气后药柱的变形量、前后凸环形药柱界面及药柱中孔处等效应力应变随内压提高有所提高,但前后凸环形药柱界面和药柱中孔处受力状态从三向或两向受拉变为三向受压状态,设计合适的充气内压有利于发动机的长期立式存放。燃烧室立式贮存试验实测了药柱立式贮存后的变形,实测结果与计算结果趋势一致。     

嵌金属丝端燃装药方案绝热层设计方法

根据固体火箭发动机绝热防护模型,提出了一种嵌金属丝端燃装药绝热层设计方法。用该法对某特定发动机燃烧室绝热层的设计结果表明:与动机原绝热层烧蚀相比,用本方法设计的绝热层可在绝热防护达到安全要求的同时,最大化地降低发动机消极质量。