空间遥感器大口径轻量化扫描镜材料发展与制作方法探讨

扫描镜是光机扫描型空间遥感器的重要组成元件。文章针对目前空间遥感器上应用的大口径轻量化扫描镜,从材料和制作方法方面进行了一定的技术研究。     

闪电成像仪的实验室定标

闪电成像仪是对地静止的天底成像遥感器,被优化适于在白天和夜间探测和定位闪电。实验室定标是发射前的业务,其作用在于保证遥感器在轨运行的性能。文章着重讨论实验室性能定标。     

一种新型的角加速度传感器

对一种新型角加速度传感器的工作原理和一些关键技术进行了阐述和分析。     

红外光学式二氧化碳分压传感器

介绍一种红外光学式二氧化碳分压传感器，该传感器基于朗伯－比尔定律，采用光源稳流，单片机温度偿及选用高性能红外探测器等技术，能够对二氧化碳气体进行有效准确地测量和分析，且结构简单，体积小，重量轻，功耗低，响应速度快，可靠性高，具有广阔的应用前景。     

准LIGA技术的研究与发展

介绍近年来准ＬＩＧＡ技术发展的概况，着重讨论国内外对它的各个工艺过程所采取的一些措施及其在微传感器和微执行器中的应用，并简单论述它的发展趋势。     

传输型光学遥感器斜模式采样新方法研究

文章介绍了实现超模式采样焦平面3种解决方案面临的技术难点,为避开器件问题提出了一 种新的斜模式采样方法。以任意两雏周期采样理论为基础分析了斜模式采样技术的物理原理,并通过实验 手段验证了斜模式采样技术的可行性。试验结果表明:改变探测器推扫方向的采样间距,斜模式采样技术 可以提高传输型光学遥感器图像的空间分辨率,该技术相对于超模式采样技术,工程实现上要简单。     

发动机热流传感器的蒸发冷却技术

本文介绍发动机热流传感器的设计和初步试验,描述了蒸发器的结构原理,从理论上并通过试验分析了影响蒸发器效率的某些因素,如:放气阀的预压力,水的充装量和散热头部的结构尺寸。试验表明,所设计的蒸发器达到了预定的性能指标。     

航天器的故障建模与应用

针对航天器工程中的典型故障进行分析与建模.首先给出几种典型故障作用模式的具体数学形式,然后分别采用状态描述矩阵对执行机构和传感器故障进行刻画,其不同的取值对应上述不同的故障模式.另外,使用有界范数和凸面体两种形式对系统故障数学建模.通过对航天器工程中的部件故障建模可为故障诊断和容错设计提供必要的数学描述.最后通过实例简...     

一种小型化无线传感网络的设计

采用zigbee技术实现基于mems传感器的无线传感网络节点小型化设计,组成的小型化系统可用于航天器各仓段内部温度、湿度、压力、加速度等状态参数的监测。小型化无线传感网络采用集中供电方式即可以减小节点体积,又便于后续电池更换。传感器信号无线传输方式,可以大大减少航天器电线电缆的数量、减小布线带来的困难及航天器总体质量。     

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.