微纳InSAR卫星总体技术研究

微纳合成孔径雷达干涉(Synthetic Aperture Radar Interferometry, InSAR)卫星是对地定量化遥感的重要手段。开展了微纳InSAR卫星系统总体技术研究,给出了使得干涉测量覆盖范围最大的双星编队构型设计方法,建立了低燃料消耗双星轨道参数设计准则,提出高功能密度比InSAR卫星系统的设计方法,包括载荷平台一体化、卫星高集成模块化等总体设计方法,并给出了相应的设计实例。     

频谱分析法在静止气象卫星调焦分析中应用研究

利用频谱分析方法,对静止气象卫星扫描辐射计的在轨调焦进行快速、准确的分析判断,确定是否需要调整及调整时所发遥控命令的调整方向和步长等,避免了单向调出焦距极限位置时,对辐射计造成永久性损坏。文章首次提出的二维频谱法,即使在图像定位精度不高的情况下仍然适用,可以得出准确的分析结果。     

A global survey of COSMIC ionospheric peak electron density and its height: A comparison with ground-based ionosonde measurements

With a network of ground-based ionosondes distributed around the world, the ionospheric peak electron density and its height measured by FORMOSAT-3/COSMIC satellites in terms of GPS radio occultation technique are extensively examined in this article. It is found that, in spite of the latitude, the mean values of the peak electron density measured by COSMIC satellites are systematically smaller than those observed by ground-based ionosondes. The discrepancy between them is dependent on the latitude, namely, it is small in low and mid-latitudes and large in high-latitude region. Moreover, statistical analysis shows that the slopes of the regression line that is best fitted to the scatter diagram of occultation-retrieved peak electron density (ordinate axis) versus ionosonde-observed peak density (abscissa axis) are universally less than one. This feature is believed to be the result of path average effect of non-uniform distribution of the electron density along the GSP ray during the occultation. A comparison between COSMIC-measured peak height and ionosonde-derived peak height hmF2 indicates that the former is systematically higher than the latter. The difference in the two can be as large as 20% or more in equatorial and low-latitude regions. This result implies that the peak height hmF2 derived from the virtual height through true height analysis based on Titheridge method seems to underestimate the true peak height. The correlation between COSMIC and ionosonde peak electron densities is analyzed and the result reveals that correlation coefficient seems to be dependent on the fluctuation of the occultation-retrieved electron density profile. The correlation will be higher (lower) for the electron density profiles with smaller (larger) fluctuations. This feature suggests that the inhomogeneous distribution of the electron density along the GPS ray path during the occultation plays an important role affecting the correlation between COSMIC and ionosonde measurements.     

Remote upgrading of a space-borne instrument

The main purposes of experiment “Obstanovka” (“Environment” in Russian) consisting of several instruments are to measure a set of electromagnetic and plasma phenomena characterizing the space weather conditions, and to evaluate how such a big and highly energy consuming body as the International Space Station disturbs the surrounding plasma, and how the station itself is charged due to the operation of so many instruments, solar batteries, life supporting devices, etc. Two identical Langmuir electrostatic probes are included in the experiment “Obstanovka”. In this paper the Langmuir probes for “Obstanovka” experiment are described, including the choice of geometry (spherical or cylindrical), a more reliable method for the sweep voltage generation, an adaptive algorithm for the probe’s operation. Special attention is paid to the possibility for remote upgrading of the instrument from the ground using the standard communication channels.     

用纤内Bragg光栅进行动态应变测量的研究

描述了用纤内Bragg光栅进行动态应变测量研究的意义，原理和方法，提出了两种用纤内Bragg光栅动态应变测量时进行Bragg波长偏移量的解调方法；光干涉相位检测Bragg光栅反射波长偏移的解调方法和用DWDM密集波分复用器解调Bragg波长的方法，前者适用于高频宽带动态应变测量，后者适用于有限频率或中等频率响应的动态应变测量。     

星用非金属材料出气模型的应用

卫星上所用非金属材料，在空间真空环境下存在出气行为，产生污染效应。为了研究这种出气行为，本文以扩散理论为理论依据，推导材料出气模型。利用空间分子污染气体分析仪，测试了星用非金属材料的出气速率变化，对所测数据进行曲线拟合，通过试验和理论分析，证实了模型推导的正确性，结果表明：经过6h的真空加热预处理能够有效减少出气污染。     

光力惯性传感技术研究进展

光力惯性传感技术是利用光子与机械振子的相互作用,通过出射光的动量和角动量的变化实现对振子运动状态的监测,进而实现对其受力（矩）,以及（角）速度、（角）加速度测量的新型惯性传感技术。该技术既有高极限精度的原理优势,又有微型化的技术优势,是惯性传感技术的前沿领域,具有极大的发展潜力。首先介绍了基于光阱系统和微腔系统的两类光力惯性技术,分析了其基本工作原理与物理特征;其次介绍了国内外光力惯性传感器件的研究现状;最后对光力惯性技术的发展特点、国内外差距进行了总结,并给出了我国发展光力惯性传感技术的建议。     

多尺度自适应直接信息采样与重构

现有的直接信息采样(Analog-to-Information Conversion,AIC)方法在压缩感知框架下,将采集和压缩过程融合,但并未充分考虑不同稀疏成分在信号重构当中的地位。针对该不足之处,提出一种多尺度自适应直接信息采样与重构算法。该算法充分考虑小波变换后的高频信号和低频信号在重构中的不同地位,实现速率自适应的直接信息采样。同时,给出变速率采样下的信号重构策略,以解决常规重构算法在速率自适应采样时失效的问题。仿真结果表明,多尺度自适应AIC系统可以获得比传统AIC系统更好的AFSNR性能。     

原子传感用垂直腔面发射激光器研究进展

垂直腔面发射激光器(Vertical-cavity Surface-emitting Laser,VCSEL)是半导体激光器家族中的最重要成员之一,因其具有单纵模、低功耗、光束易整形等一系列独特优势,是多种微型化原子传感器的理想光源。围绕原子传感这一应用需求,国内外多个科研机构和企业对Rb原子和Cs原子传感用VCSEL开展了不同层次的研究,主要对其中的代表性研究进展进行综述。     

2019年国外导航技术发展综述

近年来,国外导航技术的发展呈现出多系统融合的发展态势,结合2019年国外导航技术的发展动态,对美国、欧盟、俄罗斯、印度等国家和地区的卫星导航、惯性导航、天文导航、视觉导航、数据库匹配导航、仿生导航、量子导航和全源导航等技术发展现状进行了总结分析,并对相关技术发展进行了展望。