测量船多设备外测数据的融合算法

为了进一步提高航天测量船外弹道数据处理的精度,须根据不同的任务特点和要求选用合适的数据处理方法。针对测量船精度校飞时多设备同时跟踪飞行目标的工程背景,提出多设备外弹道数据融合处理的构思,根据数据融合的原理阐述了数据融合技术在精度校飞数据处理中的应用,给出目标位置融合的几种算法,并用加权最小二乘数据融合算法对实测数据进行处理。工程应用结果表明：本文提出的数据融合方法计算量少、精度高,适合工程应用。     

一种新的直流电压源增益校准方法设计与分析

针对校准实验室直流电压源量程增益校准的问题,提出了采用参考标准源和数字多用表直接校准DUT量程增益的新方法。此方法校准误差只与所选设备技术指标有关,便于在一般校准实验室开展且可以实现自动校准。实验结果表明,新方法与传统的电阻分压式方法相比,二者在校准精度上有较好的一致性,在1V~1000V量程范围,新方法的校准结果扩展不确定度可达到0.3μV/V.     

Highlights of the Brazilian Solar Spectroscope

The digital, decimetric (950–2500 MHz) Brazilian Solar Spectroscope (BSS, Sawant, H.S., Subramanian, K.R., Faria, C., et al. Brazilian Solar Spectroscope (BSS). Solar Phys. 200, 167–176, 2001) with high time (10–1000 ms) and frequency (1–10 MHz) resolution is in regular operation since April, 1998, at the National Space Research Institute (INPE) at São José dos Campos, Brazil. The BSS has now been upgraded with a new digital data acquisition and data processing system. The new version of the BSS has improved the observational possibilities with the capability to record up to 200 frequency channels available in the selectable frequency range 950–2500 MHz. The GPS receiver permits the acquisition of data with time accuracy in the order of 0.1 ms. The software system of the BSS is composed by two distinct modules: the first, data acquisition system provides a flexible Graphical User Interface (GUI) that allows one to choose the observational parameters. The second module is the real time visualization system that permits real time visualization of the observed dynamic spectrum and additionally allows procedures for visualization and preliminary analysis of the recorded solar spectra. Using the new visualization system, we have realized two new types of dm-radio fine structures: narrow band type III bursts with positive as well as negative group frequency drift and dots emissions arranged in zebra-like and fiber-like chains. Furthermore, we have found flare generated fast wave trains according to their tadpole signature in wavelet power spectra for a decimetric type IV radio event (June 6, 2000 flare).     

智能检测技术在靶场测控设备中的应用及前景

综合运用先进的GPS授时技术和数字仿真、虚拟仪器结构、可视化编程等计算机软件技术，构建新一代靶场智能型检测系统，解决对野外分散站点上测控设备进行检测、标校、监控和测控网通信联试等技术问题。着重阐述智能化检测技术在靶场的应用及发展趋势，为技术人员开发测试软件提供参考。     

夸贾林导弹靶场的现代化改造

为减少操作和维护 (O&M)费用 ,增强靶场设备能力 ,夸贾林导弹靶场于 1997年夏开始对目标特性雷达、遥测和光学设备以及靶场指控中心进行升级改造 ,2 0 0 3年 2月改造取得圆满成功。本文主要介绍此次改造的相关内容及特点     

基于庞加莱映射的多站数据融合算法

针对目前单目标跟踪数据融合中存在的伪数据问题,研究了基于庞加莱映射的补充条件定位引导算法和多站抗野值数据融合算法,建立了适应实际传感器数量变化的数据融合体系。理论分析和仿真结果均证明,该方法可行有效。     

紧缩场超高频(UHF)天线测试方法的研究

针对CCR120／100紧缩场超高频（UHF）天线测试的问题,根据紧缩场的现有条件,给出了利用紧缩场进行UHF天线辐射特性测试的方法,以及进一步提高测试精度的方法,以满足卫星UHF频段天线辐射特性测试的需求。     

RadioAstron reveals super-compact structures in the bursting H2O maser source G25.65+1.05

Water masers are well-known to be variable on a variety of time scales, but only three Galactic H₂O masers are known to flare to the level of 10⁵–10⁶ Jy (${\text{T}}_{\text{B}}\sim {10}^{17}$ K): Orion KL, W49N, and the recently discovered G25.65+1.05. Recently detected flaring activity of H₂O maser in the massive star-forming region G25.65+1.05 gave us a unique opportunity to study the fine structure of H₂O maser emission in the bursting state with extremely high space VLBI angular resolution. Observation of the source was carried out with ∼9 Earth diameter space-ground baseline within the framework of the RadioAstron project. H₂O maser emission from two spectral features, including the bursting one, was detected in the experiment. Only ∼1% of the bursting H₂O maser emission was detected on the space-ground baselines: it indicates the presence of a very compact spatial structure with a size of ∼25 $\mathrm{\mu }$as, which corresponds to 0.05 AU or ∼5 solar diameters at the distance to the source of 2.08 kpc, and the brightness temperature of ∼3 × 10¹⁶ K. Analysis of the flux density as a function of the baseline length for the bursting H₂O maser feature in the source shows that most of the emission comes from an extended “halo” structure, while the core of emission is very compact and has an extreme brightness temperature. These results are in agreement with the model of interacting maser clouds considered as the likely explanation of the nature of the burst in the source. Under the assumption of such a model, the beam size of maser emission is reduced while the brightness temperatures similar to the highest observed values are produced.     

基于变参数广义结构的距离扩展目标检测方法

针对特定杂波背景下的最优或次优检测器结构难以适应过渡杂波环境的问题，首先，给出基于变参数广义结构的距离扩展目标检测器，通过调整参数来适应杂波特性。其次，确定检测器最佳参数的经验公式，经验公式符合数值结果。最后，利用仿真试验分析检测器的检测性能。仿真结果表明，在介于高斯和复合高斯杂波之间的过渡环境中，提出的检测器比现有检测器具有更加优异的目标检测性能，对杂波非高斯程度时空渐变性具有较强的适应能力。     

Navigation message designing with high accuracy for NAV

Navigation message designing with high accuracy guarantee is the key to efficient navigation message distribution in the global navigation satellite system（GNSS）. Developing high accuracy-aware navigation message designing algorithms is an important topic. This paper investigates the high-accuracy navigation message designing problem with the message structure unchanged.The contributions made in this paper include a heuristic that employs the concept of the estimated range deviation（ERD） to improve the existing well-known navigation message on L1 frequency（NAV） of global positioning system（GPS） for good accuracy service; a numerical analysis approximation method（NAAM） to evaluate the range error due to truncation（RET） of different navigation messages; and a basic positioning parameters designing algorithm in the limited space allocation. Based on the predicted ultra-rapid data from the ultra-rapid data from the international GPS service for geodynamic（IGU）, ERDs are generated in real time for error correction.Simulations show that the algorithms developed in this paper are general and flexible, and thus are applicable to NAV improvement and other navigation message designs.