一种再生测距伪码的自适应捕获技术

深空探测距离远,适合使用再生伪码测距技术。针对空间数据系统咨询委员会（CCSDS）提出的T2B测距复合伪码,计算了其6个子码在不同延拓周期下的相关值,推导了星上相关运算前信号噪声的分布形式。在对判决量统计特性分析的基础上,采用最大似然估计准则（MLE）对噪声标准差进行了合理估计,通过噪声标准差估计了判决门限,并采用奈曼...     

采用MPPT技术的国外深空探测器电源系统综述

最大功率点跟踪（MPPT）技术能够最大限度利用太阳电池阵输出功率,对于光强和温度变化较大的深空探测器,具有一定的优势。对MPPT电源系统拓扑结构及其在国外深空探测领域的典型应用,如＂罗塞塔＂（Rosetta）、＂信使＂（MESSENGER）探测器电源系统等,进行了调研和综述,分析了3种MPPT拓扑结构的特点,并指出光强、温度等空间环境因素,以及负载特性、系统稳定性对电源系统的影响,可为MPPT技术在我国深空探测器电源系统设计中应用提供参考。     

归因于空间环境的航天器故障与异常

天然空间环境对航天器设计、研制和运行的影响是NASA马歇尔空间飞行中心系统分析和集成实验室电磁与航空宇宙环境部组织编写的一系列NASA RP报告的主题。其中,NASA RP-1390详细概述了天然空间环境7个主要环境因素,包括它们的简单定义、相关的型号计划事项以及对各种航天器分系统的影响。该报告提供100多个从1974～1994年间发生的归因于天然空间环境的航天器故障和异常的案例,统计分析天然空间环境及其对航天器的影响。文章是对这篇报告的介绍与点评。     

临近空间短波红外多光谱成像技术

伪装、隐身技术的发展,使传统的探测、侦察手段已难以适应要求.在临近空间平台上进行多光谱、高光谱对地探测,可以在敌方一定程度的伪装、隐身条件下完成对目标区域的成像侦察,有效地识别地面的各类伪装、空中隐身飞行器等军事目标.开展了临近空间机栽短波红外多光谱成像技术探索性研究,取得了初步成果.     

基于WinCE的发动机试验实时控制软件设计

通过对WinCE操作系统线程、进程和定时器的分析,采用多媒体定时器和外围硬件配合的方式,结合XXX液体火箭发动机试车台增压/闭环控制系统实时时序控制的设计和应用,系统论述了在WinCE操作系统下,实时控制的实现原理和设计方法,并阐述了基于多媒体定时器实时控制软件设计框架的应用前景。     

核热推进技术综述

分析了核热推进相对于现有传统推进技术的优势,介绍了可能的技术实现途径,重点是目前已经实现的固相核热推进技术,并归纳了有关文献对于固相核热推进技术的空间应用分析结果;介绍了核热推进技术的发展历程,并对当前发展态势进行了分析;最后针对我国发展核热推进技术提出几点考虑。     

基于FFT的抑制载波捕获技术

介绍三种基于快速傅里叶变换(FFT)的开环抑制载波捕获技术,并对这些算法进行性能分析及仿真.结果表明,基于FFT的交错符号积分技术,在低符号信噪比时引入的信噪比损失最小,适用于深空接收机中抑制载波捕获.     

关于域F上的向量空间V的一个性质的证明

利用扩张域论述方法，证明域Ｆ上的向量空间Ｖ的一个基本性质，即在Ｆ上，Ｖ关于Ｆ的基底的元数等于维数（Ｖ：Ｆ）。     

Coronal Mass Ejections

This workshop summary tries to distill the key difficulties and questions in the art of (I)CME physics and strategies to address them. (I)CMEs are multi-dimensional, multi-parameter, and multi-scale phenomena related to the solar dynamo, corona, and heliosphere. This workshop illustrates the immense progress made in describing and modeling these spectacular energetic solar events, but also shows clear shortcomings in our understanding of them.     

Cassini Plasma Spectrometer Investigation

The Cassini Plasma Spectrometer (CAPS) will make comprehensive three-dimensional mass-resolved measurements of the full variety of plasma phenomena found in Saturn’s magnetosphere. Our fundamental scientific goals are to understand the nature of saturnian plasmas primarily their sources of ionization, and the means by which they are accelerated, transported, and lost. In so doing the CAPS investigation will contribute to understanding Saturn’s magnetosphere and its complex interactions with Titan, the icy satellites and rings, Saturn’s ionosphere and aurora, and the solar wind. Our design approach meets these goals by emphasizing two complementary types of measurements: high-time resolution velocity distributions of electrons and all major ion species; and lower-time resolution, high-mass resolution spectra of all ion species. The CAPS instrument is made up of three sensors: the Electron Spectrometer (ELS), the Ion Beam Spectrometer (IBS), and the Ion Mass Spectrometer (IMS). The ELS measures the velocity distribution of electrons from 0.6 eV to 28,250 keV, a range that permits coverage of thermal electrons found at Titan and near the ring plane as well as more energetic trapped electrons and auroral particles. The IBS measures ion velocity distributions with very high angular and energy resolution from 1 eV to 49,800 keV. It is specially designed to measure sharply defined ion beams expected in the solar wind at 9.5 AU, highly directional rammed ion fluxes encountered in Titan’s ionosphere, and anticipated field-aligned auroral fluxes. The IMS is designed to measure the composition of hot, diffuse magnetospheric plasmas and low-concentration ion species 1 eV to 50,280 eV with an atomic resolution M/ΔM ∼70 and, for certain molecules, (such asN ₂ ⁺ and CO⁺), effective resolution as high as ∼2500. The three sensors are mounted on a motor-driven actuator that rotates the entire instrument over approximately one-half of the sky every 3 min.This revised version was published online in July 2005 with a corrected cover date.