卫星群分离控制方法研究

根据星群分离控制的一般要求，本文研究了卫星群的相对运动方程，分析了其相对运动特性，在合理的近似假设下对Ｈｉｌｌ方程为出发点，研究了各卫星相对距离限制下的分离控制方法。最后对精确方程与近似方程的仿真比较，表明所设计的健康控制方法是可行的，其结果是可信的。     

NEPE固体推进剂动态力学性能的研究

利用傅立叶红外光谱仪及扭辫法研究了不同粘合剂系统中异氰酯活性基团与羟基基团的当量比值，扩链剂以及预聚时间对ＮＥＰＥ固体推剂的次级转变温度、等参量的影响。研究结果对该类推进剂配设计和工艺参量选择提供了必要的实验依据。     

含催化剂RDXCMDB推进剂燃烧机理研究

利用常压ＤＳＣ及ＴＧ／ＤＴＧ，高压ＤＳＣ，单幅照相和燃烧波温度分布测试技术对含ＲＤＸ的复合改性双基推进剂（ＲＤＸＣＭＤＢ）含和不含催化剂时的燃烧机理进行了研究，得到了该种推进剂在热分解和燃烧方面的一些重要结果。     

关于我国遥感卫星数据源工程建设的思考

一、迎接对地观测新的发展高潮本世纪末,在经济、社会、科技发展的巨大推动下以及环境、资源问题的巨大压力下,随着空间科学技术的迅速发展,我们面临着一个世界范围的对地观测技术新的发展高潮。1.传统的卫星遥感数据源能力在增强以70年代初陆地卫星-1发射为里程碑,近30年形成了以美国陆地卫星、法国斯波特民用遥感卫星系列为主流的地球资源环境卫星遥感数据源,同时也发展了日本的海洋观测卫星-日本地球资源卫星-先进地球观测卫星系列、加拿大的雷达卫星系列、印     

耦合多体系统动力响应计算

由于弹性体与刚体之间的动力耦合，使得耦合多体系统的特征值问题非自共轭，难以用经典的模态分析方法解决含有刚、弹耦合多体系统的动力响应问题。本文以某多体系统为例，建立了耦合多体系统的特征值和边值问题的增广公式，进而求得了用正交的增广特征矢量级数表示的系统对任意激励的响应。     

中低轨道卫星星座间的激光链路

阐述在中低轨道卫星星座全球通讯网络中应用的激光星间链路与在中继星间应用的激光星间链路相比，所具有的明显的优势。同时给出了应用于小卫星上的小光学用户终端的基本组成，并指出了当前在中低轨道卫星星座激光星间链路研究中所应当进行的主要研究方面。     

Solar particle events and the International Space Station

The high inclination orbit for the International Space Station poses a risk to astronauts on EVA during occasional periods of enhanced high energy particle flux from the sun known as Solar Particle Events. We are currently unable to predict these events within the few-hour lead time required for evasive action. Compounding the threat is the fact that station construction occurs during increasing solar activity and through the peak of the solar cycle. In this paper we present an overview of the risk, the current methods to provide forecasts of SPEs, and potential risk mitigation options.     

Metabolic assessments during extra-vehicular activity

Extra-vehicular activity (EVA) has a significant role during extended space flights. It demonstrates that humans can survive and perform useful work outside the Orbital Space Stations (OSS) while wearing protective space suits (SS). When the International Space Station 'Alpha' (ISSA) is fully operational, EVA assembly, installation, maintenance and repair operations will become an everyday repetitive work activity in space. It needs new ergonomic evaluation of the work/rest schedule for an increasing of the labor amount per EVA hour. The metabolism assessment is a helpful method to control the productivity of the EVA astronaut and to optimize the work/rest regime. Three following methods were used in Russia to estimate real-time metabolic rates during EVA: 1. Oxygen consumption, computed from the pressure drop in a high pressure bottle per unit time (with actual thermodynamic oxygen properties under high pressure and oxygen leakage taken into account). 2. Carbon dioxide production, computed from CO2 concentration at the contaminant control cartridge and gas flow rate in the life support subsystem closed loop (nominal mode) or gas leakage in the SS open loop (emergency mode). 3. Heat removal, computed from the difference between the temperatures of coolant water or gas and its flow rate in a unit of time (with assumed humidity and wet oxygen state taken into account). Comparison of heat removal values with metabolic rates enables us to determine the thermal balance during an operative medical control of EVA at "Salyut-6", "Salyut-7" and "Mir" OSS. Complex analysis of metabolism, body temperature and heat rate supports a differential diagnosis between emotional and thermal components of stress during EVA. It gives a prognosis of human homeostasis during EVA. Available information has been acquired into an EVA data base which is an effective tool for ergonomical optimization.     

先进发射系统使用的通用发动机概念及降低成本的途径

讨论通用发动机设计概念及其在运载火箭上的应用，对发动机计划成本和成本节约进行估算，并与助推级、芯级独立使用发动机的设计和研制相比较。     

地球观测系统时代之后的成像光谱技术

地球观测系统(EOS)时代将向地球系统科学遥感界提供有关大气、陆地表面和海洋间相互作用的大量新信息。由EOS-1平台上的高分辨率成像光谱仪(HIRIS)等仪器提供的高光谱和空间分辨率图像将成为EOS数据集的重要组成部分。可以预料,利用EOS可以进一步认识地球,但也要求未来的传感器比现有的这一代传感器具有更高的灵活性和测量能力。声光可调谐滤光器(AOTF′S)良好的光谱灵活性、偏振选择性及简单性预示着它在未来的成像光谱仪上的重要应用。AOTF′S是致密、紧固的固态晶体,它可对两种偏振态进行快速的(毫秒级)、电控的光谱调谐。本文将讨论基于AOTF的成像光谱仪的基本原理。