关于地球卫星运动中的坐标系附加摄动问题

关于卫星运动中的坐标系附加摄动，早期是从两种赤道坐标系中卫星轨道根数的差别采用大量球面三角公式的方法导出的，本文将改用与当今高精度数值解中的坐标转换关系，在岁差章动等参数完全一致的情况下，简要清晰地导出相应的坐标系附加摄动解，既容易被读者接受，又便于与对应的数值解进行比对。     

SBN:一种新的Peer-to-Peer覆盖网络构造协议

 提出了一种新的动态模拟蝶形网络的P2P( Peer to Peer ) 覆盖网络组织结构强蝶形网络( Strong Butterfly Network, 简称SBN), 论证了其基本的网络特性, SBN 可以以常数级的度达到对数级的路径长度, 或者增加到对数级的度达到接近优化的路径长度。与目前其他的DHT( 分布式哈西表) 相比, SBN 能够表现因特网的多样性, 并利用这种多样性提供更好的性能和数据可靠性。与同样是基于蝶形网络的Viceroy 项目相比, SBN 具有较优异的性能, 同时更具有良好的可扩展性。     

按劳分配应有新的实现形式--从资本家剥削的产权分析中得出的命题

劳动力产权是一组权利束,资本主义国家的雇佣劳动制度造成了劳动力产权的残缺,资本家的剥削收入来自对雇佣工人劳动力所有权收入的侵蚀.我国实行社会主义市场经济,传统的按劳分配面临许多现实性障碍,所以应进行按劳分配实现形式的创新,采用双层分配机制,把按劳动力价值分配和按劳动力所有权分配结合起来,确保劳动力产权在分配上的完整实现.     

航迹规划中雷达探测空间的生成

从飞机突防习行任务规划出发，综合考虑地球曲率、陆地（或海洋）的反射和杂波干扰、大气折射和吸收损耗等因素的影响，采用临界散射截面法生成了对空警戒雷达在不同地貌、发现概率下，对不同雷达散射截面的目标的探测空间。计算并分析了飞行高度、目标雷达散射截面、发现概率和地貌等因素对雷达探测空间的影响，以便选择低探测概率的飞行走廓，这对制定和实施安全突防飞行策略有实际意义。     

Deep Impact Mission Design

The Deep Impact mission is designed to provide the first opportunity to probe below the surface of a comet nucleus by a high-speed impact. This requires finding a suitable comet with launch and encounter conditions that allow a meaningful scientific experiment. The overall design requires the consideration of many factors ranging from environmental characteristics of the comet (nucleus size, dust levels, etc.), to launch dates fitting within the NASA Discovery program opportunities, to launch vehicle capability for a large impactor, to the observational conditions for the two approaching spacecraft and for telescopes on Earth.     

俯仰敏捷性评估与影响因素研究

建立了现代高机动性能战斗机俯仰敏捷性仿真计算数学模型和机动飞行时的操纵动作，以Ｆ－１６战斗机为例，计算并讨论了初始飞行状态以及飞行控制系统参数对战斗机俯仰敏捷性的影响。结果表明，选择适当的飞行状态，有利于更好地发挥飞机的俯仰敏捷性；降低飞机整体系统的阻尼，将有利于提高飞机的俯仰敏捷性；控制系统有关参数的设计，除考虑飞行品质要求外，还需综合考虑飞机敏捷性等方面的要求。     

基于ATE技术的末制导雷达“天线对零”实现方案

在叙述“天线对零”过程重要性的基础上,介绍了基于ATE技术的末制导雷达“天线对零”自动过程的实现方案。该自动“天线对零”方案已经应用在“末制导雷达通用检测系统”中,保证了系统的高精度自动化测量。     

一种用于逐次逼近ADC的低电压高准确度比较器

设计了一种用于逐次逼近结构ADC中的低电压比较器,比较器由前置开关预放器和动态锁存器组成。前置放大器完成对输入信号进行放大,其高增益提高了比较器的准确度,动态锁存器的正反馈提高了比较器的速度。采用了0.6μm CMOS工艺设计,工作于2.5 V单电源电压,通过详细的电路原理分析和软件SMATSPICE的仿真,得到的分析和仿真结果说明该比较器具有速度快、准确度高、功耗小的特点,适用于逐次逼近结构中的低电压模数转换器。     

Did life exist on Mars? Search for organic and inorganic signatures, one of the goals for “SAM” (sample analysis at Mars)

Observation of Mars shows signs of a past Earth-like climate, and, in that case, there is no objection to the possible development of life, in the underground or at the surface, as in the terrestrial primitive biosphere. Sample analysis at Mars (SAM) is an experiment which may be proposed for atmospheric, ground and underground in situ measurements. One of its goals is to bring direct or indirect information on the possibility for life to have developed on Mars, and to detect traces of past or present biological activity. With this aim, it focuses on the detection of organic molecules: volatile organics are extracted from the sample by simple heating, whereas refractory molecules are made analyzable (i.e. volatile), using derivatization technique or fragmentation by pyrolysis. Gaseous mixtures thus obtained are analyzed by gas chromatography associated to mass spectrometry. Beyond organics, carbonates and other salts are associated to the dense and moist atmosphere necessary to the development of life, and might have formed and accumulated in some places on Mars. They represent another target for SAM. Heating of the samples allows the analysis of structural gases of these minerals (CO₂ from carbonates, etc.), enabling to identify them. We also show, in this paper, that it may be possible to discriminate between abiotic minerals, and minerals (shells, etc.) created by living organisms.     

A space radiation shielding model of the Martian radiation environment experiment (MARIE)

The 2001 Mars Odyssey spacecraft was launched towards Mars on April 7, 2001. Onboard the spacecraft is the Martian radiation environment experiment (MARIE), which is designed to measure the background radiation environment due to galactic cosmic rays (GCR) and solar protons in the 20–500 MeV/n energy range. We present an approach for developing a space radiation-shielding model of the spacecraft that includes the MARIE instrument in the current mapping phase orientation. A discussion is presented describing the development and methodology used to construct the shielding model. For a given GCR model environment, using the current MARIE shielding model and the high-energy particle transport codes, dose rate values are compared with MARIE measurements during the early mapping phase in Mars orbit. The results show good agreement between the model calculations and the MARIE measurements as presented for the March 2002 dataset.