一种新型数字高精度伪码快速捕获延迟锁定环的设计与实现

介绍了一种新型全并行快速捕获延迟锁定环的设计与FPGA实现,捕获时间小于等于一个伪码周期,抗干扰容限大于80 dB。此快速捕获延迟锁定环实现127路全并行捕获和高精度跟踪,仅需存储130个PN码表,相对于其他并行捕获延迟锁定环或串并结合的环路,存储量约小2/3,并具有较高捕获精度。     

SiCp／Al复合材料微蠕变行为及其影响因素分析

 通过对碳化硅颗粒增强铝基复合材料（ＳｉＣｐ／Ａｌ）微蠕变性能的测试及微观组织分析,研究了ＳｉＣｐ／Ａｌ复合材料微蠕变变形规律及机理。结果表明,ＳｉＣｐ／Ａｌ复合材料微蠕变变形行为可分为二个阶段：第一阶段是可动位错的耗尽阶段；第二阶段位错全面开动、增殖是引起材料微蠕变的主要原因。材料内的增强体颗粒、析出相可有效的提高材料的微蠕变抗力。     

利用改正数信息的北斗三号实时精密单点定位及性能分析

北斗三号全球卫星导航系统已正式建成并开通服务。为了利用实时改正数信息系统地揭示北斗三号精密单点定位性能，并为用户提供理论依据和应用参考，首先解算了卫星实时精密轨道、钟差及其改正数，分析了其精度。然后基于实时改正数信息，利用监测站广播星历和观测数据，分别进行了双频静态、双频仿动态、单频静态和单频仿动态仿实时精密单点定位，以评估其性能。结果表明：北斗三号MEO卫星实时轨道和钟差精度均值分别约为12cm和0.2ns，满足实时精密单点定位需求。静态实时精密单点定位精度优于动态，双频优于单频，均可达到分米级。对于定位收敛时间，双频静态最短，约为40min；双频动态和单频静态均约为85min；单频动态最长，约为120min。     

基于运动形态学的掠地飞行器视频检测方法

 结合数学形态学、视频图像运动分析以及数学统计分析方法，提出了一种用于空中预警控制系统(AWACS)的小型掠地飞行器运动形态学视频检测方法。该方法首先应用形态学tophat滤波提取出视频图像中的可疑目标(SO)，并求取SO的运动参数，利用真实目标和类目标干扰的不同运动特性，应用数学统计的方法对各运动参数进行分析以剔除部分类目标干扰，从而获得潜在目标(PT)的灰度分布和运动参数。在应用形态学tophat滤波器进行可疑目标提取中，一种新的金字塔型结构元的引入有效减少了虚警数量。外场试验表明，该检测方法能够有效抑制航拍掠地飞行器视频图像中的地物干扰，降低虚警目标的数量。     

The Plasma Environment of Comet 67P/Churyumov-Gerasimenko Throughout the Rosetta Main Mission

The plasma environment of comet 67P/Churyumov-Gerasimenko, the Rosetta mission target comet, is explored over a range of heliocentric distances throughout the mission: 3.25 AU (Rosetta instruments on), 2.7 AU (Lander down), 2.0 AU, and 1.3 AU (perihelion). Because of the large range of gas production rates, we have used both a fluid-based magnetohydrodynamic (MHD) model as well as a semi-kinetic hybrid particle model to study the plasma distribution. We describe the variation in plasma environs over the mission as well as the differences between the two modeling approaches under different conditions. In addition, we present results from a field aligned, two-stream transport electron model of the suprathermal electron flux when the comet is near perihelion.     

原位反应合成Nb掺杂Al2O3/TiAl复合材料的显微结构分析

利用Al-Ti-TiO2体系原位反应合成了Nb掺杂Al2O3／TiAl复合材料。借助XRD和SEM研究了Nb掺杂Al2O3／TiAl的显微结构以及Nb引入量对复合材料显微结构的影响。结果表明，复合材料由TiAl、Ti3Al、Al2O3、Nb和NbAl3相构成，细小Al2O3颗粒分布于基体晶粒交界处，存在一定的团聚；Nb元素引入量的高低，可调节产物中TiAl和Ti3Al的相对含量，随Nb含量的增大，TiAl含量逐渐减少，Ti3Al则逐渐增大；同时，基体晶粒和Al2O3颗粒均有所细化，且分布逐渐均匀，材料的均匀性得到改善。     

Micro-X概念验证机热防护系统研究进展

简述了国外可重复使用运载器的研究现状及发展趋势，详细介绍了美国下一代可重复使用运载器Micro—X概念验证机的热防护材料及设计。     

Relationship Between Substorm Auroras and Processes in the Near-Earth Magnetotail

Although the auroral substorm has been long regarded as a manifestation of the magnetospheric substorm, a direct relation of active auroras to certain magnetospheric processes is still debatable. To investigate the relationship, we combine the data of the UV imager onboard the Polar satellite with plasma and magnetic field measurements by the Geotail spacecraft. The poleward edge of the auroral bulge, as determined from the images obtained at the LHBL passband, is found to be conjugated with the region where the oppositely directed fast plasma flows observed in the near-Earth plasma sheet during substorms are generated. We conclude that the auroras forming the bulge are due to the near-Earth reconnection process. This implies that the magnetic flux through the auroral bulge is equal to the flux dissipated in the magnetotail during the substorm. Comparison of the magnetic flux through the auroral bulge with the magnetic flux accumulated in the tail lobe during the growth phase shows that these parameters have the comparable values. This is a clear evidence of the loading–unloading scheme of substorm development. It is shown that the area of the auroral bulge developing during substorm is proportional to the total (magnetic plus plasma) pressure decrease in the magnetotail. These findings stress the importance of auroral bulge observations for monitoring of substorm intensity in terms of the magnetic flux and energy dissipation.     

Type II Solar Radio Bursts: Theory and Space Weather Implications

Recent data and theory for type II solar radio bursts are reviewed, focusing on a recent analytic quantitative theory for interplanetary type II bursts. The theory addresses electron reflection and acceleration at the type II shock, formation of electron beams in the foreshock, and generation of Langmuir waves and the type II radiation there. The theory's predictions as functions of the shock and plasma parameters are summarized and discussed in terms of space weather events. The theory is consistent with available data, has explanations for radio-loud/quiet coronal mass ejections (CMEs) and why type IIs are bursty, and can account for empirical correlations between type IIs, CMEs, and interplanetary disturbances. This revised version was published online in August 2006 with corrections to the Cover Date.     

连续小波变换应用于密集模态参数识别

用连续小波变换方法进行模态参数识别时,减小小波函数的带宽可以提高小波变换的频率分辨能力,但同时也会增大边沿效应,影响密集模态参数识别的精度。本文提出了极值位置方法,在模态耦合严重的小波脊附近,找到模态解耦最好的尺度,在此尺度上进行频率和阻尼的识别,可以获得较好的识别精度。使用Morlet小波函数,对GARTEUR飞机模型中的三阶密集模态进行识别,验证了该方法的有效性。