航天器抓捕后复合体系统稳定的协调控制研究

针对航天器抓捕后由于系统质量特性和动量的改变而导致复合体系统失稳的问题,提出了两种基于角动量守恒的协调控制方法:关节阻尼控制和关节函数参数化协调控制。这两种方法通过对各关节和飞轮的速度进行协调规划和控制,实现对系统角动量的管理和重分配,在实现对目标进行停靠的同时,保证了基座的稳定性。两种方法各有优缺点,其中,关节函数参数化在实现系统稳定的同时还可使机械臂处于期望的臂型,以方便开展在轨维修等服务操作。所提出的方法将实际飞轮作为动量交换装置,具有很好的工程可实现性。仿真结果验证了方法的有效性。     

屏幕录象系统的开发与设计

屏幕实时拷贝功能是日常计算机使用中常用的功能之一，经研究发现，该功能的实现，主要应该实现计算机音频数据的捕获、屏幕视频数据的捕获，以及影音文件的合成三方面的功能。文中详细说明了系统开发的基本思想、算法和实现方法，经实践证明该方法切实可行。目前该屏幕录象系统，已经广泛应用于计算机软件操作说明的制作，以及动态多媒体教学等方面。     

基于IMD的Windows网络数据包拦截技术及应用

随着网络安全问题日益严重,网络安全产品也被人们重视起来。所有基于Windows操作系统的桌面防火墙核心技术点在于Windows操作系统下网络数据包拦截技术。主要介绍了Win dows操作系统下网络数据包拦截的技术,特别是基于IMD的网络数据包拦截方法以及应用。     

基于实际切齿方法的螺旋锥齿轮建模与实体设计

基于螺旋锥齿轮副中大轮采用的半滚切法加工原理,提出一种螺旋锥齿轮建模方法,推导出内、外齿顶线方程。应用MATLAB求解齿顶线方程,将结果导入SolidWorks软件生成曲线,基于扫描切除特征得到螺旋齿面,建立了螺旋锥齿轮的三维实体模型。最后通过具体实例说明了实体设计过程。     

某降落伞伞绳断裂仿真分析

分析了在降落伞充气过程伞衣织物的传力路线 ,得出当连接伞衣的某根伞绳断裂之后其上的力将由与其邻的伞绳承担。并且采用动力学仿真软件ADAMS进行建模 ,针对 5种情况进行分析得出伞绳间隔断裂时最危险伞绳承受的力比伞绳连续断裂时要大     

CBERS-02星红外数据系统正反扫描行配准方法研究

CBERS-02星搭载的有效载荷有一台是红外多光谱扫描仪（IRMSS），它是摆扫式的相机，与推扫式的CCD相机成像方式不同。摆扫式IRMSS相机的几何校正处理对比推扫式相机更为复杂，特别是正反扫描行之间，容易出现不配准、有缝隙或叠加等问题。文章根据IRMSS成像的机理，对CBERS-02星IRMSS图像存在的扫描行不配准问题进行了改进，达到了良好的效果。     

无人机栖落机动建模与轨迹优化

对固定翼无人飞行器栖落机动的纵向运动进行了气动特性建模与轨迹优化设计。通过运动捕捉系统测量获得试验滑翔机实时飞行数据,并结合统计学原理和平板气动理论建立了气动模型和动力学模型。针对所建立的模型采用GPOPS优化工具箱设计了栖落机动标称轨迹。优化结果表明,不同初始速度条件下执行栖落机动的空间需求不同,但最终都可以实现以相同的栖落速度落到同一位置。     

Testing baseline stability of some neutron monitors in Europe,Africa, and Asia

For six decades, the global network of neutron monitors (NMs) has provided a continuous stream of very valuable data to the heliophysics community, leading to many insights into the myriad modes of charged particle transport in the tangled magnetic fields that permeate the 3D heliosphere. Earlier, Ahluwalia and Ygbuhay (2012) reported on the drifts in some high latitude NM counting rates in the American zone. We continue our enquiry by testing the stability of the counting rate baselines of some NMs operating in Europe, Africa, and Asia. The data from these detectors have been extremely valuable for the short-term time variation studies, but caution is advised in using the data for long-term studies from NMs with baselines that are drifting for cause(s) unknown.     

On the Measurements of D/H in QSO Absorption Systems Closing in on the primordial abundance of deuterium

We present our measurements of the deuterium to hydrogen ratio (D/H) in QSO absorption systems, which give D/H = 3.40 ± 0.25 × 10-5 based on analysis of four independent systems. We discuss the properties of two systems which provide the strongest constraints on D/H. We outline the systematic effects involved in measurements of D/H and introduce a sophisticated method of analysis which properly accounts for these effects.     

Probing the first stars and black holes in the early Universe with the Dark Ages Radio Explorer (DARE)

A concept for a new space-based cosmology mission called the Dark Ages Radio Explorer (DARE) is presented in this paper. DARE’s science objectives include: (1) When did the first stars form? (2) When did the first accreting black holes form? (3) When did Reionization begin? (4) What surprises does the end of the Dark Ages hold (e.g., Dark Matter decay)? DARE will use the highly-redshifted hyperfine 21-cm transition from neutral hydrogen to track the formation of the first luminous objects by their impact on the intergalactic medium during the end of the Dark Ages and during Cosmic Dawn (redshifts z = 11–35). It will measure the sky-averaged spin temperature of neutral hydrogen at the unexplored epoch 80–420 million years after the Big Bang, providing the first evidence of the earliest stars and galaxies to illuminate the cosmos and testing our models of galaxy formation. DARE’s approach is to measure the expected spectral features in the sky-averaged, redshifted 21-cm signal over a radio bandpass of 40–120 MHz. DARE orbits the Moon for a mission lifetime of 3 years and takes data above the lunar farside, the only location in the inner solar system proven to be free of human-generated radio frequency interference and any significant ionosphere. The science instrument is composed of a low frequency radiometer, including electrically-short, tapered, bi-conical dipole antennas, a receiver, and a digital spectrometer. The smooth frequency response of the antennas and the differential spectral calibration approach using a Markov Chain Monte Carlo technique will be applied to detect the weak cosmic 21-cm signal in the presence of the intense solar system and Galactic foreground emissions.