高动态环境下惯组辅助GNSS接收机卫星导航信号的捕获

针对高动态环境下多普勒频移超出了接收机的搜索范围接收机无法捕获卫星导航信号这一问题,提出了利用INS辅助GNSS接收机卫星导航信号捕获的方法.该方法利用INS提供的载体位置、速度信息,并结合通过卫星星历(或历书)得到的卫星位置、速度估算载波多普勒频移,利用估算的载波多普勒频移重新设定GNSS接收机载波搜索中心频率,使G...     

GNSS接收机数字载波跟踪环建模与噪声性能分析

针对GNSS接收机高灵敏度跟踪问题,研究数字载波跟踪环热噪声相位颤动与相干积累时间长度的关系.在分析I·Q鉴相器的Costas载波环信号处理流程的基础上,建立了新的环路线性化模型.基于该模型,推导了由最佳模拟环路滤波器双线性变换离散化得到的数字载波跟踪环的噪声性能.数值分析表明:采用I·Q鉴相器的二阶、三阶数字载波环热噪声相位颤动,随相干积累时间的增大先减小后增大,存在热噪声相位颤动最小意义上的最佳相干积累时间.仿真结果验证了理论分析结论,同时表明新建模型对数字载波跟踪环的描述比传统模型更准确.文中给出的各载噪比和环路带宽组合条件下的最佳相干积累时间,可用于指导高灵敏度接收机载波跟踪环设计.     

天问一号探测器高动态着陆惯导系统设计与试验

考虑到火星探测任务着陆过程动态变化大,稀薄大气环境下开伞会对探测器产生剧烈晃动,为此天问一号探测器研制了一套高动态着陆惯导系统,从硬件产品、使用时序到导航算法方面均进行了针对性设计,以适应着陆过程中的高动态环境.此外,为验证天问一号探测器高动态着陆惯导系统的性能,设计了模拟火星开伞工况的火箭弹高空开伞试验,结果表明该高...     

用于压力传感器校准的高低温试验箱设计

基于压力传感器在高低温环境下的校准需求,设计了一种专用高低温试验箱。其控制温度范围可达到-120℃[KG-*4]~[KG-*7]500℃。提出了高低温试验箱的总体方案,介绍了宽温区温度的实现方法以及高温和低温系统不兼容的解决方法和控制流程。试验验证结果显示,高低温试验箱达到了实现宽温区温度的目的,满足设计指标要求。     

离散光谱分辨率对喷流红外特性FVM计算的影响

建立了辐射传递方程(RTE)的有限元体积法(FVM)计算模型,研究了离散光谱分辨率对FVM计算精度的影响,提出了离散光谱分辨率无关解的概念,并编制了相应的FORTRAN源程序,结合大气飞行发动机标准算例进行了一系列计算和比较.结果表明;在给定的红外光谱域中,随着离散光谱的分辨率的提高,计算出的方向光谱辐射强度渐渐趋向于同一个值.在航空发动机喷流2～5μm红外光谱区间中,当划分150个以上等间隔光谱微元后,FVM可以保证达到离散光谱分辨率无关解.      

基于CDMA蜂窝网的飞行器三维定位算法

针对中低空飞行器提出了一种将码分多址(CDMA)蜂窝网导频信号被动定位与惯性导航系统进行组合的导航定位方法。该定位方法是根据CDMA蜂窝网导频信号的到达时差（TDOA）进行两次加权最小二乘解算,并利用飞行器惯性组合的原始信息进行解模糊,从而实现中低空飞行器的三维实时定位。蒙特卡罗仿真证明：在高斯白噪声条件下,该算法运算速度快,精度高,其均方误差逼近克拉美罗下界（CRLB）,为组合导航实时性要求提供了理论参考。     

FY-3气象卫星中分辨率光谱成像仪结构仿真分析

用ANSYS软件仿真分析了风云三号（FY-3）气象卫星中分辨率光谱成像仪的结构。根据建立的成像仪有限元模型,进行了静力学、模态和谱分析,给出了X、Y、Z向加速度载荷下消旋机构的应力和变形、1-20阶模态频率,以及各向正弦振动谱作用下各部件的应力和变形。结果表明：有限元法与实验数据基本吻合,可用于成像仪设计的优化。     

几种典型迎风格式的分析与比较

重点分析了AUSM 格式的构造方法,同时将其与Van Leer, Roe格式等构造方法进行比较和分析,通过求解一维激波管问题,以及二维和三维跨音速流场的计算比较了AUSM 格式,VanLeer格式,Roe格式和中心格式的数值模拟结果和网格适应性,以及在经典四步Runge-Kutta显式时间推进和LU-SGS隐式时间推进下上述四种格式的计算效率.获取了对于基础研究和工程应用很有意义的结论.     

High resolution science with high redshift galaxies

We summarize the high-resolution science that has been done on high redshift galaxies with Adaptive Optics (AO) on the world’s largest ground-based facilities and with the Hubble Space Telescope (HST). These facilities complement each other. Ground-based AO provides better light gathering power and in principle better resolution than HST, giving it the edge in high spatial resolution imaging and high resolution spectroscopy. HST produces higher quality, more stable PSF’s over larger field-of-views in a much darker sky-background than ground-based AO, and yields deeper wide-field images and low-resolution spectra than the ground. Faint galaxies have steadily decreasing sizes at fainter fluxes and higher redshifts, reflecting the hierarchical formation of galaxies over cosmic time. HST has imaged this process in great structural detail to z  6, and ground-based AO and spectroscopy has provided measurements of their masses and other physical properties with cosmic time. Last, we review how the 6.5 m James Webb Space Telescope (JWST) will measure First Light, reionization, and galaxy assembly in the near–mid-IR after 2013.     

Semi-analytical investigations of high area-to-mass ratio geosynchronous space debris including Earth’s shadowing effects

This paper investigates the long-term perturbations of the orbits of geosynchronous space debris influenced by direct radiation pressure including the Earth’s shadowing effects. For this purpose, we propose an extension of our homemade semi-analytical theory [Valk, S., Lemaître, A., Deleflie, F. Semi-analytical theory of mean orbital motion for geosynchronous space debris under gravitational influence. Adv. Space Res., submitted for publication], based on the method developed by Aksnes [Aksnes, K. Short-period and long-period perturbations of a spherical satellite due to direct solar radiation. Celest. Mech. Dyn. Astron. 13, 89–104, 1976] and generalized into a more convenient non-singular formalism. The perturbations accounting for the direct radiation pressure with the Earth’s shadow are computed on a revolution-by-revolution basis, retaining the original osculating Hamiltonian disturbing function. In this framework, we compute the non-singular mean longitude at shadow entry and shadow exit at every orbital revolution in opposition to classical approaches where the singular eccentric anomalies at shadow entry and shadow exit are computed. This new algorithm is developed using non-singular variables. Consequently, it is particularly suitable for both near-circular and near-equatorial orbits as well as orbits which transit periodically around null eccentricities and null inclinations.The algorithm is tested by means of numerical integrations of the equations, averaged over the short periods, including radiation pressure, J₂, the combined Moon and Sun third body attraction as well as the long-term effects of the 1:1 resonance occurring for geosynchronous objects. As an extension of [Valk, S., Lemaître, A., Anselmo, L. Analytical and semi-analytical investigations of geosynchronous space debris with high area-to-mass ratios influenced by solar radiation pressure. Adv. Space Res., doi:10.1016/j.asr.2007.10.025, 2007b], we especially apply our analysis to space debris with area-to-mass as high as 20 m²/kg. This paper provides numerical and semi-analytical investigations leading to a deep understanding of the long-term evolution of the semi-major axis. Finally, these semi-analytical investigations are compared with accurate numerical integrations of the osculating equations of motion over time scales as high as 25 years.