星载相控阵GNSS-R测高系统设计与实验

星载GNSS-R测高系统采用多波束相控阵天线和干涉互相关处理方式,接收北斗导航卫星和GPS导航卫星发射的L波段导航直射信号与海面反射信号,进行海面高度探测。详细介绍GNSS-R测高系统设计与实现、集成和外场试验等,外场试验不仅验证了相控阵GNSS-R测高系统功能,更重要的是验证了核心软件算法的正确性。GNSS-R测高系统适用于中尺度海洋现象的观测,可在时间和空间尺度上扩展雷达高度计的观测能力,并与之相互补充,有利于对复杂海面的中尺度结构进行较高时间分辨率的观测。GNSS-R测高仪为星载高精度海面高度探测提供了新型载荷。     

关于飞机结冰的多重安全边界问题

边界保护是保障飞机安全性的重要方面,对目前国内外飞机结冰安全边界问题的研究现状及进展进行了综述,对飞机结冰致灾物理链路的影响因素及规律进行了分析,指出目前从飞行力学角度出发的安全边界尚未全面考虑飞机结冰致灾复杂物理现象的相关因素,并提出了飞机结冰多重安全边界的概念,将飞机结冰的安全边界分为气象边界、冰形边界和飞行安全边界。结合相应的物理规律和实际应用,按照飞机结冰导致性能恶化的影响程度、飞行操纵影响程度等对边界又进行了多重属性划分。进一步梳理了多重安全边界研究需解决的主要关键问题,提出了下一步的相关研究方向,可为飞机设计、适航认证、飞行操纵、航路规划、分级优化保护等方面的应用提供支撑和参考。     

飞机结冰热力学行为研究综述

热力学现象是制约飞机结冰特性的重要现象之一。开展飞机结冰过程热力学行为的研究旨在深入把握结冰过程的规律特征,从而为建立科学有效的结冰防护手段、保障结冰条件下的飞行安全奠定基础。本文回顾和介绍了飞机结冰热力学研究所涉及的过冷水滴存在的物理机制、结冰热力学条件、形核与晶体生长、耦合液/固相变的复合传热传质特性,以及热力学效应作用下的结冰物理特性等相关领域的研究进展及发展现状,并基于国外相关研究的发展趋势,提出了中国未来飞机结冰热力学研究需重点关注的方向。     

基于实测数据的海杂波时空相关性分析

海杂波的相关特性分为时间相关性和空间相关性,二者均与雷达系统参数、环境条件等多种因素有关。文章利用X波段雷达实测海杂波数据,重点研究了不同极化条件下海杂波的时间相关性、高低典型海况和不同入射余角条件下的海杂波距离向和方位向空间相关性。经大量实测数据验证表明,极化方式对海杂波强时间相关性影响较小,海杂波距离向空间相关性受海况影响较大、方位向相邻分辨单元空间相关性较弱,这些结论对于海杂波中目标检测方法优化设计具有重要意义。     

The effect of geocenter motion on Jason-2 orbits and the mean sea level

We compute a series of Jason-2 GPS and SLR/DORIS-based orbits using ITRF2005 and the std0905 standards ( Lemoine et al., 2010). Our GPS and SLR/DORIS orbit data sets span a period of 2 years from cycle 3 (July 2008) to cycle 74 (July 2010). We extract the Jason-2 orbit frame translational parameters per cycle by the means of a Helmert transformation between a set of reference orbits and a set of test orbits. We compare the annual terms of these time-series to the annual terms of two different geocenter motion models where biases and trends have been removed. Subsequently, we include the annual terms of the modeled geocenter motion as a degree-1 loading displacement correction to the GPS and SLR/DORIS tracking network of the POD process. Although the annual geocenter motion correction would reflect a stationary signal in time, under ideal conditions, the whole geocenter motion is a non-stationary process that includes secular trends. Our results suggest that our GSFC Jason-2 GPS-based orbits are closely tied to the center of mass (CM) of the Earth consistent with our current force modeling, whereas GSFC’s SLR/DORIS-based orbits are tied to the origin of ITRF2005, which is the center of figure (CF) for sub-secular scales. We quantify the GPS and SLR/DORIS orbit centering and how this impacts the orbit radial error over the globe, which is assimilated into mean sea level (MSL) error, from the omission of the annual term of the geocenter correction. We find that for the SLR/DORIS std0905 orbits, currently used by the oceanographic community, only the negligence of the annual term of the geocenter motion correction results in a – 4.67 ± 3.40 mm error in the Z-component of the orbit frame which creates 1.06 ± 2.66 mm of systematic error in the MSL estimates, mainly due to the uneven distribution of the oceans between the North and South hemisphere.     

Radar Imaging of Mercury

Earth-based radar has been one of the few, and one of the most important, sources of new information about Mercury during the three decades since the Mariner 10 encounters. The emphasis during the past 15 years has been on full-disk, dual-polarization imaging of the planet, an effort that has been facilitated by the development of novel radar techniques and by improvements in radar systems. Probably the most important result of the imaging work has been the discovery and mapping of radar-bright features at the poles. The radar scattering properties of these features, and their confinement to permanently shaded crater floors, is consistent with volume backscatter from a low-loss volatile such as clean water ice. Questions remain, however, regarding the source and long-term stability of the putative ice, which underscores the need for independent confirmation by other observational methods. Radar images of the non-polar regions have also revealed a plethora of bright features, most of which are associated with fresh craters and their ejecta. Several very large impact features, with rays and other bright ejecta spreading over distances of 1,000 km or more, have been traced to source craters with diameters of 80–125 km. Among these large rayed features are some whose relative faintness suggests that they are being observed in an intermediate stage of degradation. Less extended ray/ejecta features have been found for some of the freshest medium-size craters such as Kuiper and Degas. Much more common are smaller (<40 km diameter) fresh craters showing bright rim-rings but little or no ray structure. These smaller radar-bright craters are particularly common over the H-7 quadrangle. Diffuse areas of enhanced depolarized brightness have been found in the smooth plains, including the circum-Caloris planitiae and Tolstoj Basin. This is an interesting finding, as it is the reverse of the albedo contrast seen between the radar-dark maria and the radar-bright cratered highlands on the Moon.     

用低纯原料制备电冰箱起动器PTCR的重要途经——热敏钛酸钡陶瓷第二相结晶

根据Al_2O_3-SiO_2系统相图,调整Al_2O_3,SiO_2添加剂比例,可在热敏钛酸钡陶瓷显微结构中形成莫来石结晶相,莫来石的形成改善了用国产低纯原料制备电冰箱起动器PTCR的性能。本文就莫来石第二相与PTCR性能关系进行了讨论。     

基于蒙特卡洛方法的冰晶撞击特性计算

航空发动机摄入冰晶易发生内部结冰、造成发动机推力损失,严重时引发航空事故。冰晶结冰数值模拟是研究冰晶结冰的重要手段,而撞击收集系数计算是冰晶结冰数值模拟的关键环节。基于NNWICE平台开展冰晶结冰前期的阻力系数、运动轨迹和撞击收集系数的数值模拟与计算研究,实现了基于蒙特卡洛方法的冰晶撞击收集系数的准确计算;在此基础上发展了拉格朗日框架下冰晶粒子运动、传热传质耦合数值计算方法;通过完成二维NACA0012翼型的相关算例,对比分析了不同阻力模型和冰晶相变对撞击收集系数的影响。结果表明阻力模型对冰晶撞击收集系数影响较小,冰晶相变过程会对冰晶运动轨迹及撞击收集系数产生显著影响,为进一步发展冰晶结冰数值模拟计算方法奠定了基础。     

面向过冷大水滴适航验证的结冰探测技术研究

过冷大水滴（Supercooled large droplet,SLD）结冰超出了常规防除冰系统的防护范围,是一种更为严重的结冰情形,极大地影响着飞行安全。在美国联邦航空管理局14 CFR 25.140条款中明确提到为保证飞机在SLD结冰条件下的安全运行,首先且必须要对SLD结冰气象环境进行探测。由于水滴破碎会改变水滴运动轨迹和表面撞击水分布,使水滴撞击极限变小,而水滴飞溅对结冰极限位置影响不大,因此本文通过研究大、小粒径水滴在飞机上收集范围不同的特点,提出一种可以满足SLD结冰适航符合性的结冰探测技术。该结冰探测技术采用常规结冰探测器,根据水滴收集范围将其布置于不同敏感结冰部位,可以实现全剖面飞行的结冰环境探测。     

飞机机翼积冰研究方法和进展分析

通过对目前国内外研究飞机机翼积冰三种方法的分析,指出了它们各自优缺点,重点介绍了现行国内外研究的进展和新趋势,提出了研究方法的改进方案和进一步研究的建议。