酸性磺酞类染料共振Rayleigh散射光谱法测定奈替米星

用共振Rayleigh散射（RRS）光谱研究了酸性磺酞类染料溴甲酚绿和溴酚蓝分别与奈替米星的相互作用.溴甲酚绿和溴酚蓝在酸性介质中分别与奈替米星相互作用,导致RRS光谱显著增强,最大的RRS峰分别位于606nm和572nm处,散射强度与奈替米星的质量浓度在一定的范围内成正比.此方法具有很高的灵敏度,对于奈替米星的检测限（3σ）分别为30ng/mL和10ng/mL,据此发展了一种测定奈替米星的新方法.     

Determination of station positions and velocities from laser ranging observations to Ajisai,Starlette and Stella satellites

The positions and velocities of the four Satellite Laser Ranging (SLR) stations: Yarragadee (7090), Greenbelt (7105), Graz (7839) and Herstmonceux (7840) from 5-year (2001–2005) SLR data of low orbiting satellites (LEO): Ajisai, Starlette and Stella were determined. The orbits of these satellites were computed from the data provided by 20 SLR stations. All orbital computations were performed by means of NASA Goddard’s GEODYN-II program. The geocentric coordinates were transformed to the topocentric North–South, East–West and Vertical components in reference to ITRF2005. The influence of the number of normal points per orbital arc and the empirical acceleration coefficients on the quality of station coordinates was studied. To get standard deviation of the coordinates determination lower than 1 cm, the number of the normal points per site had to be greater than 50. The computed positions and velocities were compared to those derived from LAGEOS-1/LAGEOS-2 data. Three parameters were used for this comparison: station coordinates stability, differences from ITRF2005 positions and velocities. The stability of coordinates of LEO satellites is significantly worse (17.8 mm) than those of LAGEOS (7.6 mm), the better results are for Ajisai (15.4 mm) than for Starlette/Stella (20.4 mm). The difference in positions between the computed values and ITRF2005 were little bit worse for Starlette/Stella (6.6 mm) than for LAGEOS (4.6 mm), the results for Ajisai were five times worse (29.7 mm) probably due to center of mass correction of this satellite. The station velocities with some exceptions were on the same level (≈1 mm/year) for all satellites. The results presented in this work show that results from Starlette/Stella are better than those from Ajisai for station coordinates determination. We can applied the data from LEO satellites, especially Starlette and Stella for determination of the SLR station coordinates but with two times lower accuracy than when using LAGEOS data.     

Satellite and ground detection of very dense smoke clouds produced on the islands of the Paraná river delta that affected a large region in Central Argentina

Intense fires were produced on the Paraná river delta islands, Argentina, during most part of 2008, by a combination of an exceptionally dry period and the farmers’ use of a fire land-cleaning technique. In April 2008, those fires significantly affected the nearby regions and their inhabitants, from Rosario city to Buenos Aires mega-city. In this work we present satellite as well as ground Aerosol Optical Depth (AOD) at 550 nm data obtained during the propagation of pollution clouds to the central zone of Argentina. The highest value (1.18) was registered at Buenos Aires by atmospheric remote sensing, using the satellite instrument MODIS/Terra on April 18th 2008 at 10:35 local time (= UT − 3 h). On the same day, ground air quality detectors also measured in this city the highest Total Suspended Particle (TSP) value of the month, 2.02 mg/m³. The AOD(550) daily variation at Rosario Astronomical Observatory, which is located near the Paraná riverside, was derived by combining solar ultraviolet erythemal irradiance data (measured with a YES biometre) with model calculations. On April 25th 2008, from 12:00 to 15:30 local time, a rather high and constant AOD(550) value was registered, with a mean value of (0.90 ± 0.21). Cities located on the side of the Rosario–Buenos Aires highway (San Nicolás, Baradero and San Pedro) were also affected, showing a mean AOD(550) between the Rosario and Buenos Aires values. The particulate matter was collected with gridded samplers placed on the Paraná river islands as well as at the Rosario Observatory. They were analysed with a Scanning Electron Microscope (SEM) and mainly showed a biological origin. Even if normally large particles travel small distances from the source, organic aerosol in the range of 40–100 μm and complex asymmetric structures were registered several kilometres away from the aerosol sources on the islands. Another event of intense UV index attenuation (98.6%) occurred on September 18th 2008, due to very dense smoke clouds that extended over the Rosario area for several hours. The clouds were driven away from the fires by East–northeast and East–southeast winds. The minimum value of this index measured around noon allows to derive a maximum AOD(550)_max = (3.65 ± 0.90) at 12:45 local time. Soot clouds extended over the Paraná river, transporting Burned Biomass Debris (BBD) that deposited on Rosario. In particular, burned leaves and small branches with dimensions of 1–20 cm were collected. The mean (BBD) particles deposited on the ground from 7:00 to 19:00 local time were (0.92 ± 0.20) BBD/(m² h).     

机械蝴蝶模型悬停飞行的流动显示实验

为了探索蝴蝶独特的外形及运动模式下蕴含的流动机理，与以往只考虑翅膀气动影响的拍动翼实验不同，我们开发了一种同时考虑身体及翅膀的机械系统用以模拟蝴蝶的悬停飞行，并采用染色液流动显示的方法对升力的主要来源——前缘涡进行了细致的观测。结果显示，在蝴蝶飞行的上下拍动过程中均有前缘涡产生，且不是以往观测到的螺旋或锥状结构，而是近似等直径的柱状联通形式，其明显特征为：在拍动加速阶段存在明显的展向流动，而在减速阶段则会出现破裂；另外，蝴蝶看似杂乱无章的运动实际上是一种自适应控制的结果，有助于提高升力。     

脉冲激光测距误差标定及不确定度分析CSCD

以脉冲激光测距机的测距误差标定为背景,通过对测距误差解析表达式的推导,给出了系统各不确定度分量对测距误差的影响,计算了信号延迟时间、探测器和激光二极管响应时间、晶振频率、大气折射率等不确定度分量。通过对某已标定激光测距机实验验证表明:该装置在500m^20 000m测距范围内,测量重复性引入的相对标准不确定度最大值为0.67m,满足该类激光测距机测量不确定度5m(k=2)的校准测试需求。因此,利用该解析表达式可以实现对脉冲激光测距误差的有效评估,这对于脉冲激光测距测试系统、脉冲激光测距机的设计具有重要的指导意义。     

使用ASIC芯片实现高清视频编码的设计

本文以高清视频编码为切入点,首先介绍了一款高性能的视频编码ASIC芯片FH8735,然后通过对视频编码设备整体框架的设计介绍,引入了视频编码设备的硬件原理设计方案和软件设计方案,硬件设计方案以不同输入视频格式的种类为章节详细叙述了几种常用视频编码的原理设计,软件设计方案从软件架构和软件流程上对视频编码设备软件进行了讨论。可以看出,ASIC芯片以其独有的优势使得视频编码设备设计越来越简单、功能越来越强大、性能越来越可靠。     

一种关于目标与安全管道相对位置估算方法

针对靶场试验安全控制中目标与安全管道位置估算的实际需求,结合靶场实时数据处理要求,提出了利用滑动窗口技术,动态载人理论弹道数据,并采用折半查找和KNN查询相结合的思想实现了目标与理论弹道最近邻点查询,完成了飞行目标与理论规划航迹间的位置等参数偏差查询。利用区间估计原理,给出了目标与安全管道相对位置估算方法,解决了传统试验中无法对目标与管道边界的接近程度进行量化的问题。     

星间链路在空间态势感知中的应用研究

通过对星间链路和空间态势感知系统国内外发展现状的分析,指出星间链路在空间信息有效获取、安全传输和实时应用以及保障空间态势感知系统战场生存能力等方面起着重要的作用.针对星间链路在未来空间态势感知系统中的应用需求,提出包含空间通信模型和空间导航模型在内的空间感知体系基本架构,并对该架构下星间链路的设计要求或者特点进行分析,指出星间链路应该具有灵活可变的星间路由策略和联网结构,并能够支持高速可变和安全可靠的星间数据传输.分别从空间网络和卫星节点2个层面提出了系统实现的关键技术,并给出部分关键技术的研究重点和研究方法.上述研究结果可以为星间链路及相关领域的研究工作提供一定的借鉴和帮助.     

基于概率统计的DS/FH系统干扰检测算法

基于时频分布的干扰检测算法是DS/FH（Direct Sequence/Frequency Hopping,直接序列扩频/跳频扩频）系统干扰检测的传统手段,针对其运算量大、实时性差,以及无法检测某些特殊干扰信号等问题,提出一种基于概率统计的干扰检测算法.通过统计DS/FH系统频谱图中各频率的幅值出现位置,以DS/FH信号与干扰信号频谱分布规律的差别为判决依据,完成DS/FH系统中干扰信号的检测.分析和仿真结果表明：该检测算法能够有效识别DS/FH系统中的典型干扰信号,与传统基于时频分布的检测算法相比,能够实现某些特殊干扰信号的有效检测;同时,由于该算法不需要进行复杂的时频联合分析,其运算复杂度大大降低,能够实现DS/FH系统干扰信号的快速检测.     

中国深空网首次△DOR联合测轨试验分析

通过分析中国深空网首次△DOR（Delta Differential One way Ranging,双差分单向测距）联合测轨试验的干涉测量事后数据,重点从观测量随机精度、闭合时延等方面讨论了国内深空网与国内VLBI（Very Long Baseline Interferometry,甚长基线干涉测量）观测网、国内深空网与国际深空网的联合干涉处理情况,并与ESOC（European Space Operation Center,欧洲空间操作中心）数据处理结果进行了比对.试验结果表明：我国深空网已具备独立或联合开展深空探测器导航测轨的系统支持能力;深空站系统具备高速率数据接收、采集、记录、传输能力,采集数据处理精度优于1 ns;深空网干涉测量信号处理中心具备多体制信号的干涉处理分析能力,其分析精度与ESOC处理精度差异在0.1 ns量级.