人工增雨防雹火箭弹道跟踪系统的研制及初步试验

由于受到高空风场的影响,人工增雨防雹火箭真实的弹道轨迹和射程与理论弹道值具有不一致性。为增强实施增雨防雹作业的科学性、精准性及其作业效果评估准确性,研制了一套人工增雨防雹火箭播撒作业跟踪系统。该系统分为火箭定位系统和数据传输系统两部分,利用卫星定位模块加上数据传输电台模式将火箭飞行轨迹实时传输至地面。并开展了一次人工增雨防雹火箭弹道跟踪实弹发射试验,发射两发人工增雨防雹测试火箭,除初始阶段4～5 s卫星定位失锁而没有数据外,其余时间所有数据均接收完整。结合高空风场数据对人工增雨防雹测试火箭进行风偏修正后的实际弹道更接近于理论弹道,风偏修正意义明显,有利于增雨防雹火箭精准作业。     

The H.E.S.S. central data acquisition system

The High Energy Stereoscopic System (H.E.S.S.) is a system of Imaging Atmospheric Cherenkov Telescopes (IACTs) located in the Khomas Highland in Namibia. It measures cosmic gamma rays of very high energies (VHE; >100 GeV) using the Earth’s atmosphere as a calorimeter. The H.E.S.S. Array entered Phase II in September 2012 with the inauguration of a fifth telescope that is larger and more complex than the other four. This paper will give an overview of the current H.E.S.S. central data acquisition (DAQ) system with particular emphasis on the upgrades made to integrate the fifth telescope into the array. At first, the various requirements for the central DAQ are discussed then the general design principles employed to fulfil these requirements are described. Finally, the performance, stability and reliability of the H.E.S.S. central DAQ are presented. One of the major accomplishments is that less than 0.8% of observation time has been lost due to central DAQ problems since 2009.     

Atmospheric entry profiles from the Mars Exploration Rovers Spirit and Opportunity

Accelerometer measurements made by Spirit and Opportunity during their entries through the martian atmosphere are reported. Vertical profiles of atmospheric density, pressure, and temperature with sub-km vertical resolution were obtained using these data between 10 and 100 km. Spirit's temperature profile is ∼10 K warmer than Opportunity's between 20 and 80 km. Unlike all other martian entry profiles, Spirit's temperature profile does not contain any large amplitude, long wavelength oscillations and is nearly isothermal below 30 km. Opportunity's temperature profile contains a strong inversion between 8 and 12 km. A moderate dust storm, which occurred on Mars shortly before these two atmospheric entries, may account for some of the differences between the two profiles. The poorly known angle of attack and unknown wind velocity may cause the temperature profiles to contain errors of tens of Kelvin at 10 km, but these errors would be an order of magnitude smaller above 30 km. On broad scales, the two profiles are consistent with Mars Global Surveyor Thermal Emission Spectrometer (TES) pressure/temperature profiles. Differences exist on smaller scales, particularly associated with the near-isothermal portion of Spirit's profile and the temperature inversion in Opportunity's profile.     

水资源优化配置决策支持系统中的软件集成方法

根据水资源优化配置决策支持系统的开发实践，分析了多平台软件的集成问题，给出了多平台软件集成中用户数据及控制信息的相互传递方法。     

水流冲刷沉积物生成泥石流的条件及运动规律的试验研究

在铺满卵石的陡槽上释放不同浓度、不同流量的泥浆或清水，观测卵石在泥浆流作用下的运动，研究泥石流的形成条件和运动规律。试验结果表明，当K（=rqJ）大于某临界值K_c时就会发生泥石流，但这个临界值K_c随波相泥浆浓度而变。泥石流龙头由大卵石组成，在不断摩擦和碰撞中翻滚着推进，消耗大量动能，同时控制着后续流不离散。后续流液相流速显著大于龙头，不断把能量输送到龙头，维持龙头运动。大卵石在运动中受到液相流的推动力较大，而受到的碰撞阻力较小，比龙头运动的快。因而大卵石逐渐集中于龙头。     

空间太阳望远镜高速数据传输系统

“空间太阳望远镜”是中国的一项非常重要的天文卫星计划。卫星上将搭载 5个有效载荷 ,在可见光、远紫外、硬X射线、软X射线、Hα和射电波段同时观测太阳 ,其中的主光学望远镜口径达 1m。各有效载荷的CCD器件和其它敏感器件每天采集的科学数据量经过预处理后达 50Gbytes,再由数据压缩系统压缩至 8Gbytes,并储存在海量存储器中。如此庞大的数据量要求空间太阳望远镜的科学数据传输系统以高达 60Mbps的码速率向地面站传送。本文所有的工作均围绕着空间太阳望远镜高速数据传输系统展开 :1 .根据空间太阳望远镜的需求 ,综合研究、分析了它的科学数据传输系统的性能指标和特点 ,并作总体的方案设计 ;2 .设计开发了科学数据传输系统的信道编码和信道解码单元。信道编码单元将把海量存储器中的数据转换为适于QPSK射频调制格式化的串行数据流 ,信道解码单元实现相反的过程 ,文中详细给出了信道编码系统的原理、方法和实验结果。设计中引入了新的设计思想和方法 ,通信协议与现有地面站兼容 ;3 .完成了信道编码、解码环路的地面试验 ,结果表明信道编码、解码系统的技术指标完全符合空间太阳望远镜的要求。在理想无噪声条件下 ,闭环试验数据传输结果无误码 ,数据传输率达 60Mbps,是目前国内科学数据传输系统码速率     

一种无线数据传输接口及控制装置

本文介绍一种无线数据传接口及控制装置。装置中采用计算机软件实现串—并、并—串变换及频率调制、其硬件成本低廉,工作可靠,可用于速率为50、300、600或1200bps的数传通信。     

SOFTWARE REVIEWS

software reviews are in this article BMDP/PC CONCEPTS COMPUTERIZED ATLAS EVALUATION OF ALTERNATE PROPOSALS (EAP) EXTRA: EXPRESS TRANSIT ANALYSIS MATC CAD MOTORS TRANSPORTATION PACKAGE PCMAP: Thematic Mapping Software for the IBM Personal Computer, Version 2.3 PLACE TRANPLAN . US-ATLAS     

针对MODIS数据的大气水汽含量反演及31和32波段透过率计算

 针对MODIS的波段特征,首先,用近红外波段反演大气水汽含量; 然后,通过LOWTRAN模拟大气水汽含量与MODIS 31和32热红 外波段透过率的统计关系; 最后,计算31和32波段的透过率。该方法克服了以往一景图像只用1个透过率的局限性,使得透过率的求 算精确到每1个像元,同时保证参数获取的实时性。     

Methodological Development of the Conditional Sampling Method. Part II: Quality Control Criteria of Relaxed Eddy Accumulation Flux Measurements

Determination of biosphere–atmosphere exchanges requires accurate quantification of the turbulent fluxes of energy and of a wide variety of trace gases. Relaxed Eddy Accumulation (REA) is a method that has received increasing attention in recent years, because it does not require any rapid sensor for the scalar measurements as the Eddy Correlation method (EC) does. As in all micrometeorological studies, REA measurements in the atmospheric surface layer are valid under some restrictive conditions so as to be representative of a specific ecosystem. These conditions are the homogeneity of the underlying surface, stationary and horizontally homogeneous turbulence. For most experiments these conditions are not fully satisfied. Data uncertainties can also be related to not fulfilling the method principles or to the technical characteristics of the REA system itself. In order to assess REA measurement quality, a methodological approach of data analysis is developed in this study. This methodological analysis is based on the establishment of criteria for data quality control. A set of them, deduced from the mean and turbulent flow, are called ‘Dynamic criteria’ and are designated to control the stationarity and homogeneity of the w function and the validation of Taylor’s hypothesis. A second set (‘REA operational criteria’) is designed to check the sampling process and, more precisely, the homogeneity of the negative and positive selection process throughout the sampling period. A third set of criteria (‘Chemical scalar criteria’) concerns the scalar measurements. Results of the criteria application to data measured at two different experimental sites are also presented. Cut-off limits of criteria are defined based on their statistical distribution and shown to be specific for each site. Strictness of each criterion, defined by the percentage of flagged samples, is analysed in conjunction with the meteorological conditions and atmospheric stability. It is found that flagged samples mainly correspond to neutral and stable nocturnal conditions. During daytime, nearly free convection conditions can also yield poor quality data.