γ暴内激波的速度变化

对γ暴GRB960113的高能段与低能段的时间延迟和脉冲宽度进行了分析，结果表明，其随时间有规律地增加和展宽．γ暴的内激波模型可对此现象作出合理的解释。     

硅液相外延生长的晶向自动偏离现象

通过对液相外延的薄膜Ｘ衍射测试，结果显示不论衬底是否偏离［１１１］晶向，外延层在同一衍射位置都出现了双峰。经比较分析，确认了硅（１１１）面在液相外延生长时存在晶向自动偏转现象。     

基于红外视频的火灾探测算法

视频火灾探测技术成为火灾探测的主要研究方向之一,该技术的难点是保证对火灾准确快速地探测。针对目前视频火灾探测识别率较低、报警时间较长的问题,为了提高火灾识别率,增强算法实时性,本文提出一种红外视频的火灾火焰探测方法,采用带有截止可见光透红外滤波片的摄像头采集现场红外影像,结合火焰的静态和动态特征,对火灾进行准确快速探测,同时,综合运用火焰圆形度和尖角个数变化判据对稳定火焰和非稳定火焰进行区别,实现对火灾的分级报警。实验结果表明,改进算法对火焰识别的准确性高,抗干扰能力较强,并且具有显著的快速性,其处理速度达到20ms/帧,并且系统平均报警时间小于200ms。     

短波射线追踪技术中的电离层混合建模方法

在国际参考电离层模型和多层准抛物模型的基础上,提出了一种混合应用两种模型进行电离层建模的新方法.利用射线追踪技术,分别对混合模型和传统国际参考电离层模型下短波射线在电离层中的轨迹进行了仿真,得到了电波群路径.通过与实测电波群路径的对比,结果表明:对中国中纬度地区在电离层混合模型下的射线追踪精度优于传统国际参考电离层模型下的射线追踪精度,同时混合建模方法降低了多层准抛物模型对输入条件的要求,扩展了多层准抛物模型在射线追踪技术中的应用范围.     

Dark Matter Particle Explorer:The First Chinese Cosmic Ray and Hard γ-ray Detector in Space

The Dark Matter Particle Explorer (DAMPE) mission is one of the five scientific space science missions within the framework of the Strategic Pioneer Program on Space Science of the Chinese Academy of Science (CAS) approved in 2011. The main scientific objective of DAMPE is to detect electrons and photons in the range of 5GeV-10TeV with unprecedented energy resolution (1.5% at 100GeV) in order to identify possible Dark Matter (DM) signatures. It will also measure the flux of nuclei up to above 500TeV with excellent energy resolution (40% at 800GeV), which will bring new insights to the origin and propagation high energy cosmic rays. With its excellent photon detection capability, the DAMPE mission is well placed for new discoveries in high energy-ray astronomy as well.      

现场校准试验用便携式γ射线照射装置研制

固定式环境γ辐射剂量率监测仪表是承担环境连续监测任务的主要设备,这类仪表通常不便于拆卸和安装,而且送检周期较长（一周左右）,影响了连续监测点数据的连续性。为了固定式仪表的按期校准,结合蒙卡方法研制了便携式γ射线照射装置,利用PTW剂量计对辐射场进行标定,最后利用便携式照射装置对固定式环境γ辐射剂量率监测仪表进行现场校准实验。     

Lunar cosmic ray radiation environments during Luna and Lunar Reconnaissance Orbiter missions

The RV-2N-series instruments onboard Luna missions and the Cosmic Ray Telescope for the Effects of Radiation (CRaTER) instrument onboard Lunar Reconnaissance Orbiter (LRO) were designed to characterize the global lunar radiation environment and its biological impacts by measuring cosmic ray (CR) intensity. In this study, we have shown that the RV-2N-series instruments onboard of Russian Luna missions and the CRaTER reliably detect both background CRs and solar proton events (SPEs) in the lunar radiation environment using the proton intensity measured by the RV-2N-series onboard Luna missions out of the Russian Luna program for the exploration of the Moon (November 1970–August 1975) and the CR intensity on the Moon observed by the CRaTER (June 2009–March 2011). Those were compared with the CR intensities observed by neutron monitors (McMurdo, Thule, Oulu) on the Earth. The sunspot number is used as the index of solar activity (NOAA National Geophysical Data Center). As a result, the background CR intensities on the Moon turned out to have a good anti-correlation with the solar activity. We have also identified the proton intensity increasing events on the Moon which have the similar profiles to those observed by neutron monitors on the Earth. Most of these events show the significant increase of proton intensities in the lunar radiation environment when the SPEs associated with solar eruptions are verified. Therefore, most of the proton intensity increasing events are associated with the energetic solar particles in the lunar environment.     

脉冲星导航试验卫星科学观测数据分析

脉冲星导航试验卫星是我国发射的一颗专用试验卫星.经过4个多月的在轨观测,该卫星已成功获取了大量观测数据.介绍利用该卫星搭载的掠入射聚焦型X射线探测器在近4个月中对PSR B0531+21获得的观测数据第一批处理结果.本文详细阐述掠入射聚焦型X射线探测器的观测模式,给出脉冲星观测数据的处理方法以及脉冲星参数的拟合过程,利用基于第一手观测数据的脉冲星精化参数验证掠入射聚焦型探测器在轨工作性能,得以回答使用国产X射线探测器是否能够“看得见”脉冲星问题.     

后台阶流动的Hybrid RANS/LES模拟

采用雷诺平均的Navier-Stokes和大涡模拟混合的方法对后台阶流动进行了数值模拟,并与实验结果进行了对比;分区尺度采用IDDES(Improved Delayed Detached Eddy Simulation)模式:来流包含背景湍流度时,混合方法转化为WMLES(Wall Modeling in LES)模拟,除了近壁区外的大部分区域都是直接求解;不包含来流湍流度时,转化为DDES(Delayed Detached Eddy Simulation)模式,附面层采用纯RANS模拟,大分离流动区用类脱体涡模拟方法模拟;对流通量的离散采用迎风型低耗散通量分裂格式和中心型四阶偏斜对称格式组合的模式;湍流模型采用Spalart-Allmaras(S-A)模型;亚格子长度尺度取决于网格分布和到壁面的距离.      

嵌入式处理器P2020机器码程序到C语言源程序的溯源方法

处理器PowerPC P2020在航空航天等嵌入式领域被广泛应用,以RTCA/DO-178C中A级软件的适航要求作为研究的出发点,提出了从文件、函数声明、函数体代码3层次实现P2020机器码程序到C源程序的溯源方法。在获取C语言源程序与PowerPC P2020机器码程序文件名列表的基础上,实现PowerPC P2020机器码文件主名的溯源;通过遍历C源程序抽象语法树和PowerPC P2020机器码获取函数名列表,实现PowerPC P2020机器码函数声明的溯源;通过定义C语言程序抽象语法树节点生成期望汇编指令序列的规则,实现PowerPC P2020机器码函数体的溯源。通过设计245个C源程序文件与345个PowerPC P2020机器码程序文件,1 111个C语言函数声明与1 273个PowerPC P2020机器码函数声明,以及覆盖C语言程序23类语法结构的460个测试用例,验证了PowerPC P2020机器码程序到C源程序的自动化溯源方法的有效性。结果表明：文件溯源和函数声明溯源的追溯匹配率达100%,程序函数体代码的平均溯源匹配率达97.22%。溯源匹配结果可以检查PowerPC P2020机器码程序是否在编译过程插入例外异常代码,以防止其带来的安全隐患,保证航空航天嵌入式安全关键软件机器码的安全性和可靠性。