基于FPGA的北斗B1频点接收机 基带信号处理器设计

针对北斗二代B1频点信号比特翻转频繁的问题,设计并实现了基于FPGA的北斗B1频点导航接收机基带处理器.该处理器在信号捕获过程中设计了频率精细搜索的精捕获算法,避免了假捕获并且提高了捕获频率的精度;在载波跟踪环路中设计2阶锁频环辅助3阶锁相环的方案,以提高环路跟踪的动态性能.其中,锁频环和锁相环均设计了对比特翻转敏感的鉴别器,保证环路跟踪的准确性.试验结果表明,该基带处理器设计具有较高精度的捕获频率和良好的高动态跟踪能力.     

Microstructure evolution of a hypereutectic Nb–Ti–Si–Cr–Al–Hf alloy processed by directional solidification

In this work, the Nb–14Si–24Ti–10Cr–2Al–2Hf–0.1Y alloy(at.%) was processed by the liquid–metal-cooled directional solidification(DS) at 1750 C with withdrawal rates of 1.2, 6,18 mm/min and post heat treatment(HT) at 1450 C for 10 h. The microstructures of the directionally solidified and heat treated samples were investigated. The results show that the microstructure of directionally solidified alloy mainly consists of petaloid Nbss+ Nb5Si3eutectics and Ti-rich Nbss+ Nb5Si3+ Cr2Nb eutectics. With the increase of withdrawal rate, the primary Nb5Si3is eliminated, Nbss+ Nb5Si3eutectic cells turn round and connected with the microstructure refinement and Nbss+ Nb5Si3+ Cr2Nb eutectics turn to a river-like morphology. After heat treatment,Nbss+ Nb5Si3+ Cr2Nb eutectics disappeared and petaloid Nbss+ Nb5Si3eutectics turn to a specific fiber-mesh structure gradually, which is promoted by higher withdrawal rates. Furthermore,both the volume fraction of Cr2Nb and the content of Cr in Nbssof Nbss+ Nb5Si3eutectics change regularly with the increase of withdrawal rate and heat treatment at 1450 C for 10 h.     

正交设计在沉淀硬化不锈钢热处理研究中的应用

用正交设计法研究固溶温度、固溶时间、调整处理温度和调整处理时间对0Cr17Ni5Mo3沉淀硬化不锈钢力学性能的影响.研究结果表明,在沉淀硬化不锈钢热处理研究中采用正交设计法安排试验,可以用很少的试验量获得主要热处理工艺参数对力学性能影响的规律.     

转子—机匣系统碰摩故障特征试验研究

以转子-机匣模型试验器为对象,试验模拟航空发动机试车过程中所遇到的典型碰摩故障现象,研究分析其碰摩类型及相应的振动特性,总结并建立包括转子、支承、机匣共同影响在内的旋转机械转、静件碰摩故障特征谱。     

激光熔化沉积15-5PH沉淀硬化不锈钢组织及拉伸性能

利用激光熔化沉积技术制备15-5PH沉淀硬化不锈钢板,利用金相显微镜(OM)、扫描电镜(SEM)、透射电镜(TEM)、电子探针(EPMA)技术,对沉积态组织进行分析,测试沉积态组织的室温拉伸性能。结果表明:激光熔化沉积15-5PH不锈钢沉积态组织由沿沉积增高方向贯穿多层外延生长的柱状晶组成,柱状晶内包含多个细长整齐排列的胞状树枝晶,枝晶内为马氏体组织,枝晶间为铁素体;沉积态组织中弥散分布大量细小的NbC析出相,尺寸12～20 nm;15-5PH不锈钢沉积态组织具有良好的力学性能,纵向抗拉强度和延伸率分别为1 128.5 MPa和14.0%,横向抗拉强度和延伸率分别为1 101 MPa和12.25%。     

GJB5000 A与DO-178 B／C的综合应用研究

针对软件研制单位目前存在的型号软件研制必须同时满足GJB5000 A与适航软件研制标准的要求,通过对GJB5000 A与DO-178 B／C的对比分析,提出一种将GJB5000 A与DO-178 B／C相互融合的方法,并对方法实际工程实践时应注意的问题进行了说明。     

基于ArcGIS的公路沿线三维地形的建立和应用分析

以勉宁高速公路为例,在1：2000的公路沿线地形平面图的基础上,利用AutoCAD和R2V软件对其进行预处理,然后在ArcGIS中建立高精度的DEM,通过DEM和公路沿线平面图的叠加,生成公路沿线单个三维地形,建立Oracle数据库存储二维和三维地形数据,并对其中三维数据进行了缓冲区、面积和体积计算等三维应用分析。     

X-ray study of accretion flow in narrow-line Seyfert 1 galaxies

We present the results of a systematic study of narrow-line Seyfert 1 galaxies (NLS1s) observed with XMM-Newton. The 2–12 keV X-ray spectra of NLS1s are well represented by a single power law with a photon index Γ ∼ 2. When this hard power law continuum is extrapolated into the low energy band, we found that all objects in our sample show prominent soft excess emission. This excess emission is well parameterized by the thermal emission expected from an optically thick accretion disk, and we found the following three peculiar features: (1) The derived disk temperatures are significantly higher than the expectation from a standard Shakura-Sunyaev accretion disk, if we assume a central mass of a black hole to be 10^6–8M_⊙. (2) The temperatures are distributed within narrow range (ΔkT ∼ 0.08 keV) with an average temperature of 0.18 keV in spite of the range of four orders of magnitude in luminosity (10^41–45 erg s⁻¹). (3) We found a peculiar temperature–luminosity relation, where the luminosity seems to be almost saturated in spite of the significant change in temperature, during the observations of the most luminous NLS1 PKS 0558-504. These results strongly suggest that the standard accretion disk picture is no longer appropriate in the nuclei of NLS1s. We discuss a possible origin for the soft excess component, and suggest that a slim disk may be able to explain the observational results, if the photon trapping effect is properly taken into account.