基于F2812的多处理器串行加载系统设计

阐述了一种基于F2812的多处理器串行加载系统,对加栽系统的工作原理和软件设计进行了详细介绍。系统可实现系统集成环境下多处理器软件代码的在线编程。经过大量测试和环境试验考核,串行加载系统工作稳定可靠。     

不同机翼优化构型的轻质F4模型气动特性实验研究

采用光固化快速成型技术（SL）加工基于气动/结构耦合分析的六套不同机翼优化构型的轻质F4模型,在0.6m跨超声速风洞完成了马赫数0.6-0.85范围内的气动力测量试验。试验结果表明,采用气动/结构耦合优化设计的代号为6#的轻质F4模型升力特性与国外结果较接近,与机翼三维变形的事实吻合,验证了采用的气动/结构耦合优化设计方法基本可行,为探索模型静气动弹性风洞试验数据修正方法提供了参考。     

热处理状态对LD10 铝合金化铣表面质量的影响

为了解决运载火箭结构中口盖零件化铣后表面质量较差的问题,对LD10 铝合金板材的化铣加

工进行了试验研究。采取同批次、相同变形量、不同热处理状态(淬火+人工时效、淬火+过时效)的零件在相同

的化铣工艺参数下进行试验,并对零件的化学成分、金相组织进行了分析。理论研究及试验结果表明:LD10 铝

合金的化铣表面质量与加工前热处理状态有关,退火状态及淬火+人工时效状态的零件化铣后表面质量较好,

在不影响力学性能的前提下,可采用过时效处理提高化铣表面质量。

     

一种手自一体石英挠性加速度计温控仪的设计

为满足惯性导航系统中石英挠性加速度计精确测试要求,设计了一种以模拟电路和功率放大为核心的高精度加速度计温度控制仪器,温控精度达到0.02℃.该温控仪除具有精密温度控制外,还具有手动模拟量测量、自动模拟量测量及多通道I/F输出测试于一体的特点.为满足多只加速度计测试一致性要求,采用单一温度受控的采样电阻方法,提高了石英挠性加速度计性能指标如4小时稳定性、模拟量长期重复性测试的准确性和稳定性.     

LD10铝合金不均匀焊接接头的拉伸性能研究

针对5.5 mm厚LD1ocs铝合金进行单面两层TIG焊工艺试验,分析了接头的力学性能不均匀性,并采用abaqus有限元分析软件模拟研究了该力学性能不均匀接头的拉伸断裂行为,结果表明:接头过时效区的变形能力强,有助于提高接头塑性;过时效区的软化程度和宽度对接头拉伸性能有重要影响,宽度增大、软化程度在一定范围内增加,会略微降低接头拉伸强度、但使延伸率增大,另外保留焊缝余高,明显地提高了接头的抗拉强度和延伸率.     

F119发动机总体性能特点分析与评估

根据航空发动机总体性能设计的一般规律,对不同的资料数据进行筛选,初步选定了F119发动机相对准确的总体及部件性能参数,并以此为参照基准进行了F119发动机设计点、起飞点和超声速巡航点的总体性能计算,评估了F119发动机在这三个典型状态点的性能,概要地梳理了F119发动机的总体性能设计理念。     

计算机辅助FMECA与FTA正向 综合分析方法研究

FMECA(Failure Mode Effect and Criticality Analysis)和FTA(Fault Tree Analysis)是分析系统故障因果关系的两种常用技术.大量工程实践表明,它们在用于系统安全性、可靠性分析时取得了显著的效益.这两种技术分别独立应用时,既有各自的优点,也存在着一定的缺陷和不足,为此综合了FMECA与FTA的优点,阐述了复杂动态系统FMECA与FTA综合的思路,着重阐述了由计算机辅助FMECA向FTA正向综合建立故障子树的推理算法,通过三余度舵机系统的应用,证明该方法效果良好.     

国外10MW风力机叶片气动布局研究

降低风能利用成本是风力机单机装机功率向大型化发展的主要驱动力,10MW风力机已成为当今国外大型风力机研发的目标。本文简要回顾了风力机叶片空气动力研究对风力机大型化发展的贡献,探讨国外针对10MW风力机开展的新型叶片气动布局研究。     

A regional model for the prediction of M(3000)F2 over East Asia

Research on empirical or physical models of ionospheric parameters is one of the important topics in the field of space weather and communication support services. To improve the accuracy of predicting the monthly median ionospheric propagating factor at 3000 km of the F2 layer (identified as M(3000)F2) for high frequency radio wave propagation, a model based on modified orthogonal temporal–spatial functions is proposed. The proposed model has three new characteristics: (1) The solar activity parameters of sunspot number and the 10.7-cm solar radio flux are together introduced into temporal reconstruction. (2) Both the geomagnetic dip and its modified value are chosen as features of the geographical spatial variation for spatial reconstruction. (3) A series of harmonic functions are used to represent the M(3000)F2, which reflects seasonal and solar cycle variations. The proposed model is established by combining nonlinear regression for three characteristics with harmonic analysis by using vertical sounding data over East Asia. Statistical results reveal that M(3000)F2 calculated by the proposed model is consistent with the trend of the monthly median observations. The proposed model is better than the International Reference Ionosphere (IRI) model by comparison between predictions and observations of six station, which illustrates that the proposed model outperforms the IRI model over East Asia. The proposed method can be further expanded for potentially providing more accurate predictions for other ionospheric parameters on the global scale.     

Solar activity variations of equatorial spread F occurrence and sustenance during different seasons over Indian longitudes: Empirical model and causative mechanisms

A comprehensive analysis using nearly two decades of ionosonde data is carried out on the seasonal and solar cycle variations of Equatorial Spread F (ESF) irregularities over magnetic equatorial location Trivandrum (8.5°N, 77°E). The corresponding Rayleigh Taylor (RT) instability growth rates (γ) are also estimated. A seasonal pattern of ESF occurrence and the corresponding γ is established for low solar (LSA), medium solar (MSA) and high solar (HSA) activity periods. For LSA, it is seen that the γ maximizes during post sunset time with comparable magnitudes for autumnal equinox (AE), vernal equinox (VE) and winter solstice (WS), while for summer solstice (SS) it maximizes in the post-midnight period. Concurrent responses are seen in the ESF occurrence pattern. For MSA, γ maximizes during post-sunset for VE followed by WS and AE while SS maximises during post-midnight period. The ESF occurrence for MSA is highest for VE (80%), followed by AE (70%), WS (60%) and SS (50%). In case of HSA, maximum γ occurs for VE followed by AE, WS and SS. The concurrent ESF occurrence maximizes for VE and AE (90%), WS and SS at 70%.The solar cycle variation of γ is examined. γ shows a linear variation with F10.7?cm flux. Further, ESF percentage occurrence and duration show an exponential and linear variation respectively with γ. An empirical model on the solar activity dependence of ESF occurrence and sustenance time over Indian longitudes is arrived at using the database spanning two solar cycles for the first time.