ZL205A铝合金大型复杂筒体构件淬火过程模拟与变形预报

基于ABAQUS软件采用有限元方法建立ZL205A铝合金大型复杂构件淬火过程的温度场与应力场模型,分析构件在淬火过程中不同时刻的温度场分布.根据构件结构特征,选择4个特征点获得淬火过程冷却曲线,并对构件厚壁、加强筋与薄壁部分的冷却曲线进行研究,使用有限元模拟方法预报构件变形和残余应力.ZL205A铝合金大型复杂构件淬火变形主要为径向变形,通过比较淬火后残余应力的6个分量可知正应力远大于剪应力.模拟厚壁在不同换热系数下的淬火效果,发现增加换热系数可以提高厚壁淬火冷却速度,但是作用比较有限.     

Observing the Sun at 20–650 MHz at Thermopylae with Artemis

Fine structure of type IV radio solar bursts with a great variety and complexity often give much information in different ways and enable estimation of various coronal characteristics. In this work, we expose our new method for fine structure revealing and separation of two basic kinds of type IV fine structure, as fibers and pulsations. We also estimate frequency drift of fibers from dynamic spectra, clean from continuous background, with a prototype method using 2-D Fourier transform and we estimate periodicities of fibers as well as pulsations with continuous wavelet transform. Working with the last method we found periodicities close to 3 min umbral oscillations and 5 min global solar oscillations.     

基于DSP的数字下变频软件实现

数字下变频(DDC)技术将宽带大数据流信号变成窄带低数据流信号,以便 DSP 实时处理。在分析数字下变频的基本模型基础上,提出了一种基于 DSP 芯片的数字下变频软件实现方案,讨论了相应的算法及分析,并给出了软件实现的主程序结构。软件数字下变频比常规 DDC专用芯片有更大的灵活性、适应性和更高的处理中频。     

超声速来流稳焰凹腔上游气体燃料横向喷注的流动混合特征

对Ma=1.7的空气超声速来流稳焰凹腔上游气体燃料横向喷注的流动混合特征进行了实验和数值模拟研究。在喷注的模拟燃料氦气中添加丙酮,采用平面激光诱导荧光技术(PLIF)观测了设置开式凹腔时燃料在展向和流向的空间分布。针对下游布置不同凹腔时燃料分布相似的实验结果,选取L/D=7的凹腔对其燃料混合流场进行了大涡模拟。实验和仿真结果表明:实验来流条件下喷注燃料大部分直接由喷流引起的上升反转旋涡对带走,只有小部分燃料经由喷流与凹腔流动涡结构的相互作用进入凹腔剪切层,并随剪切层运动对流进入凹腔内部。     

基于火焰面模型的超声速燃烧混合LES/RANS模拟

为了明晰超燃冲压发动机燃烧室内部燃烧过程的细节,建立了超声速湍流燃烧稳态火焰面亚格子模型,并采用混合LES/RANS方法对氢燃料超燃冲压发动机进行算例验证.控制方程对流项用五阶精度WENO格式离散,时间方向采用二阶Runge-Kutta方法.研究表明:(1)冷流流场中燃料分布与大尺度结构分布相似,说明混合过程受大涡控制;(2)燃烧流场中涡的尺寸明显变大,且仅存在于火焰面上,另外温度分布和主要生成物分布与涡量云图基本相同,说明燃烧过程也由大涡控制;(3)时均计算结果与实验阴影基本符合,速度剖面和温度剖面与实验测量值定性一致,说明本文的数值模拟方法和燃烧模型可以较好地描述和预测超声速流动燃烧过程.     

大型不规则椭球回转面的曲面重构与仿真加工

提出了大型不规则椭球回转面的一种新的曲面重构与仿真加工方法。基于GeomagicStudio软件,处理大型不规则椭球回转面的采集数据点云,重构了实测曲面的等距面模型;采用Pro/E对实测曲面的等距面模型进行等距操作,生成实测曲面模型;利用GeomagicQualify软件对实测曲面的等距面模型相对于原始数据点云,以及实测曲面模型相对于理论曲面模型进行误差分析;最后利用Pro/NC模块对实测曲面模型进行数控编程和仿真加工。研究结果表明,该方法提高了大型不规则椭球回转面的曲面重构精度,生成的标准数控加工程序具有可移植性,解决了原加工方法对专用设备的依赖。     

Statistical study of radio drifting pulsation structures with associated CMEs and other observations

Solar radio burst, especially the fine structures (FSs) and the drifting pulsation structures (DPSs), may be used as an important diagnostics tool to draw the evolution map of the flare loop in the initial phase of solar flares. In this work, 52 radio events were found accompanying with DPSs. They were all observed with the Solar Radio Spectrometers (0.625–7.6 GHz) of China during 1998–2004. Combining the radio observations with LASCO-C2, Goes-8 SXR, H_α, EUV and Trace observations, we analyzed all these events and obtained some statistic conclusions: First, 88% DPSs take place at the initial phase of the radio burst, and their rich spectrum characteristics are helpful to understand the events further. Second, 83% DPSs are associated with CMEs or ejection events, and all the events are accompanied by Goes SXR flare. Third, for CMEs and DPSs, which take the first step, there is no significant predominance of either of them. The relationship between the DPSs and CMEs is still not clear in this study because of the lack of spatial resolution in the centimeter–decimeter band. However, the EIT or Trace ejection happened during the onset/end time of DPSs. They are signatures of the initial phase of CMEs. Two events will be illustrated to explain this.     

International scientific optical network for space debris research

A joint team of researchers under the auspices of the Center for Space Debris Information Collection, Processing and Analysis of the Russian Academy of Sciences collaborates with 15 observatories around the world to perform observations of space debris. For this purpose, 14 telescopes were equipped with charge-coupled device (CCD) cameras, Global Positioning System (GPS) receivers, CCD frame processing and ephemeris computation software, with the support of the European and Russian grants. Many of the observation campaigns were carried out in collaboration with the Astronomical Institute of the University of Bern (AIUB) team operating at the Zimmerwald observatory and conducting research for the European Space Agency (ESA), using the Tenerife/Teide telescope for searching and tracking of unknown objects in the geostationary region (GEO). More than 130,000 measurements of space objects along a GEO arc of 340.9°, collected and processed at Space Debris Data Base in the Ballistic Center of the Keldysh Institute of Applied Mathematics (KIAM) in 2005–2006, allowed us to find 288 GEO objects that are absent in the public orbital databases and to determine their orbital elements. Methods of discovering and tracking small space debris fragments at high orbits were developed and tested. About 40 of 150 detected unknown objects of magnitudes 15–20.5 were tracked during many months. A series of dedicated 22-cm telescopes with large field of view for GEO survey tasks is in process of construction. 7 60-cm telescopes will be modernized in 2007.     

民航VHF地空通信干扰对策研究

民航VHF地空通信干扰是近年来困扰中国民航的难点问题。通过对中国某机场干扰情况的深入调查和研究，明确了主要干扰源及其产生机理。同时结合中国电磁环境的实际情况和民航自身的特点，提出了从民航自身入手、加强管理、建立监控体系和应急VHF通信接收系统的解决思路。     

十二通道GPS信号发生器方案研制

为了测试GPS(全球定位系统)接收机的性能,需要应用GPS信号模拟器来模拟各种条件下真实的GPS信号.分析了单通道与多通道GPS信号的时域及频域特性,建立了十二通道GPS信号模拟器的数学模型.该模型应用了软件无线电的设计思想和内插理论,可以直接产生35.42MHz的中频信号,以降低硬件设计的复杂度.文中用SystemView软件的仿真结果验证了系统设计的可行性,并提出了该系统的硬件实现.