Academy of Aerospace Solid Propulsion Technology

Academy of Aerospace Solid Propulsion Technology (AASPT) is a professional research institution which is responsible for the design, development, manufacture, conducting various tests on     

Developing Space Manufacturing Industry To Serve National Economy And Promote Social Progress

Over the past 50 or more years, China's space industry has made brilliant achievements typically represented by the three milestones in China's space development history,i.e.launching the first man-made satellite into space in 1970,realizing the manned spaceflight for the first time in 2003 and sending the first lunar probe to the moon in 2007.At the same time, China's space industry has also mastered a great number of core technologies based upon its own intellectual property rights,accumulated rich exp...     

Influence of solar-geomagnetic disturbances on SABER measurements of 4.3 μm emission and the retrieval of kinetic temperature and carbon dioxide

Thermospheric infrared radiance at 4.3 μm is susceptible to the influence of solar-geomagnetic disturbances. Ionization processes followed by ion-neutral chemical reactions lead to vibrationally excited NO⁺ (i.e., NO⁺(v)) and subsequent 4.3 μm emission in the ionospheric E-region. Large enhancements of nighttime 4.3 μm emission were observed by the TIMED/SABER instrument during the April 2002 and October–November 2003 solar storms. Global measurements of infrared 4.3 μm emission provide an excellent proxy to observe the nighttime E-region response to auroral dosing and to conduct a detailed study of E-region ion-neutral chemistry and energy transfer mechanisms. Furthermore, we find that photoionization processes followed by ion-neutral reactions during quiescent, daytime conditions increase the NO⁺ concentration enough to introduce biases in the TIMED/SABER operational processing of kinetic temperature and CO₂ data, with the largest effect at summer solstice. In this paper, we discuss solar storm enhancements of 4.3 μm emission observed from SABER and assess the impact of NO⁺(v) 4.3 μm emission on quiescent, daytime retrievals of Tk/CO₂ from the SABER instrument.     

Interplanetary Coronal Mass Ejections Observed in the Heliosphere: 2. Model and Data Comparison

With the recent advancements in interplanetary coronal mass ejection (ICME) imaging it is necessary to understand how heliospheric images may be interpreted, particularly at large elongation angles. Of crucial importance is how the current methods used for coronal mass ejection measurement in coronagraph images must be changed to account for the large elongations involved in the heliosphere. We present results comparing a new model of interplanetary disturbances with heliospheric image data, from the Solar Mass Ejection Imager. A database containing a range of ICMEs simulated with varying parameters describing its topology, orientation, location and speed was produced and compared with two ICMEs observed in February and December 2004. We identify the simulated ICME that best matches the data, and use the parameters required to identify their three-dimensional leading-edge structure, orientation and kinematics. By constant comparison with the data we are able to keep track of small changes to the ICME topology and kinematic properties, thus for the first time are able to monitor how the dynamic interaction between the ICME and the interplanetary medium affects ICME evolution. This is the second part of a series of three papers, where the theory behind the model is presented in an accompanying paper and the physical implications are discussed in the third part. The first part considers the effects of Thomson scattering across the entire span of the disturbance and includes its apparent geometry at large elongations. We find that the model converges reliably to a solution for both events, although we identify four separate structures during the December period. Comparing the 3-D trajectory and source location with known associated features identified with other spacecraft, we find a remarkable agreement between the model and data. We conclude with a brief discussion of the physical implications of the model.     

AN ELEMENTARY ANALYSIS OF PROBLEMS IN APPLICATION OF SPACE METHOD IN STRATEGIC MANAGEMENT OF ENTERPRISES

企业战略管理在我国还是一门新兴学科，随着改革发展的深入，越来越多的企业已认识到它的重要性，并最终采用它。本文论述了在企业战略管理ＳＰＡＣＥ方法中，如何应用Ｄｅｌｐｈｉ方法确定企业战略要素及评价。而它的确定及评价，真实刻划了企业在目前竞争环境中所处的战略位置，为企业正确选择发展战略奠定了基础。     

基于升力线理论的机翼几何扭转设计方法

针对飞机设计对于减小诱导阻力的需求,结合升力线理论中三维机翼诱导阻力的相关研究,提出机翼的几何扭转设计方法.此设计方法以总升力、机翼平面形状、翼型气动特性为输入参数,以机翼的几何扭转为输出.在低速情况下,利用此方法得到的机翼具有椭圆形升力分布,从而具有最小的诱导阻力.采用远场法计算诱导阻力,应用参数化方法和CATIA实现机翼的自动生成,应用网格生成工具ICEM的脚本语言实现气动网格自动生成,应用MATLAB的符号运算功能编制程序.该设计方法适用于低速有粘流中平直翼的几何扭转设计,算例的CFD(Computational Fluid Dynamics)计算结果表明:利用该方法设计的机翼展向升力分布为椭圆,并能有效降低机翼的诱导阻力.     

用于海洋磁测的芯片量子干涉磁力仪

随着海洋环境探测工作的发展,海域磁测对磁力仪在微小型化、高精度方面提出了新的需求.在介绍了几个常见的弱磁场测量仪器后,重点分析了一种基于双光场量子干涉效应的磁力仪.根据在磁场中光与原子相互作用的物理机制,阐析了利用量子干涉效应进行高精度磁场测量的基本原理.在此基础上,分析了在芯片上实现量子干涉磁力仪的可能性,详细讨论了芯片量子干涉磁力仪的一种设计方案,并给出了芯片量子干涉磁力仪的性能预期以及其在海洋磁测领域的应用前景.     

基于神经网络的电磁干扰的预测

提出了一种应用神经网络预测电磁干扰的方法.针对遗传算法总体搜索能力较强但容易陷入局部最优,而模拟退火算法具有较强的局部搜索能力,又能避免搜索陷入局部最优解的特点,将模拟退火算法与遗传算法相结合,优化多层前馈(BP, Back Propagation)神经网络,获取最优的权值和阈值,并采用模拟退火的思想确定隐含层神经元的个数,进而建立基于神经网络的电磁干扰预测模型.以双平行导线间的电磁干扰问题为实例,明确干扰要素,建立训练样本和测试样本,对比期望输出和预测输出之间的误差,结果表明该方法可以准确有效地进行电磁干扰预测.