固体火箭发动机无损检测技术和结构缺陷判废标准研究的发展和展望

阐述了近年来固体火箭发动机整体综合无损检测中采用的新技术和固体火箭发动机结构缺陷判废标准研究的一些进展。根据最近出现的新检测设备和研究结果，展望了这一研究领域未来的发展趋势。     

组合叶栅的定义及其应用研究

提出了组合叶栅设想及其评价准则 ,并对组合叶栅进行了性能实验。通过实验数据的分析 ,肯定了组合叶栅设想应用于可逆风机叶片设计的可行性。实验还证明 ,选取适当的叶栅组合参数 B、T,可以使组合叶栅的整体性能得到大幅度的改善 ,与现有的翼型相比 ,CN Ry max、αN RCymax均有不同程度的提高     

联接翼布局直接升力控制特性的初步研究

本文对联接翼气动布局的直接升力控制特性进行了初步的探索。通过前、后机翼上升降舵面的同向偏转组合所产生的直接升力，与相应的正常布局相比较，不仅显示了飞机优异的气动性能：增加了最大升力系数和升力线斜率，改善了失速特性，提高了纵向静稳定性，而且明显改善了ΔＣｙ、Δｎｙ、ΔＨ、ωｚ等参数对操纵输入的瞬态响应品质，给飞机提供独立的姿态或轨迹控制的非同寻常的运动模态。头部鸭翼的增加进一步提高和改善了联接翼布局的直接升力特性。     

基于ATE技术的末制导雷达“天线对零”实现方案

在叙述“天线对零”过程重要性的基础上,介绍了基于ATE技术的末制导雷达“天线对零”自动过程的实现方案。该自动“天线对零”方案已经应用在“末制导雷达通用检测系统”中,保证了系统的高精度自动化测量。     

风挡防（除）雾表面瞬态热特性计算

风挡表面瞬态热特性计算是热空气射流防（除）雾系统设计的重要内容。在分析风挡防（除）雾换热机理的基础上，建立了风挡表面瞬态热特性的计算模型，用差分法对其求解。通过计算机模拟，得出计算结果，与试验结果比较，计算误差小于５％，研究的内容，具有工程实用价值。     

One-up on L1: Can X-rays provide longer advanced warning of solar wind flux enhancements than upstream monitors?

Observations of strong solar wind proton flux correlations with ROSAT X-ray rates along with high spectral resolution Chandra observations of X-rays from the dark Moon show that soft X-ray emission mirrors the behavior of the solar wind. In this paper, based on an analysis of an X-ray event observed by XMM-Newton resulting from charge exchange of high charge state solar wind ions and contemporaneous neutral solar wind data, we argue that X-ray observations may be able to provide reliable advance warning, perhaps by as much as half a day, of dramatic increases in solar wind flux at Earth. Like neutral atom imaging, this provides the capability to monitor the solar wind remotely rather than in situ.     

Propagation of interplanetary shocks into the Earth’s magnetosphere

This paper is devoted to the study of propagation of disturbances caused by interplanetary shocks (IPS) through the Earth’s magnetosphere. Using simultaneous observations of various fast forward shocks by different satellites in the solar wind, magnetosheath and magnetosphere from 1995 till 2002, we traced the interplanetary shocks into the Earth’s magnetosphere, we calculated the velocity of their propagation into the Earth’s magnetosphere and analyzed fronts of the disturbances. From the onset of disturbances at different satellites in the magnetosphere we obtained speed values ranging from 500 to 1300 km/s in the direction along the IP shock normal, that is in a general agreement with results of previous numerical MHD simulations. The paper discusses in detail a sequence of two events on November 9th, 2002. For the two cases we estimated the propagation speed of the IP shock caused disturbance between the dayside and nightside magnetosphere to be 590 km/s and 714–741 km/s, respectively. We partially attributed this increase to higher Alfven speed in the outer magnetosphere due to the compression of the magnetosphere as a consequence of the first event, and partially to the faster and stronger driving interplanetary shock. High-time resolution GOES magnetic field data revealed a complex structure of the compressional wave fronts at the dayside geosynchronous orbit during these events, with initial very steep parts (10 s). We discuss a few possible mechanisms of such steep front formation in the paper.     

利用F区电离层特性参量获取等效中性风的方法及讨论

讨论利用电离层特性参量获取F层峰值高度附近中性风信息的三类方法.这些方法主要有:传统的和改进的伺服理论方法、借助电离层模式和数据同化思想的方法和刘立波等提出的方法.并以美国Millstone Hill非相干散射雷达浓度剖面和离子速度数据,以及澳大利亚Beveridge(37°S,144°E)FPI风场和测高仪数据为个例,初步考察利用电离层特性数据导出的等效中性风与观测值的一致性.     

粉尘运动风洞模拟试验的相似律

本文提出了粉粒状堆料风吹起尘规律研究的相似律和在装卸作业中风吹扬尘规律研究的相似律,所获得的一些相似律,经大小两个风洞试验验证是较为满意的,并以此为指导,对煤堆起尘和煤炭装卸中起尘作了大量风洞模型试验,其结果表明也是合理的。