民用通风机气动设计新特点及设计方法的新发展

本文通过对一种新型高性能矿用局部通风机的设计、制造及试验全过程的综述,展现了新的先进设计体系在民用通风机上的成功运用,其研制特点是:(1)在叶片气动设计中为了降低叶根及叶尖区二次流损失,采用可控涡扭向规律设计,样机实测的高性能验证了这种方法的可行性和高效性;(2)在设计方法中采用较精确的数值反验算,获取最优设计方案,大大提高设计的准确性和成功率,并缩短了设计试制周期。      

Apmoc-II和Kevlar-49纤维结晶的X射线衍射分析研究

采用Ｘ射线衍射（ＸＲＤ）方法与理论,对Ａｐｍｏｃ－Ⅱ和Ｋｅｖｌａｒ－４９纤维进行了Ｘ射线衍射测试。应用图解分峰法对衍射图中结晶峰与非结晶峰进行了分离,分别计算出各结晶峰与非结晶峰的相对积分强度,从而计算出各自结晶度及晶面间距的大小,其中Ａｐｍｏｃ－Ⅱ和Ｋｅｖｌａｒ－４９纤维的结晶度分别为５２．３４％与６８．６８％,同时分析了两种纤维结晶程度、晶面间距差别的原因。然后把两种纤维分别溶于浓Ｈ２ＳＯ４,     

Modified Generalized Sign Test Processor for 2-D Radar

The modified generalized sign test processor is a nonparametric, adaptive detector for 2-D search radars. The detector ranks a sample under test with its neighboring samples and integrates (on a pulse-to-pulse basis) the ranks with a two-pole filter. A target is declared when the integrated output exceeds two thresholds. The first threshold is fixed and yields a 10-6 probability of false alarm when the neighboring samples are independent and identically distributed. The second threshold is adaptive and maintains a low false-alarm rate when the integrated neighboring samples are correlated and when there are nonhomogeneities, such as extraneous targets, in the neighboring cells. Using Monte Carlo techniques, probability of false-alarm results, probability of detection curves, and angular accuracy curves have been generated for this detector. The detector was built and PPI photographs are used to indicate the detector's performance when the radar is operated over land clutter.     

7. Dynamics,winds, circulation and turbulence in the atmosphere of venus

With the possible exception of the lowest one or two scale heights, the dominant mode of circulation of Venus' atmosphere is a rapid, zonal, retrograde motion. Global albedo variations in the ultraviolet may reflect planetary scale waves propagating relative to the zonal winds. Other special phenomena such as cellular convection in the subsolar region and internal gravity waves generated in the interaction of the zonal circulation with the subsolar disturbance may also be revealed in ultraviolet imagery of the atmosphere. We discuss the contributions of experiments on the Orbiter and Entry Probes of Pioneer Venus toward unravelling the mystery of the planet's global circulation and the role played by waves, instabilities and convection therein.     

Relationship Between Substorm Auroras and Processes in the Near-Earth Magnetotail

Although the auroral substorm has been long regarded as a manifestation of the magnetospheric substorm, a direct relation of active auroras to certain magnetospheric processes is still debatable. To investigate the relationship, we combine the data of the UV imager onboard the Polar satellite with plasma and magnetic field measurements by the Geotail spacecraft. The poleward edge of the auroral bulge, as determined from the images obtained at the LHBL passband, is found to be conjugated with the region where the oppositely directed fast plasma flows observed in the near-Earth plasma sheet during substorms are generated. We conclude that the auroras forming the bulge are due to the near-Earth reconnection process. This implies that the magnetic flux through the auroral bulge is equal to the flux dissipated in the magnetotail during the substorm. Comparison of the magnetic flux through the auroral bulge with the magnetic flux accumulated in the tail lobe during the growth phase shows that these parameters have the comparable values. This is a clear evidence of the loading–unloading scheme of substorm development. It is shown that the area of the auroral bulge developing during substorm is proportional to the total (magnetic plus plasma) pressure decrease in the magnetotail. These findings stress the importance of auroral bulge observations for monitoring of substorm intensity in terms of the magnetic flux and energy dissipation.     

An Introduction to CMEs and Energetic Particles

Energetic particle observations in the interplanetary medium provide fundamental information about the origin, development and structure of coronal mass ejections. This paper reviews the status of our understanding of the ways in which particles are energised at the Sun in association with CMEs. This understanding will remain incomplete until the relationship between CMEs and flares is determined and we know the topology of the associated magnetic fields. The paper also discusses the characteristics of interplanetary CMEs that may be probed using particle observations.     

基于语音标签的语音浏览器

随着互联网的发展,Web已经成为获取各种信息的重要途径,但是并不是所有人都能享受互联网所带来的便利。针对某些不便于使用鼠标和键盘输入的情况,开发了一个基于语音的网页浏览系统。主要特点是通过采用给网页自动添加语音标签的方法来辅助用户与互联网的语音交互。该系统通过对互联网上的网页进行本地缓存并加入语音标签,对用户的语音输入进行引导和提示,实现了语音控制的网页浏览。     

气氢/气氧塞式喷管模型发动机实验

以气氢/气氧为推进剂,对圆转方内喷管单元直排塞式喷管进行了热试实验研究。介绍了实验系统及实验发动机主要零部件的结构和设计参数,给出了实验参数测量结果、实验照片和数据分析。无再生冷却塞式喷管发动机采用耐烧蚀材料钨渗铜加工内喷管和燃烧室内衬,碳钢材料加工塞锥,成功进行了多次短时间热试实验。在三个压比下获得了塞式喷管性能数据,实验表明,塞式喷管具有良好的高度补偿能力和较高的效率。在CNPR=110附近,效率达到93%~95%;在CNPR=450附近,效率达到96%~98%;在CNPR=1000附近,效率达到93%~96%。预计在设计点的效率不低于98%。     

缝合复合材料弹性常数细观力学模型的分析比较

对近几年来公开发表的缝合复合材料弹性常数的细观力学模型进行了分析比较。通过计算对比了铺层纤维面内弯折、正弦波状弯曲、多项式描述纤维弯曲三个典型的缝合复合材料弹性常数的细观力学分析模型。结果表明,采用面内纤维弯折假设的弹性常数分析模型对缝纫参数的改变不敏感;采用面内纤维弯曲假设的模型对缝纫参数改变敏感,不同模型得到的弹性常数随缝纫参数变化趋势几乎是相同的。但是,假设纤维在针脚附近只有部分纤维发生弯曲比假设纤维全部发生弯曲得到的结论更合理。     

飞行器尖化前缘的热结构特性

在分析尖化前缘热环境特性的基础上,给出了尖化前缘相应的热结构特性的计算和分析,分析结果表明：尖化前缘热流密度在2～3个自由程内下降到原来的1/3,而表面温度仅有10%的下降;高热导率的防热材料可降低前缘的最高表面温度,对非烧蚀热防护十分有利,它还可提高后部的表面温度,增加辐射散热的力度,这是非烧蚀热防护的重要机制.