多点压力扫描阀系统在测量大型复射流流场中的应用

一种由微机控制的测量速度和压力的快速扫描阀系统已经用于双流道氧枪复射流流场中。在氧气炼钢转炉中为了使 CO 进行二次燃烧,必须使用双流道氧枪。为了研究双流道氧枪复射流特性,在射流完全发展区沿直径方向放一根测杆,在测杆上排列着96支皮托管。皮托管末端的总压管和静压管用塑料软管分别与扫描阀中的4个压力传感器相连接,在16秒钟内扫描阀能自动扫描192个测压点。结果,总压、静压和速度分布能立即显示在 CRT上。为了获得高的测量精度,压力传感器的零点漂移能由软件来消除,同时每支皮托管都用 DANTEC 标定设备进行了速度标定。该测量系统也能用于其它工业规模的流场,如大型风洞,喷气发动机,流化床等。     

涡轮叶片内冷却通道的流阻与换热研究

用实验方法研究了冷却气流在放大1倍模型涡轮叶片内通道的压力、冷热态流阻及局部换热系数分布。得出了相应的经验公式。冷却空气径向进入前缘冷却通道, 到顶端折而向下在两隔板间流动, 大部分空气经隔板5个穿孔弦向流入带三排扰流柱的收缩通道, 并弦向排出叶片尾部。      

平面应力裂端约束与J控制裂纹稳态扩展

利用有限元法计算模拟了紧凑拉伸和中心裂纹两种试样在Ⅰ型平面应力条件下的裂纹准静态扩展过程。结果表明:两种不同的薄板试样中扩展裂纹尖端约束和应力场完全满足静态裂纹HRR奇异性解的相应要求,即对于扩展裂纹J主导裂端场条件依然有效。值得注意的是:与平面应变情形相反,在平面应力条件下,较高的J主导水平发生在纯拉伸条件下,而较低的J主导水平发生在纯弯曲条件。由两种试样实测及有限元计算模拟的平面应力J阻力曲线符合良好。因而,作为一个独立于试样几何的准则,平面应力J阻力曲线适于表征材料抵抗裂纹稳态扩展阻力,并且能够合理地用于评估给定材料状态条件下的薄壁含裂纹构件和结构的安全性。     

复合丁羟推进剂压强指数现状评述

本文详细叙述了我国研究压强指数的历史、低压强指数的优点,列举了我国丁羟推进剂压强指数研究的状况,分析比较了国内外水平,指出了今后努力方向.     

密闭容器试验用人体代谢模拟装置

文章简要介绍了人体代谢地面模拟装置的原理、结构组成和应用结果。为在密闭容器中进行地面模拟试验,考核产品性能提供了一个较为可靠而全面的模拟环境。     

Adaptive recognition and correction of baseline shifts from collocated GPS and accelerometer using two phases Kalman filter

The real-time recognition and precise correction of baseline shifts in strong-motion records is a critical issue for GPS and accelerometer combined processing. This paper proposes a method to adaptively recognize and correct baseline shifts in strong-motion records by utilizing GPS measurements using two phases Kalman filter. By defining four kinds of learning statistics and criteria, the time series of estimated baseline shifts can be divided into four time intervals: initialization, static, transient and permanent. During the time interval in which the transient baseline shift is recognized, the dynamic noise of the Kalman filter system and the length of the baseline shifts estimation window are adaptively adjusted to yield a robust integration solution. The validations from an experimental and real datasets show that acceleration baseline shifts can be precisely recognized and corrected, thus, the combined system adaptively adjusted the estimation strategy to get a more robust solution.     

磁暴期间甚低纬哨声的导管传播

对磁暴期间甚低纬哨声导管传播的机理进行了初步的讨论，根据暴时低纬哨声的特点，认为暴时出现的扩展哨、多跳回波是沿东向扰动电场导致的场列电离增强路径传播的。对在东向电场影响下低纬Ｆ层的数值模拟表明，东向电场导致的场列电离增强结构有利于哨声的捕获和传播。     

平台压强指数附加物“TCA”与配方组分粒度和含量的关系

较详细地叙述了平台推进剂压强指数附加物“ＴＣＡ”与推进剂组与的粒度、含量的关系。     

MHD structures, waves and turbulence in the solar wind: Observations and theories

A comprehensive overview is presented of recent observational and theoretical results on solar wind structures and fluctuations and magnetohydrodynamic waves and turbulence, with preference given to phenomena in the inner heliosphere. Emphasis is placed on the progress made in the past decade in the understanding of the nature and origin of especially small-scale, compressible and incompressible fluctuations. Turbulence models to describe the spatial transport and spectral transfer of the fluctuations in the inner heliosphere are discussed, and results from direct numerical simulations are dealt with. Intermittency of solar wind fluctuations and their statistical distributions are briefly investigated. Studies of the heating and acceleration effects of the turbulence on the background wind are critically surveyed. Finally, open questions concerning the origin, nature and evolution of the fluctuations are listed, and possible avenues and perspectives for future research are outlined.     

Augmented Empirical Models of Plasmaspheric Density and Electric Field Using IMAGE and CLUSTER Data

Empirical models for the plasma densities in the inner magnetosphere, including plasmasphere and polar magnetosphere, have been in the past derived from in situ measurements. Such empirical models, however, are still in their initial phase compared to magnetospheric magnetic field models. Recent studies using data from CRRES, Polar, and Image have significantly improved empirical models for inner-magnetospheric plasma and mass densities. Comprehensive electric field models in the magnetosphere have been developed using radar and in situ observations at low altitude orbits. To use these models at high altitudes one needs to rely strongly on the assumption of equipotential magnetic field lines. Direct measurements of the electric field by the Cluster mission have been used to derive an equatorial electric field model in which reliance on the equipotential assumption is less. In this paper we review the recent progress in developing empirical models of plasma densities and electric fields in the inner magnetosphere with emphasis on the achievements from the Image and Cluster missions. Recent results from other satellites are also discussed when they are relevant.