催化点火气氢气氧推力器试验研究

为探索催化点火气氢气氧推力器的点火规律和相关性能,设计并搭建了1N催化点火气氢气氧推力器试验系统,进行了冷热试试验。试验成功实现了不同工况下的多次催化点火。结果表明:供给氧氢混合比控制在100时,推力器预燃室产生的点火温度为700℃,能够满足燃烧室点火要求;催化剂面积体积比对催化氢氧点火具有决定性影响,采用面积体积比大的催化载体可以实现常温(8℃)下的催化点火;另外,试验中氢氧燃烧产生的高温和试验结束后推力器内残留的液态水也对催化组件提出了一定的耐温性和防水性要求。     

表面热流可辨识性初步分析

表面热流的可辨识性分析可用于飞行器防热层内温度测量精度和测温点位置的确定,在工程上有较强的实用意义。从无量纲分析和仿真辨识出发,根据防热层材料热物性系数、测点位置、表面热流的频域特性等参数对表面热流辨识结果的影响规律,总结出了表面热流辨识问题的相似参数：基于表面热流频率参数的傅立叶数。此后,以这一傅立叶数为判据,针对不同测量误差值的情况初步建立起了表面热流可辨识性的准则和分析方法。     

Analysis of geometrically nonlinear shells of revolution based on the finite element method with the vector interpolation of desired quantities

In this paper, we present an algorithm for geometrically nonlinear finite element analysis of the shells of revolution. Use is made of the most proper algorithms for vector interpolation of displacements through the nodal unknowns and an efficient algorithm for obtaining the stress-strain increment relation at a step of loading. By comparing the results of analyzing a geometrically nonlinear shell of revolution obtained on the basis of the ANSYS software with the scalar interpolation of displacements with those obtained on the basis of an author-developed finite element, it has been shown that application of the FEM vector displacement interpolation leads to increasing the accuracy of the finite element solutions in analyzing the stress-strain state of the geometrically nonlinear shells.     

圆度仪的数字化测量

介绍了对圆度仪的数字化改造方法。讨论了测量数据的数字化处理的方法及利用单纯形法对测量对象圆度进行评定，给出了实际的测量结果。     

大迎角细长旋成体绕流结构演变过程实验研究

 通过烟流显示和测压实验, 系统地观察和分析了尖拱头细长旋成体绕流结构随迎角的演变过程。实验发现在不同迎角下, 不仅细长旋成体绕流结构形态不同, 而且不同流态结构的演变过程所含迎角范围较小,几乎在几度迎角内就可完成。     

Modelling of the electromagnetic field in the interplanetary space and in the Earth's magnetosphere

A magnetohydrodynamic model of the solar wind flow is constructed using a kinematic approach. It is shown that a phenomenological conductivity of the solar wind plasma plays a key role in the forming of the interplanetary magnetic field (IMF) component normal to the ecliptic plane. This component is mostly important for the magnetospheric dynamics which is controlled by the solar wind electric field. A simple analytical solution for the problem of the solar wind flow past the magnetosphere is presented. In this approach the magnetopause and the Earth's bow shock are approximated by the paraboloids of revolution. Superposition of the effects of the bulk solar wind plasma motion and the magnetic field diffusion results in an incomplete screening of the IMF by the magnetopause. It is shown that the normal to the magnetopause component of the solar wind magnetic field and the tangential component of the electric field penetrated into the magnetosphere are determined by the quarter square of the magnetic Reynolds number. In final, a dynamic model of the magnetospheric magnetic field is constructed. This model can describe the magnetosphere in the course of the severe magnetic storm. The conditions under which the magnetospheric magnetic flux structure is unstable and can drive the magnetospheric substorm are discussed. The model calculations are compared with the observational data for September 24–26, 1998 magnetic storm (Dst _min=−205 nT) and substorm occurred at 02:30 UT on January 10, 1997. This revised version was published online in August 2006 with corrections to the Cover Date.     

Summary of quantitative interpretation of IMAGE far ultraviolet auroral data

Direct imaging of the magnetosphere by instruments on the IMAGE spacecraft is supplemented by simultaneous observations of the global aurora in three far ultraviolet (FUV) wavelength bands. The purpose of the multi-wavelength imaging is to study the global auroral particle and energy input from the magnetosphere into the atmosphere. This paper describes the method for quantitative interpretation of FUV measurements. The Wide-Band Imaging Camera (WIC) provides broad band ultraviolet images of the aurora with maximum spatial resolution by imaging the nitrogen lines and bands between 140 and 180 nm wavelength. The Spectrographic Imager (SI), a dual wavelength monochromatic instrument, images both Doppler-shifted Lyman-α emissions produced by precipitating protons, in the SI-12 channel and OI 135.6 nm emissions in the SI-13 channel. From the SI-12 Doppler shifted Lyman-α images it is possible to obtain the precipitating proton flux provided assumptions are made regarding the mean energy of the protons. Knowledge of the proton (flux and energy) component allows the calculation of the contribution produced by protons in the WIC and SI-13 instruments. Comparison of the corrected WIC and SI-13 signals provides a measure of the electron mean energy, which can then be used to determine the electron energy flux. To accomplish this, reliable emission modeling and instrument calibrations are required. In-flight calibration using early-type stars was used to validate the pre-flight laboratory calibrations and determine long-term trends in sensitivity. In general, very reasonable agreement is found between in-situ measurements and remote quantitative determinations.     

刘家峡右岸水电站模型试验的光路布置

使用二维激光多普勒测速仪（ＬＤＶ）对圆管中水注流进行测速时,对于窗口的设置、利用反射镜前向接收的方法和侧向接收方式等问题,本文进行了探讨,并总结了测量中的一些实际经验。     

灯丝放电磁场约束型原子氧效应地面模拟试验设备

介绍了用于原子氧剥蚀效应研究的灯丝放电磁场约束型地面模拟设备 ( IFM)的构成及工作原理,简单阐述了装置的运行测量结果,分析了等离子体参数随试验条件的变化趋势。并用 IFM设备对 Kapton空间用材料进行了地面模拟试验,试验结果与国外空间飞行暴露试验结果相似     

混流式水泵工况起动过渡过程导叶漏水的计算

本文利用动量矩定理推导出抽水蓄能电站水泵轮机导叶漏水量与漏水转矩的计算公式。同时在考虑漏水转矩的情况下,完成了两座抽水蓄能电站混流式水泵机组泵工况起动过渡过程的校核计算,分析了导叶间隙、漏水量等对起动过程的重要影响,过大的导叶间隙将使机组不能起动。计算分析表明,本文提出的考虑导叶间隙漏水影响进行泵工况起动过渡过程的计算方法是正确的。正确考虑漏水转矩影响,对水泵水轮机的运行特性和过滤过程的准确计算具