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     

尖脊(Caret)进气道地面气动特性试验研究

在地面静止状态下试验研究了尖脊进气道气动特性以及唇口厚度对进气道性能影响 ,给出了进气道各侧壁沿程静压分布及其出口总压分布图谱 ,研究了进气口流动特点及其对出口总压畸变流场的影响。试验表明 ,Caret进气道进口存在一大一小的反向旋转涡 ,该旋涡的作用使得进气道高、低压区均旋转了 90°以上。进口下唇口和外唇口厚度对地面静止状态下的进气道总压恢复系数和总压畸变指数有较大的影响 ,为进气唇口厚度的选择提供了依据。     

弹道导弹自由段飞行中的守恒量及其应用

从精确弹道计算所用的数学模型出发，指出了弹性在自由段飞行中的两个具有明确物理意义的运动守恒量，并给出了用发射坐标系下的运动参数求这些守恒量的简洁计算公式。这两个守恒量可作为一种简单、实用的辅助评估手段用于计算结果可信性分析以及导弹发射诸元的校验。     

壁面加热湍流标度律的实验研究

用热线风速仪测量了风洞中壁面加热和不加热平板湍流边界层不同法向位置的流向速度和温度的时间序列信号，研究了壁面加热的边条件和不同法向位置的剪切作用对速度和温度增量的p阶结构函数的非线性反常标度律的影响，实验结果表明，壁面加热的边界条件不同法向位置的剪切作用对层次结构模型中间歇参数β和最奇异指数γ的影响明显存在，并初步分析了在具有强剪切作用的壁湍流中这种影响产生的原因。     

An Algorithm for Designing Burst Waveforms with Quantized Transmitter Weights

An algorithm is described which finds optimum transmitter and receiver weights to maximize clutter suppression in a predetermined clutter region when using burst waveforms. It is assumed that the transmitter weights can only take on values from a finite set. This optimization problem is solved using a branch and bound algorithm. An example is given which shows the improvement in clutter suppression when this new design procedure is used as compared to a simpler nonoptimal procedure.     

三维极坐标视线动力学

阐述了极坐标视线动力学方程的研究现状。建立了三维极坐标视线动力学方程，讨论了该动力学方程的简化问题，得到了特殊平面（攻击平面）内的简化形式，该简化形式在特定的条件下与三维极坐标视线动力学方程是等价的。