Preliminary Study on Magnetic Induction Intensity Induced by Plasma During Hypervelocity Impact

An experimental system has been built to produce and measure the magnetic field in the backward ejected matter during hypervelocity impact. The designs of measurement system and coil, the choice of associated equipment, and the system calibration are also described in detail. The measurement of magnetic induction intensity for different given coil positions and azimuth angles are performed with two-stage light-gas gun. On condition that impact velocities are approximately equal and incidence angles are 45°, 60° and 90° respectively, the relationship between average magnetic induction intensity and impact angle at different time spans is obtained. Experimental results show that the average magnetic induction intensity with incidence angle of 90° is larger than those with incidence angles of 45°and 60°.     

高负荷低压涡轮时序效应数值模拟与试验验证

为了研究上下游叶片的相位对低压涡轮流动的影响机理，使用商用 CFX 软件进行数值模拟，并辅以试验校核。选取了 0°和180°2个流动相差较大的相位，分析边界层分离与转捩、边界层积分参数，对吸力面的载荷系数、壁面剪力、附面层形状因子及 动量厚度等进行对比，并从边界层的瞬态流动分析着手，在1个尾迹扫掠周期内对Klebanoff条纹、K-H涡等结构进行分析。结果 表明：不同相位的流动特性差异主要取决于势流的压力扰动与速度扰动的相位，这将决定尾迹诱导转捩与寂静区之间的主导关 系。当压力扰动与速度扰动同相时，寂静区处于逆压梯度逐渐增强的阶段，保持层流的能力被削弱；反之当二者异相时寂静区强 度较大，尾迹诱导转捩带来的湍流损失可以被寂静区平衡。通过瞬态分析可知，0°相位尾迹诱导全展向K-H涡的卷起，全展向涡 的破碎会带来较大的能量耗散，且其诱导的Klebanoff条纹强度较大，二者共同作用使得尾缘动量损失较大。     

An investigation of high frequency auroral plasma emissions with a tubular dipole antenna

A band of enhanced amplitudes which follows a local plasma frequency fn in raw high frequency (HF) noise spectra is usually related to plasma emissions in the upper hybrid band (fn, fu). The enhanced band in question occurs permanently in noise spectra recorded on the Intercosmos-19, APEX and CORONAS satellites in the altitude range of 500 km–3000 km. For moderately magnetized plasma with fn > 2fc (fc – electron gyro frequency), the band occurs below fn determined from the topside sounder and impedance data or from electron beam induced spectra. The simulations of an equivalent circuit composed of a dipole antenna in a cold plasma and its preamplifiers, determined the physical origin of the band as the passive circuit resonance, due to inductive character of the antenna in a frequency band (fc, fu). The resonance spectral content is highly structured due to an inflight variability of the circuit impedances. In this report we analyze the noise and impedance spectra which are the most typical in an auroral zone if fn > fc. We focus attention on determination of local electron plasma density, essential for provisional HF mode classification. We found that the natural plasma emission in the upper hybrid band does not manifest itself as the banded natural emission, which may be used for reliable determination of local plasma frequency in the altitude range of 500–3000 km. The fast magnetosonic mode predominates in the auroral emissions. The broadband and multi banded electromagnetic emissions extending from the fast magnetosonic band well above fn > fc are characteristic for the strong wave activity and are much less frequent.     

JUXTA: A new probe of X-ray emission from the Jupiter system

For the future Japanese exploration mission of the Jupiter’s magnetosphere (JMO: Jupiter Magnetospheric Orbiter), a unique instrument named JUXTA (Jupiter X-ray Telescope Array) is being developed. It aims at the first in-situ measurement of X-ray emission associated with Jupiter and its neighborhood. Recent observations with Earth-orbiting satellites have revealed various X-ray emission from the Jupiter system. X-ray sources include Jupiter’s aurorae, disk emission, inner radiation belts, the Galilean satellites and the Io plasma torus. X-ray imaging spectroscopy can be a new probe to reveal rotationally driven activities, particle acceleration and Jupiter–satellite binary system. JUXTA is composed of an ultra-light weight X-ray telescope based on micromachining technology and a radiation-hard semiconductor pixel detector. It covers 0.3–2 keV with the energy resolution of <100 eV at 0.6 keV. Because of proximity to Jupiter (∼30 Jovian radii at periapsis), the image resolution of <5 arcmin and the on-axis effective area of >3 cm² at 0.6 keV allow extremely high photon statistics and high resolution observations.     

用椭圆型、抛物型两种方法计算平面叶栅湍流尾迹

本文用连续方程、稳定不可压缩椭圆型和抛物型时均N-S方程及K-ε双方程湍流模型计算了平面叶栅湍流尾迹。计算表明,上述两种方法都能得到较好的数值结果,但抛物方法可节省大量计算时间和内存空间。     

运动等离子柱体的电磁散射

 本文应用Minkowski变换研究了轴向运动非均匀等离子柱体的电磁散射。表明在坐标变换中易于导出相应稳态问题的解。文中详细研究了一半径为1m的等离子柱体的一些散射远场特性,其中包括远场方向图和后向散射横截面积(RCS)。     

基于等离子体激励器简化模型的流动分离控制

对等离子体激励器做简化模型,并研究简化模型对于NACA0015翼型流动分离的控制效果.通过改变激励器在翼型上表面的位置及激励强度的大小,研究了实施流动控制的较佳位置及强度的大小.数值模拟结果表明,在前缘点附近加入控制的作用要优于其它位置;且激励强度对于流动控制的效果有极大的影响,大的激励强度有好的控制效果.此控制方法可以有效地延迟流动的分离,达到增升减阻的目的.是一种有前途的流动主动控制方法.     

Spraying of Super Fine Powders With HVOF and Axial Plasma Thermal Spray Systems

The use of fine powders in thermal spray can lead to many advantages. These advantages include denser coatings, coatings with increased wear resistance, coatings with smoother surface finish, coatings that can be applied to internal surfaces, less expensive coatings. The use of fine powders also has an disadvantage that th ey can have poor flow characteristics. The paper will discuss a feeder that is able to feed fine powders to overcome this difficulty and the coating equipment, both axial plasma and HVOF systems, used to deposit these materials to produce smooth dense coatings.     

瞬态空气等离子体场的全息术研究

采用双波长双脉冲激光全息术,对有激波存在下的空气放电现象进行了研究。建立了双波长电弧折射率场方程,推导出冲击波区的压强同折射率之间的关系式,得出电弧场的压强分布.曲线及等离子体区的温度分布和电子、离子、原子、分子等粒子的数密度分布。