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.     

航天磁悬浮发射脉冲磁流体供能系统方案分析

针对航天发射低成本、安全可靠运输方式的需要,阐述分析了航天运载器磁悬浮发射概念及其能量供给需求。在重点研究了固体火箭燃料脉冲磁流体发电机的关键技术及发展水平后,基于俄罗斯四台“Sakhalin”脉冲磁流体发电机单元,提出和设计了用于助推发射100吨地面载荷(飞行器和磁悬浮橇体)实现4g加速度的能量供给方案,同时分析磁悬浮发射过程中三相直线电机加速和控制的特点,提出可行的逆变器功率转换系统方案。     

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。     

ISEE卫星等离子体能谱图片处理与初步分析

本文利用图象分析的方法，将ＩＳＥＥ卫星的等离子体能谱图数值化，以便定量地分析ＩＳＥＥ卫星观测到的磁尾等离子体和磁场资料。以及研究磁尾中性片的纤维结构，对今后研究近地磁尾（２２个地球半径以内）各种空间动力学机制，电流结构体系等问题都有很重要的利用价值。     

空间尘埃的充电过程及与等离子体参数的关系

考虑了地球附近的彗星、行星环、行星际介质等空间尘埃等离子体环境中尘埃颗粒的充电问题．应用典型的空间尘埃等离子体参数，计算了不同种类的尘埃颗粒，以及不同等离子体成分下等离子体中尘粒的平衡电势，得到了尘埃颗粒的平衡电势与尘埃等离子体成分、温度，及其他等离子体参数之间的相互关系．     

Numerical study of magnetic reconnection possibly occurring near heliospheric current sheet

The third-order accurate upwind compact difference scheme has been applied for the numerical study of the magnetic reconnection driven by a plasma blob impacting the heliospheric current sheet, under the framework of the two-dimensional compressible magnetohydrodynamics. The results show that the driven reconnection near the current sheet could occur in about 10–30 min for the interplanetary high magnetic Reynolds number, R_M = 2000–10,000, a stable magnetic reconnection structure can be formed in hour order of magnitude, and there appear some basic properties such as the multiple X-line reconnections, vortex structures, filament current systems, splitting and collapse of the high-density plasma blob. These results are helpful in understanding and identifying the magnetic reconnection phenomena possibly occurring near the heliospheric current sheets.     

“Oblique” Bernstein modes in solar preflare plasma: Generation of second harmonics

Process of second harmonics generation due to development of corresponding instability has been investigated for pure electron weakly oblique Bernstein mode. This mode was supposed to be modified by taking into account the influence of pair Coulomb collisions and weak large-scale electric field in flare loop. Investigated area was located near the loop foot-point in the “lower–middle” chromosphere of active region. It has been shown, that for the Fontenla–Avrett–Loeser model of solar atmosphere the investigated process of second harmonics generation starts at the extremely low threshold values of subdreicer electric field, well before the beginning of “preheating” phase of flare process.     

Distribution of electric current in solar plasma loops

The distributing profile of electric current in solar plasma loop is a key factor for the MHD instabilities of the loops. However, it is very difficult to measure such profile in single loop. In this paper, we assume that, in spite of the complexity of the structure in most of the sunspots, the distribution of the electric current in some small simple sunspots may reflect the main feature of the distribution in solar plasma loops. We utilize the high-cadence, high-resolution vector magnetograms observed by Big Bear Solar Observatory (BBSO) to derive the longitudinal electric current and analyze the distribution of the longitudinal electric current in the region of sunspots, and simulate the distributing features of the solar plasma loops. From these analysis, we find that the electric current in some small simple sunspots, or to say in plasma loops, are concentrated to their center. Such distribution feature is consistent with the theory of pinch effect in current-carrying plasma loops.