一种适合飞行仿真应用的非定常非线性旋翼尾迹增强模型

基于被广泛应用的Peters—He有限状态动态尾迹模型,本提出了一种增强的非线性、非定常的旋翼尾迹模型,并混合王氏涡流理论建立了旋翼尾迹的旋转分量计算模型(桨尖轨迹平面处)。将原来的线性动态入流理论改造为非线性理论模型,并取消了计算影响系数短阵中的小角度假设。增强后的诱导速度模型适合计算低速飞行状态下旋翼平面内诱导速度,理论计算结果和实验值吻合较好。经优化的FORTRAN程序在常规单CPH微机系统中即可实现实时计算。     

电磁力连续控制圆柱绕流态变化的研究

作用于电介质溶液流体边界层上的Lorentz电磁力可以改变流体边界层的结构,从而控制流体绕流的形态。通过理论分析和数值模拟确定了实验控制的关键参数,交替分布的电极和磁极包覆在圆柱体的表面置于电介质溶液中,简单调整电磁力的分布可以方便地控制圆柱尾迹的流动结构,实现了电磁力消涡和增涡的连续控制。     

背风涡隔离对大攻角旋成体表面压力分布的影响

通过在背风母线处沿纵向对称面嵌入隔离板，观测了大攻角旋成体在这种背风涡被隔离状态下的表面压力分布情况。隔离板的作用旨在削弱、隔阻两侧背风涡间的相互联系和诱导，以便考察背风涡诱导作用对物面流动的影响。不同隔离（包括无隔离情况）状态下的实验结果表明，背风涡的隔离对表面压力分布有不同程度的影响，故这一研究和结果可供探讨大攻角流动非对称性成因作参考。     

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.     

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。     

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.     

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。     

“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.