基于DIS的空战仿真系统的应用实现

针对现代高技术条件下航空武器系统作战效能评估在任务与功能上的客观需求,基于分布交互仿真的设计思想,进行了空战仿真系统的实现方案研究.提出了方案的体系结构和功能划分,介绍了其中所涉及的若干关键技术,并分析了在一个虚拟作战环境下利用该系统开展的有关空战仿真的相关实验研究.仿真结果表明,较之传统的飞机作战效能评估方法,新系统在拓展仿真的内容与规模,增强仿真的逼真感和可信度等方面都显示出其独特的优势和良好的应用前景.     

Force-free magnetic field in a cylindrical flux rope without a constant alpha

It is generally assumed that magnetic fields inside interplanetary magnetic clouds and flux ropes in the solar photosphere are force-free. In order to model such fields, the solution of rot B = B is commonly used where  = const. But comparisons of this solutions with observations show significant difference. To treat this problem,we examine the solutions with .     

Coronal streamers' theories

Some theoretical aspects of solar coronal streamers are discussed with emphasis on the current sheet and reconnection processes going on along the axis of the streamer. The dynamics of the streamer is a combination of MHD and transport, with acceleration of particles due to reconnection and leakage of plasma outwards as a slow solar wind as the observable results. The presence of the almost-closed magnetic bottles of streamers that can store high-energy particles for significant times provides the birdcage for solar cosmic rays, the reconnection in the sheet feeds medium-energy protons into the corona for the large-scale storage needed for certain flare models, and the build-up of excess density sets the stage for coronal mass ejections.     

DSP在电机控制中的应用

本文阐述了DSP（TMS320C240）的基本结构，指出该DSP计算速度快，具有PWM波形发生器等特点，并将DSP芯片应用于电机的矢量控制系统中，同时给出了控制系统的软件及硬件设计图。     

某舰飞行甲板区域流场特性的水洞试验

为了满足舰载直升机的需要，南航直升机技术研究所对某舰飞行甲板区域流场进行了水洞试验。本文详述了水洞试验的方法和技术，通过对舰模在各种水速、各种航行偏角状态下的试验，得到了大量照片，并据此对该舰机库后部、飞行甲板上部周围流场进行了分析，得出了在飞行甲板机库门外有一趋于收缩的稳态区，随着流速Ｖ的增大，这一区域变短。稳态区之后很快变为乱流区。从侧面上看，稳态区高度有从降低再向上扩散的趋向。在向右偏航时，     

扇面波导宽面横缝的等效参量

给出扇面波导ＴＥ模式场分量的近似表达式，根据等效原理，应用矩量法求解了扇面波导宽面窄横缝口面电场的分布，研究了散射参数，归一化等效串联阻抗，谐振电阻，谐振长度等重要参数。     

Global characteristics of ionospheric electric fields and disturbances during the first hours of magnetic storms

The ionospheric plasma density can be significantly disturbed during magnetic storms. In the conventional scenario of ionospheric storms, the negative storm phases with plasma density decreases are caused by neutral composition changes, and the positive storm phases with plasma density increases are often related to atmospheric gravity waves. However, recent studies show that the global redistribution of the ionospheric plasma is dominated primarily by electric fields during the first hours of magnetic storms. In this paper, we present the measurements of ionospheric disturbances by the DMSP satellites and GPS network during the magnetic storm on 6 April 2000. The DMSP measurements include the F region ion velocity and density at the altitude of ∼840 km, and the GPS receiver network provides total electron content (TEC) measurements. The storm-time ionospheric disturbances show the following characteristics. The plasma density is deeply depleted in a latitudinal range of ∼20° over the equatorial region in the evening sector, and the depletions represent plasma bubbles. The ionospheric plasma density at middle latitudes (20°–40° magnetic latitudes) is significantly increased. The dayside TEC is increased simultaneously over a large latitudinal range. An enhanced TEC band forms in the afternoon sector, goes through the cusp region, and enters the polar cap. All the observed ionospheric disturbances occur within 1–5 h from the storm sudden commencement. The observations suggest that penetration electric fields play a major role in the rapid generation of equatorial plasma bubbles and the simultaneous increases of the dayside TEC within the first 2 h during the storm main phase. The ionospheric disturbances at later times may be caused by the combination of penetration electric fields and neutral wind dynamo process.     

Stochastic particle acceleration by the forced interaction of relativistic current sheets

We address the problem of interacting relativistic current sheets in self-consistent kinetic plasma simulations within the framework of the Particle-In-Cell model. The interaction is enforced in head-on collisions of up to 10 current sheets at relativistic bulk speeds. The simulations are motivated by the general problem of Poynting flux dissipation in ‘striped wind’ configurations presumably governing the relativistic outflows pervasive in pulsar winds and gamma-ray bursts. We identify the generation of non-thermal particles and formation of a stable power-law shape in the particle energy distributions f(γ) dγ ∝ γ^−s dγ. In 1D, a spectral index s ∼ 2 is observed and attributed to a stochastic Fermi-type acceleration mechanism. In 2D, the generic index of s ∼ 3–4 is retained as in previous simulations of individual current sheets. Whereas in 2D the high energy cut-off is constrained by the limited dissipation of magnetic energy, in 1D the process converts the bulk motion of current sheets towards directed particle momentum of an exclusive class of non-thermal particles.     

空间电推进技术应用现状与发展趋势

电推进技术是近年来空间推进领域发展和应用最为活跃的专业技术。文章阐述了电推进在航天器上应用的优势与问题,电推进应用于航天器可带来节省推进剂、提高姿控精度、扩展深空探测距离等优势,同时需要关注带来的表面电位变化、荷能粒子影响、电磁干扰等问题。目前,电推进已经广泛应用于GEO及低轨卫星、深空探测器等航天器上,并且电推进正逐步向更大功率、超高比冲、更多模式、更低成本等方向发展。建议我国加大需求牵引,夯实基础理论,尽快开展多种电推进空间飞行,并不断培育新型电推进技术,占领未来电推进技术制高点。     

利用奇异辛几何构作新的带仲裁的认证码

利用有限域上奇异辛几何构造了一个新的带仲裁的认证码，并计算了这个码的参数。当收方和发方的编码规则按等概率分布选取时，计算出了各种攻击成功的概率。