局部涂敷RAM复杂目标的电磁散射特性计算

给出了平行和垂直极化平面波投射到物体时散射场的通用表达式,阐述了确定目标主要回波源位置的方法,提出选取吸波材料涂敷区域的有效方法,同时分析了局部涂敷吸波材料(RAM)的复杂目标电磁散射特性的计算,最后给出计算结果,并经验证.这种方法提高了复杂目标雷达散射截面计算的精度,适用于工程应用.     

正丁醇/煤油混合物非预混燃烧压力振荡特性

为探索生物混合燃料在燃气轮机燃烧室内的应用,将丁醇掺混入航空煤油中,根据燃烧室的实验结果构建熵波对流模型,定量分析其不同体积分数对燃烧室内压力振荡频率的影响。实验结果表明:在燃烧室进口压力1.98 MPa、温度600 K和油气比0.03下,随着丁醇所占体积分数增大,燃烧室内压力振荡频率逐渐下降,而幅值变化无明显规律。熵波对流模型结果与实验吻合较好,通过分析表明,不同燃料组分热值变化引起的对流时间改变,是燃烧室压力振荡频率变化的主要原因,为控制燃烧室内压力振荡提供了参考。      

大功率无线电波加热低电离层

等离子体对大功率电波的欧姆耗散会使电子温度升高,进而导致电子密度和其他等离子体参数改变,实现电离层的地面人工变态.本文基于大功率无线电波与低电离层相互作用的自洽模型,分析了不同入射条件下电离层参数的变化,主要结论如下:电离层D区是电波的主要吸收区,并且其吸收强度随入射频率的升高而降低,当入射频率为6 MHz（有效入射功率为200 MW）时电子温度的最大增幅约为520 K,电子密度最大增幅为7300 cm^-3左右;电子温度达到饱和所需时间小于电子密度的饱和时间,前者具有μs量级,后者具有ms量级;停止加热后,电子温度和密度迅速恢复到初始状态,恢复时间均小于各自的饱和时间,但量级相当;入射功率越高,电子温度和密度的增幅越大,并且饱和时间也越长,在相同入射条件下,夜晚的饱和时间要大于白天.     

Heating heavy ions in the polar corona by collisionless shocks: A one-dimensional simulation

Recently a new model for explaining the observations of preferential heating of heavy ions in the polar solar corona was proposed ( and ). In that model the ion energization mechanism is the ion reflection off supercritical quasi-perpendicular collisionless shocks in the corona and the subsequent acceleration by the motional electric field E = −V × B/c. The mechanism of heavy ion reflection is based on ion gyration in the magnetic overshoot of the shock. The acceleration due to the motional electric field is perpendicular to the magnetic field, giving rise to large temperature anisotropy with T_⊥ ? T_∥, in agreement with SoHO observations. Such a model is tested here by means of a one dimensional test particle simulation where ions are launched toward electric and magnetic profiles representing the shock transition. We study the dynamics of O⁵⁺, as representative of coronal heavy ions for Alfvénic Mach numbers of 2–4, as appropriate to solar corona. It is found that O⁵⁺ ions are easily reflected and gain more than mass proportional energy with respect to protons.     

航空发动机风扇机匣行波振动的分析方法

本文提出对风扇机匣应进行行波振动分析, 作出频率响应曲线, 进行限幅设计。在分析过程中, 根据结构特点给出了模型的简化方法, 采取周期对称模型, 并根据周期对称的理论结合激振力的特点给出了旋转脉动激励在周期对称模块中的施加方法。      

Aeroelastic stability analysis of heated flexible panel subjected to an oblique shock

The critical conditions for aeroelastic stability and the stability boundaries of a flexible two-dimensional heated panel subjected to an impinging oblique shock are considered using theoretical analysis and numerical computations, respectively. The von-Karman large deflection theory of isotropic flat plates is used to account for the geometrical nonlinearity of the heated panel, and local first-order piston theory is employed in the region before and after shock waves to estimate the aerodynamic pressure. The coupled partial differential governing equations, according to the Hamilton principle, are established with thermal effect based on quasi-steady thermal stress theory. The Galerkin discrete method is employed to truncate the partial differential equations into a set of ordinary differential equations, which are then solved by the fourth-order Runge-Kutta numerical integration method. Lyapunov indirect method is applied to evaluate the stability of the heated panel. The results show that a new aeroelastic instability (distinct from regular panel flutter) arises from the complex interaction of the incident and reflected wave system with the panel flexural modes and thermal loads. What’s more, stability of the panel is reduced in the presence of the oblique shock. In other words, the heated panel becomes aeroelastically unstable at relatively small flight aerodynamic pressure.     

HIGH ORDER ACCURACY SCHEME FOR 2-D TRANSONIC FLOWS

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TYPES OF FLOW OVER LEESIDE OF A SLENDER TAPERED WING AT SUPERSONIC SPEED

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Some Observational Evidence of Alfven Surface Waves Induced Magnetic Reconnection

The surface wave induced magnetic reconnection (SWIMR) model based on Alfven Resonance theory will be discussed briefly both for collisional and collisionless plasmas. It is shown that the spatial scales and time delays associated with Flux Transfer Events and Pulsed Ionospheric Flows, as observed by satellites and SuperDARN radars and the magnetic bubbles, observed at the high latitude boundary of the magnetopause, can be explained by the SWIMR model. This revised version was published online in August 2006 with corrections to the Cover Date.     

Recent Developments in Magnetospheric Diagnostics Using ULF Waves

One of the most ubiquitous indicators of the state and topology of the magnetosphere are ultra-low frequency (ULF) waves. These may be continuously and inexpensively monitored from the ground using networks of magnetometers. The most robust measurable quantity provided by magnetometer networks is signal phase and this paper emphasizes the usefulness of this parameter in a variety of ULF wave diagnostic processes ranging from equatorial to high latitudes. This revised version was published online in August 2006 with corrections to the Cover Date.