Study of VLF wave with relativistic effect in Saturn magnetosphere in the presence of parallel A.C. electric field

Cassini radio and plasma wave surveys aim to study radio emissions, plasma waves, thermal plasma and dust near Saturn. Using the characteristic solution and dynamics method, the influence of electron beam on the loss cone and bi-Maxwellian distribution of whistler mode waves in the parallel alternating electric field and magnetic field is studied. The dispersion relation and the growth rate of Saturn's magnetic layer were deduced and calculated in detail. Parameter analysis is performed by changing the parameters of the plasma like number density, AC frequency, temperature anisotropy, etc. The influence of AC frequency on Doppler shift and the comparative study of growth rate of oblique and parallel propagating waves are analyzed using generalized distribution function. We found temperature anisotropy ${\text{A}}_{\text{T}}=1.25$ can explain the linear spatiotemporal growth rate of whistler mode waves. It provides the majority of the observed frequency integral power. It can be seen that the effective parameters for the generation of Whistler mode waves are not only temperature anisotropy, but also the relativistic factors discussed in the results and discussion section, and the AC field frequency and width of the loss cone distribution function.     

高海况下反舰导弹对舰船目标攻击策略

反舰导弹攻击海面舰船目标时,通常根据目标的散射特征数据进行目标类型判定并做出决策。但是在高海况下:如果导弹横浪飞行,海浪对导弹命中目标的影响会变小,基本能保证可靠命中目标;但如果导弹顶浪飞行,则海浪会引起目标雷达反射截面积(Radar Cross Section,RCS)的起伏甚至突变,影响导弹对目标的锁定和判断。文章建立了不同海况和舰船目标的融合模型,并针对融合模型仿真计算了导弹不同突击方向时的 RCS,最终根据高海况时舰船横浪或顶浪航行的原则,按照捕捉概率最大的方向确定导弹的攻击方向。     

基于不相干平面波叠加以模拟混响声场的航天器低频声固耦合分析

文章针对航天器在混响声场中的随机振动问题,提出一种通过多个不相干的平面波线性叠加以模拟混响声场的实现方法,给出了每个平面波的具体参数并从理论上证明其满足理想混响声场假设。在此基础上利用有限元-边界元耦合方法对整星低频声固耦合问题进行分析,并用混响室噪声试验响应数据进行了验证。研究结果表明:该方法理论推导正确,为航天器低频声固耦合分析及声振力学环境预示提供了一种新的有效手段。     

The radiation impedance of electrodynamic tethers in a polar Jovian orbit

Juno, the second mission in the NASA New Frontiers Program, will both be a polar Jovian orbiter, and use solar arrays for power, moving away from previous use of radioisotope power systems (RPSs) in spite of the weak solar light reaching Jupiter. The power generation at Jupiter is critical, and a conductive tether could be an alternative source of power. A current-carrying tether orbiting in a magnetized ionosphere/plasmasphere will radiate waves. A magnitude of interest for both power generation and signal emission is the wave impedance. Jupiter has the strongest magnetic field in the Solar Planetary System and its plasma density is low everywhere. This leads to an electron plasma frequency smaller than the electron cyclotron frequency, and a high Alfven velocity. Unlike the low Earth orbit (LEO) case, the electron skin depth and the characteristic size of plasma contactors affect the Alfven impedance.     

基于Lamb波与时频分析的复合材料结构损伤监测和识别

采用将Lamb波和时频分析相结合的方法,对碳纤维增强复合材料层板结构进行在线的连续监测。首先研究Lamb波在复合材料层板结构中的传播问题,利用Mindlin板理论建立了低阶反对称Lamb波在各向异性复合材料层板中随传播角变化的频散关系;然后用小波变换对由压电传感元件激励和接收的Lamb波信号在时频域进行分析,提取特征信息,测量出Lamb波在结构中实际传播的飞行时间和群速度,并与理论结果相比较;在此基础上结合理论与实际量测信息,考虑各向异性对Lamb波速度的影响,使用遗传算法确定损伤位置,并估算损伤尺寸。实验研究表明了本文方法的可应用性和有效性。     

数值模拟中的边界处理方法研究

为适应于模拟超声速流场中的一些特殊物理现象,研究了不同物理现象对边界处理的要求。针对激波、旋涡和声波等流场中典型的流动现象,采用常用的外推、特征和缓冲三类边界处理方法分别进行数值模拟。计算结果表明超声速流场边界采用外推技术,只适于计算带有激波的边界。特征方法还能适于旋涡运动的计算。声波的计算只能采用缓冲层技术。     

单激励直线行波超声马达定子振动特性研究

利用弹性动力学理论对半无限长弹性细长梁进行了分析,得出在弹性细长梁上激励出大振幅弯曲行波振动的条件,对以此为基础研制的直线超声行波马达的定子进行了振动特性分析,着重分析了行波反射对定子振动状态的影响,认为一般情况下定子上的振动是含有驻波场的行波,并对不同反射系数条件下的定子振动波形进行仿真,最后通过实验研究了驻波场对超声马达驱动特性的影响.      

大功率高频无线电波对赤道E区双流不稳定性的影响--PIC静电粒子模拟研究

地面入射的大功率高频无线电波(泵波)和电离层等离子体之间的参数相互作用，能够引起静电波的激发，在一定条件下，产生不稳定性．本文用PIC静电粒子模拟方法，研究泵波与赤道电离层E区等离子体的相互作用．研究结果表明，泵波能够控制双流不稳定性的发生，在不同条件下，泵波对双流不稳定性起着稳定与不稳作用，模拟结果定性地与理论研究结果相符合，这为我们对不规则体产生的地面人工控制提供了依据．     

行波液体静压轴承浮力及其稳定方法的实验研究

提出了一种基于蠕动传输作用的新型行波液体静压轴承。首先基于行波液体静压轴承原理,建立了轴承原理验证装置。然后基于差动螺纹机构建立了轴承面倾斜调整机构,实现轴承的完全上浮。利用所开发的轴承验证装置,实验研究了行波液体静压轴承在上浮方向上有导轨时的轴承承载能力,证明了行波液体静压轴承及其稳定方法的可行性,并给出了驱动参数,例如:驱动电压和驱动频率,以及轴承间隙高度对轴承浮力稳态值的影响规律。     

A study of a long duration B9 flare-CME event and associated shock

We present and discuss here the observations of a small long duration GOES B-class flare associated with a quiescent filament eruption, a global EUV wave and a CME on 2011 May 11. The event was well observed by the Solar Dynamics Observatory (SDO), GONG H$\alpha$, STEREO and Culgoora spectrograph. As the filament erupted, ahead of the filament we observed the propagation of EIT wave fronts, as well as two flare ribbons on both sides of the polarity inversion line (PIL) on the solar surface. The observations show the co-existence of two types of EUV waves, i.e., a fast and a slow one. A type II radio burst with up to the third harmonic component was also associated with this event. The evolution of photospheric magnetic field showed flux emergence and cancellation at the filament site before its eruption.