Theoretical properties of offset bipolar electric field solitary structures in space plasmas

The bipolar electric field solitary (EFS) structures have been frequently observed in the near Earth plasma regions, such as auroral zone, magnetopause, cusp regions, and magneto-tail. Sometimes these structures are observed as offset bipolar structures. In this paper, the properties of the offset bipolar EFS structures parallel to the magnetic field are studied with an ion fluid model in a cylindrical symmetry by considering electrostatic condition. The model results show that the offset bipolar EFS structures can develop from both ion-acoustic waves and ion cyclotron waves, and propagate along the magnetic field line in the space plasmas if plasma satisfies some conditions. The offset bipolar EFS structures can have both polarities. It will be first negative pulse and then positive pulse if the initial electric field E₀ < 0 or reverse in order if E₀ > 0. The amplitude of the offset bipolar EFS structures first decreases and then increases with the wave propagation velocity. Some results from our model are consistent with the observations.     

Response of the mid-latitude D-region ionosphere to the total solar eclipse of 22 July 2009 studied using VLF signals in South Korean peninsula

In this paper, we analyze VLF signals received at Busan to study the the D-region changes linked with the solar eclipse event of 22 July 2009 for very short (∼390 km) transmitter–receiver great circle path (TRGCP) during local noon time 00:36–03:13 UT (09:36–12:13 KST). The eclipse crossed south of Busan with a maximum obscuration of ∼84%. Observations clearly show a reduction of ∼6.2 dB in the VLF signal strength at the time of maximum solar obscuration (84% at 01:53 UT) as compared to those observed on the control days. Estimated values of change in Wait ionospheric parameters: reflection height (h′) in km and inverse scale height parameter (β) in km⁻¹ from Long Wave Propagation Capability (LWPC) model during the maximum eclipse phase as compared to unperturbed ionosphere are 7 km and 0.055 km⁻¹, respectively. Moreover, the D-region electron density estimated from model computation shows 95% depletion in electron density at the height of ∼71 km. The reflection height is found to increase by ∼7 km in the D-region during the eclipse as compared to those on the control days, implying a depletion in the Lyman-α flux by a factor of ∼7. The present observations are discussed in the light of current understanding on the solar eclipse induced D-region dynamics.     

超短波电台自动检测与故障诊断系统设计

介绍了超短波电台自动检测系统与故障诊断系统的功能,并根据功能要求进行了硬件电路的设计,采取面向信号的ATLAS语言进行软件设计和建立在专家知识输入故障推理模型.该系统经使用证明,检测结果精确,检测效率较高.     

时频分析在超声导波信号分析中的应用

超声导波信号是一种非平稳信号,存在频散现象,利用传统的时域和频域分析方法不能揭示其频谱随时间变化的特点.为了解决这一问题,研究了导波信号的非平稳特征,介绍了短时傅里叶变换(STFT,Short-Time Fourier Transform)时频分析原理,分别对铝板试样和蜂窝板试样内传播的导波信号进行了STFT和时频谱分析,得出了铝板内导波信号中各频率成分随时间的变化情况,分析出导波信号的模式转换现象,比较精确地计算了导波的群速度;对于蜂窝板内的导波信号,由于能量泄露比较严重,当激励频率为1.5MHz时,A0模式只能近距离传播,这就使得采用STFT不能很好地进行模式识别.研究结果表明,当导波传播距离较远时,利用STFT可以对其信号进行动态的频谱分析和模式识别,并可对实际的群速度进行较精确的测量.     

自适应滤波方法研究

证明Ｓａｇｅ－Ｈｕｓａ的自适应卡尔曼滤波算法不能同时估计Ｑ和Ｒ,并分析了该法导致滤波发散的原因。介绍了一种新的自适应卡尔曼滤波算法,该法当Ｒ（或Ｑ）已知时可以准确地估计出Ｑ（或Ｒ）。该法的独特之处在于当对Ｑ（或Ｒ）进行修正估计时,只采用矩阵的乘运算和求逆运算,而不进行加减法运算,因此消除了滤波发散现象。数字仿真表明效果良好。     

损失锥电子速度分布激发的哨声波

利用一维粒子模拟方法研究了损失锥电子速度分布激发的哨声波非线性演化过程, 并与双麦克斯韦电子分布激发哨声波的情况进行了比较. 结果表明, 这两种情况下, 在线性增长阶段哨声波的主导频率 (能量最集中的一个频率) 是一样的, 波动的激发使得平行于背景磁场方向的电子温度有所提高. 比较而言,在损失锥分布情况下, 哨声波具有主导频率的波模可较早地被激发, 而在线性增长阶段, 哨声波的能量更倾向于集中在高频(短波长)波段. 部分粒子被散射到损失锥中, 而使损失锥分布得以补充. 本文还研究了不同各向异性分布和磁场强度条件下的激发过程.      

Design and optimization of supersonic turbines for detonation combustors

Detonation-based engines offer a potential surge in efficiency for compact thermal power systems. However, these cycles require ad-hoc components adapted to the high outlet velocity from the detonation combustors. This paper presents the design methodology of turbine stages suitable for supersonic inlet conditions and provides a detailed analysis of optimized turbine geometries. A reduced-order solver examines the supersonic blade rows’ functional design space, quantifies the turbine’s non-isent...     

准定常强激波马赫反射波形的数值研究

应用DCD频散控制激波捕捉格式,求解二维、多组分、带有化学反应的Euler方程组,数值模拟了准定常强激波的马赫反射问题.研究结果表明:与经典马赫反射理论相比,在强激波条件下,激波诱导的气体分子振动激发和化学反应使马赫反射的三波点轨迹角变小、马赫杆高度变低、楔顶附体激波倾角变小;马赫杆的相对突出量随入射激波马赫数和楔角的增大而增大,而气体分子的振动、离解等真实气体效应能进一步加剧马赫杆的向前突出.     

运动激波绕射过程中的粘性效应

应用 TVD格式求解二维非定常全 N- S方程 ,以研究运动激波绕射现象。考虑粘性后 ,绕凹角流动时 ,压缩拐角附近表面压力分布与实验结果更为符合 ;绕凸起物时 ,出现反射激波因边界层干扰根部加宽 ,前、后角点附近有局部分离与再附 ,并引起局部压力上升 (与无粘流场模拟相比 )等现象。结果表明 ,全 N- S方程可较好地模拟实际粘性流中复杂激波障碍物干扰流场特性