Wave-Particle-Electric Field Synergetic Auroral Electron Acceleration

Space Science Reviews - We discuss afresh the problem of the auroral electron acceleration based on the controversy reports of Bryant, D. A. et al.: 1992, Phys. Rev. Lett. 68, 37, and Borovsky, J.:...     

Solar and Heliospheric Modulation of Galactic Cosmic Rays

The significance of external influences on the environment of Earth and its atmosphere has become evident during recent years. Especially, on time scales of several hundred years, the cosmogenic isotope concentration during the Wolf-, Spoerer-, Maunder- and Dalton-Minimum indicates an increased cosmic ray flux. Because these grand minima of solar activity coincide with cold periods, a correlation of the Earth climate with the cosmic ray intensities is plausible. Any quantitative study of the effects of energetic particles on the atmosphere and environment of the Earth must address their transport to Earth and their interactions with the Earth’s atmosphere including their filtering by the terrestrial magnetosphere. The first problem is one of the fundamental problems in modern cosmic ray astrophysics, and corresponding studies began in the 1960s based on Parker’s cosmic ray modulation theory taking into account diffusion, convection, adiabatic deceleration, and (later) the drift of energetic particles in the global heliospheric magnetic field. It is well established that all of these processes determining the modulation of cosmic rays are depending on parameters that are varying with the solar magnetic cycle. Therefore, the galactic cosmic ray intensities close to Earth is the result of a complex modulation of the interstellar galactic spectrum within the heliosphere. The modern view of this cosmic ray modulation is summarized in our contribution.     

Phase coherence of MHD waves in the solar wind

Large amplitude MHD waves are commonly found in the solar wind. Nonlinear interactions between the MHD waves are likely to produce finite correlation among the wave phases. For discussions of various transport processes of energetic particles, it is fundamentally important to determine whether the wave phases are randomly distributed (as assumed in quasi-linear theories) or they have a finite coherence. Using a method based on a surrogate data technique and a fractal analysis, we analyzed Geotail magnetic field data (provided by S. Kokubun and T. Nagai through DARTS at the Institute of Space and Astronautical Science) to evaluate the phase coherence among the MHD waves in the earth's foreshock region. The correlation of wave phases does exist, indicating that the nonlinear interactions between the waves is in progress. This revised version was published online in August 2006 with corrections to the Cover Date.     

正—反激组合式变换器与单端式变换器的比较

以５０Ｗ变换器为例，分别从磁性元件的大小，功率管上的电应力、磁恢复问题，输出纹波及输出特性等方面，详细分析比较了组合式变换器与单端式变换器的优缺点，并给出了具体数据，提出了正－反激组合式变换器具有电压应力低，磁性元件小，体积小，重量轻，输出纹波小及可靠性高的结论。     

二维通道内湍流边界层分离的实验研究

用激光多普勒技术测量了二维扩压器中不可压湍流边界层分离流动，得到了时均速度和雷诺剪应力分布。实验结果分析表明：以Ｃｏｌｅｓ速度律发展的Ｂａｒｄｉｎａ速度分布可以描述瞬时间歇分离点以前和瞬时间歇再附点以后的时均速度分布，但无法描述分离区的边界层速度型。Ｃｒｏｓｓ速度分布可描述分离区的边界层速度分布。Ｃｅｂｅｃｉ＆Ｓｍｉｔｈ涡粘性代数模型难以正确地描述分离边界层的雷诺剪应力。     

镀膜光纤声光相位调制器频率响应特性的研究

本文对光纤声光相位调制器（OF—AOPM）的频率特性进行研究。分析了OF—AOPM的调相原理，研究结果表明：在调制频率远离氧化锌压电薄膜的半波谐振频率的时候，光相位的调制不仅依靠径向应力。同时还依靠轴向应力。通过同时考虑径向和轴向应力的变化，得出了OF—AOPM在整个频率域范围内的响应特性。     

基于FM-AM转换的伪码调相-载波调频复合引信信号的脉内特征提取研究

伪码调相和载波调频复合信号因具有好的距离、速度分辨率和测速测距精度,所以广泛应用在雷达和引信中。在电子对抗中为了实施欺骗性干扰,必须有效地提取复合信号的参数特征,为此本文研究了FM-AM转换时频分析的理论及其实现方法,并利用该方法对伪码调相-载波调频复合信号进行了脉内特征分析。具体包括伪码调相正弦载波信号、伪码调相复合正弦调频信号及伪码调相复合线性调频信号。仿真结果表明,在信噪比为5dB时,利用FM-AM转换时频分析技术,不但可以提取载波调频的特征信息,而且能够有效提取伪码的特征信息。     

伪码调相与PAM复合测距系统研究

介绍了PAM伪随机码的构成原理,推导了PAM伪随机码的自相关函数和功率谱密度。结合图形分析了它们的性质特点。设计了伪码调相与PAM复合测距系统,并分析了在加性高斯白噪声信道中的各个阶段的信号形式。研究了复合测距系统的性能,详细推导了复合测距系统的信噪比增益。结果表明,与单纯的伪码测距系统相比,复合测距系统有更强的抗干扰性能和测距能力。     

谐振腔光纤陀螺频率调制原理及仿真

简述对谐振腔光纤陀螺入射光进行频率调制的基本方法，采用洛仑兹公式来描述光纤陀螺的传递函数，结合输入信号特征，建立其频域的数学模型，最后给出结果和相关仿真图形，以及关键参数的优化值和优化方向，再对全光路的结构提出具体的配置建议，仿真结果表明，谐振腔光纤陀螺具有良好的线性工作区间，精度也能够得到进一步的提高。     

轴对称降落伞稳定下降阶段的流场特性

文章根据降落伞的特点,通过3点假设(伞衣的薄膜假设、降落伞的轴对称假设和流场的定常 假设),将三维复杂流动问题,转化成二维轴对称问题,以节约计算时间。然后,建立轴对称降落伞的流体力 学计算模型,利用数值模拟手段,求解RNG(Renormalization Group)k-epsilon湍流模型下的N—S方程组,获 得与有关单位试验相吻合的计算结果。分析发现带顶孔的轴对称降落伞绕流和亚临界状态下带中心孔的 圆球绕流,在尾流区拓扑结构上几乎完全一致。结果表明建立的轴对称降落伞模型,能够揭示降落伞流场 的本质特性,为进一步研究降落伞流场的流动机理和流固耦合问题打下基础。