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.:...     

Phase coherence of foreshock MHD waves: wavelet analysis

The earth's foreshock is a region where particularly large amplitude MHD waves are commonly observed. They exhibit various waveforms, suggesting that nonlinear interaction between the waves is in progress. In a previous paper (Hada et al., 2003) we have introduced a method to quantitatively evaluate the strength of phase coherence among the waves from a given time series data. Here we further develop our method by applying wavelet filtering technique. From the analysis it was found that, although the turbulence is consisted of waves with a wide range of plasma rest frame frequencies, only those frequencies lower than the ion gyrofrequency are responsible for generating the phase coherence. This revised version was published online in August 2006 with corrections to the Cover Date.     

EFFECT OF THE RIBLETS SURFACE ON THE BOUNDARY LAYER DEVELOPMENT

ＥＦＦＥＣＴ　ＯＦ　ＴＨＥ　ＲＩＢＬＥＴＳ　ＳＵＲＦＡＣＥ　ＯＮ　ＴＨＥ　ＢＯＵＮＤＡＲＹ　ＬＡＹＥＲ　ＤＥＶＥＬＯＰＭＥＮＴＷａｎｇＪｉｎｊｕｎ；ＬａｎＳｈｉｌｏｎｇ；ＬｉａｎＱｉｘｉａｎｇ（ＩｎｓｔｉｔｕｔｅｏｆＦｌｕｉｄＭｅｃｈａｎｉｃｓＩＢｅ...     

利用微气囊扰动进行流动控制的数值模拟研究

探讨一种可以用来模拟“三角翼上分布微气囊，从而控制流动获得滚转力矩”的数值方法。为微型飞机的气动设计提供一种工具。研究的内容包括：考虑微气囊的三角翼网格生成、流场NS方程计算、微气囊不同布局对流动的扰动等。     

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.     

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。     

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。     

高超声速钝楔边界层转捩大涡模拟

 以五阶迎风和八阶对称格式混合差分格式求解三维可压缩滤波Navier-Stokes方程，对来流Mach数为6.0、半锥角5°的高超声速空间发展钝楔边界层转捩至完全湍流进行了大涡模拟。时间推进采用紧致存储三阶Runge-Kutta方法，亚格子尺度模型为Driest因子修正的Smagorinsky涡黏性模型。通过定常流场入口边界附近吹／吸引入不稳定扰动斜波的方法数值模拟得到了层流失稳转捩直至完全湍流的空间发展全过程。对扰动的线性、非线性增长以及湍流斑的形成和发展进行了分析，给出了转捩及完全湍流下的速度相关量统计并与实验、DNS结果进行了对比分析，计算结果与理论及实验吻合。     

飞行器完全非定常气动力的一种工程计算方法

本文以谐振运动非定常气动力计算理论为基础,采用偶极子格网技术进行数值计算、有理式拟合、Fourier积分和Duhamel积分等步骤,给出了飞行器任意运动和受任意大气扰动时完全非定常气动力的一种工程计算方法。该方法数学处理方便,得到的气动力表达式简单。算例结果表明:该完全非定常气动力计算方法可行,精度令人满意,具有工程实际意义。     

轴对称湍流射流的相似解

本文在相似性条件下,得到了用k-ε模式的轴对称湍流射流的相似方程。利用动量相似方程的近似求解结果作为初值,同时引入变量变换,进行迭代求解。本文的方法收敛速度快,计算简便。