相对论性离子束（环束）流引起的电磁不稳定性

在相对论性框架下，研究了冷离子流产生的右旋共振模，非共振模电磁不稳定性的特征结果表明，非共振模不稳定性增长率受离子流初始参数影响较大，而右旋共振模的增长率则受离子流初始参数影响较小。此结果可应用于太阳高能离子流通过低日冕区和地球磁层辐射带俘获的高能质子情形。     

The evolution of mirror type magnetic fluctuations in the magnetosheath based on multipoint observations

Two orbits were selected in January–February 2006 when the separation between the Cluster spacecraft was large and mirror type magnetic field fluctuations were observed by all spacecraft in different regions of the terrestrial magnetosheath. Minimum variance analysis was applied to find the mirror type fluctuations, and the amplitude of the fluctuations was determined individually. Mirror mode structures are moving along the streamlines frozen in the plasma. A model was developed for the calculation of plasma flowtime from the bow shock to the observation point. The growth rate of the field strength perturbations was estimated by comparing the amplitudes of fluctuations observed simultaneously at distant locations (∼10,000 km) based on the assumption that δB ∼ exp(γt). The obtained growth rate values were about an order of magnitude smaller than those provided by linear models and they decreased in the inner regions of the magnetosheath, indicating some saturation in the growth of the waves when proceeding towards the magnetopause. The results of these two case studies suggest that mirror type fluctuations originate from the compression region downstream of the quasi-perpendicular bow shock, and the growth of the fluctuations cannot be described by linear approximations.     

Cluster observations showing the indication of the formation of a modified-two-stream instability in the geomagnetic tail

This study presents several observations of the Cluster spacecraft on September 24, 2003 around 15:10 UT, which show necessary prerequisites and consequences for the formation of the so-called modified-two-stream instability (MTSI). Theoretical studies suggest that the plasma is MTSI unstable if (1) a relative drift of electrons and ions is present, which exceeds the Alfvèn speed, and (2) this relative drift or current is in the cross-field direction. As consequences of the formation of a MTSI one expects to observe (1) a field-aligned electron beam, (2) heating of the plasma, and (3) an enhancement in the B-wave spectrum at frequencies in the range of the lower-hybrid-frequency (LHF). In this study we use prime parameter data of the CIS and PEACE instruments onboard the Cluster spacecraft to verify the drift velocities of ions and electrons, FGM data to calculate the expected LHF and Alfvèn velocity, and the direction of the current. The B-wave spectrum is recorded by the STAFF instrument of Cluster. Finally, a field aligned beam of electrons is observed by 3D measurements of the IES instrument of the RAPID unit. Observations are verified using a theoretical model showing the build-up of a MTSI under the given circumstances.     

POD和DMD方法分析不同间隙压气机旋转不稳定性特性

对一台单级低速轴流压气机旋转不稳定性(RI)进行分析。在前期的旋转不稳定性特性、流场成因和不同间隙影响的研究基础上,进一步基于全通道数值模拟,采用两种流场降阶方法分析不同叶顶间隙条件下旋转不稳定性各阶模态对应的流场成分、模态能量占比和稳定性等特性。计算结果表明,前几阶模态能量占比大,对流场起主要贡献,并且稳定性相对较强。随着间隙的减小,旋转不稳定性的能量占比和稳定性下降,各阶的叶片转动成为流场的主要成分。      

Shock Wave Interaction with the Magnetopause

The magnetopause is in continuous motion and shock waves and impulsive acceleration events can occur. As an example, we show that the interaction of an interplanetary shock with the bow shock can generate a shock wave that after passing through the magnetosheath can interact with the magnetopause. In fluid dynamics, when a shock wave encounters a fluid discontinuity, the interface may become unstable and form bubbles and spikes. We consider this Richtmyer-Meshkov instability in magnetohydrodynamics. At the dayside magnetopause, the instability tends to be stabilized by the magnetic field. However, the shock wave interaction can initiate magnetic field reconnection for the southward IMF, which may be important in strong interplanetary shock events. This revised version was published online in August 2006 with corrections to the Cover Date.     

绝对不稳定性理论在尾流稳定性分析方面的研究

介绍了绝对／对流不稳定性的理论框架，并应用于钝体尾流剪切层的稳定性分析研究中。钝体尾流可以认为是局部平行流，而局部平行流的稳定性分析可以归结为Ｏｒｒ－Ｓｏｍｍｅｒｆｅｌｄ方程的求解。Ｏ－Ｓ方程求解化为一个复广义矩阵问题ＡＸ＝ωＢＸ，并分别约化Ａ，Ｂ为上Ｈｅｓｓｅｎｂｅｒｇ阵和上三角阵，通过Ｃｈｅｂｙｓｈｅｖ配置法可以求出特征值。最后对于Ｇａｕｓｓ尾流计算模型，给出了其在不同Ｒｅｙｎｏｌｄｓ下，流动     

剪切层与边界层组合流动的线性不稳定性分析

对不可压缩剪切层与边界层的组合流动完成了线性稳定性研究.组合流动的数学模型为Blasius边界层相似解与双曲正切函数的叠加,采用整体数值方法求解组合流动的稳定性方程,并验证了程序的准确性及网格无关性.研究给出组合流动的不稳定模态的辨识,即边界层模态和剪切层模态.在此基础上研究了剪切层对边界层模态不稳定性的影响以及壁面对剪切层模态的影响.由于剪切层的存在,使边界层模态中性曲线向左上方平移,临界雷诺数减小.此外,边界层模态不稳定性得到增强或抑制的影响,取决于扰动频率以及剪切层速度比的变化.组合流动中壁面边界层促使剪切层不稳定性减弱,主要表现在低频区域;而在高频区域,剪切层不稳定性几乎不受壁面边界层的影响.      

基于经验模态分解的燃烧不稳定性分析

实验研究了在常温常压条件下贫燃预混旋流火焰的燃烧不稳定性,发生燃烧不稳定性时其压力脉动表现为非平稳信号.利用一种基于经验模态分解(EMD)的希尔伯特-黄变换(HHT)算法对在当量比分别为0.71和0.80工况下的压力脉动信号进行了时频分析.针对压力脉动信号进行经验模态分解,选取主要的固有模态函数(IMF),对IMF通过HHT变换得到瞬时频率并进行统计分析.结果表明:在当量比为0.71时,压力信号呈间歇式的脉动,其振型为拍振;在当量比为0.80时,脉动压力信号则呈现出极限环振型.在基于EMD的HHT变换中,IMF体现了燃烧不稳定性的固有模态且具有自适应性强的特点.      

用自由空间法测量材料复介电常数的研究

分析电磁波在自由空间通过平板电介质材料的传播特性,得到了散射参数与复介电常数之间的关系式和求解复介电常数的三种表达式,并对三种表达式分别进行误差分析.解决自由空间法测量电介质材料复介电常数的不稳定性问题和相位模糊性问题.建立测试系统,并在X波段对平板电介质材料进行测量.实验结果表明,本测试方法和测试系统是正确的.     

空腔倾向对泄漏影响的流动分析

给出了前倾斜腔，矩形空腔和后倾斜腔三种结构的四空腔迷密封实验结果。通过数值求解非定常Ｎ－Ｓ方程，预测上述三种结构的单空腔迷宫通道的内部流动，计算结果表明：后倾斜腔结构内部是稳态流动，而对于前斜腔和矩形空腔结构，流动表现为总体结构的基本稳定和局部结构的不稳定，局部不稳定的强弱顺序依次是前倾斜腔，矩形腔和后倾斜腔的迷宫结构。通过分析局部结构不稳定对减小泄漏的作用机制，说明不稳定效应的强弱是造成密封效果