航空发动机双转子系统的拍振分析

 在双转子航空发动机中，由于转子系统不可避免地存在不平衡量，当两个转子的转速比较接近时，发动机会出现拍振现象，拍振将引起振动强度过大问题。对双转子系统的拍振进行了研究，分析了拍振的周期性、信号强度及其反向转子特性，阐明了拍振产生的机理和特征，并采用数值仿真和试验对拍振进行了定量分析和验证。研究表明，拍振与双转子转速差和不平衡量的相位因素有关，当转速差小于工作转速的20%时，双转子系统拍振信号的强度较大。     

大多普勒容限巴克码脉压

 本文介绍用补偿式非相干型旁瓣抑制滤波器(SSF)实现13位巴克码脉冲压缩旁瓣抑制的理论计算及实验结果。补偿式非相干型SSF采用最小二乘近似逆滤波方法设计,若子脉冲宽度为0.7μs,峰值旁瓣电平不超过-30dB,这种SSF的多普勒容限能达到-40kHz～+40kHz。理论计算及实验结果都表明,所设计的补偿式非相干型SSF的多普勒容限比具有同样长度冲激响应序列的R-G-ISSF有显著改善。     

Type II Solar Radio Bursts: Theory and Space Weather Implications

Recent data and theory for type II solar radio bursts are reviewed, focusing on a recent analytic quantitative theory for interplanetary type II bursts. The theory addresses electron reflection and acceleration at the type II shock, formation of electron beams in the foreshock, and generation of Langmuir waves and the type II radiation there. The theory's predictions as functions of the shock and plasma parameters are summarized and discussed in terms of space weather events. The theory is consistent with available data, has explanations for radio-loud/quiet coronal mass ejections (CMEs) and why type IIs are bursty, and can account for empirical correlations between type IIs, CMEs, and interplanetary disturbances. This revised version was published online in August 2006 with corrections to the Cover Date.     

典型几何和流动参数对高超声速进气道性能的影响

用N-S方程模拟了一系列典型二元高超声速进气道内压缩通道及隔离段模型,模拟发现内压缩通道及隔离段增压比、温升比和总压恢复系数等性能参数主要受面积收缩比、内压缩通道收缩角、隔离段长高比等几何参数以及内压缩通道进口马赫数、密度、附面层厚度等流动参数的影响。内收缩比和内收缩通道收缩角的增大都会使压缩增强;隔离段内沿程平均温升比、马赫数和总压恢复系数曲线则均接近平行直线。内压缩通道进口马赫数的增大也会使压缩增强,但较小的进口马赫数可能引起分离,进而增大增压比;而进口密度增大使附面层变薄,对气流的压缩减弱;进口附面层厚度对沿程平均温升比、增压比以及马赫数的影响近似线性。     

三维编织复合材料圆柱壳轴压下的屈曲分析

根据边界层理论,采用奇异摄动法,考虑非线性前屈曲、大挠度和初始几何缺陷的影响,分析在固支条件下,三维四向编织复合材料圆柱壳在轴压下的屈曲和后屈曲性态,讨论了纤维体积含量、几何参数等因素对圆柱壳屈曲的影响.结果表明,纤维体积含量、编织角和初始缺陷对编织复合材料圆柱壳的影响是不可忽视的.     

圆环压缩的刚塑性有限元分析与应用

本文采用刚塑性有限元法分析圆环压缩,并与上限法分析和试验结果进行比较。结果表明,采用这种方法可以计算标定曲线,计算各种润滑剂的摩擦因素和压缩状态下材料的应力应变曲线,模拟圆环的变形和摩擦面的正压力分布。 本文还通过试验,求得四种高温润滑的摩擦因素和Ti-6Al-4V在不同条件下的应力应变曲线。     

极区中层惯性重力波VHF雷达观测的统计特征

本文采用ＳＯＵＳＹＶＨＦ雷达１９８７年６月２２日至６月２９日在挪威Ａｎｄφｙａ（６９°Ｎ，１０°Ｅ）的观测数据，研究中层惯性重力波传播的统计特征．２１个周期为数小时的准单色波例子，在垂直方向上有确定的相位移动，表明它们是惯性内重力波．通过分析波相关水平扰动速度的矢端曲线，获得了水平传播矢量的大小和方向的分布，大多数（７６％）波具有西向传播的波矢分量，似乎与中层顶具有强的西向背景风有关；水平传播速度的大小与中层高度上典型的观测值一致．本文分析结果还表明在极区中不仅存在向上的能量传输，也存在强烈的向下的能量传输．     

双轴连续旋转调制捷联惯导系统大失准角初始对准技术

由于可以补偿惯性器件在三个轴向上的输出误差，双轴旋转调制技术被广泛应用于捷联惯导系统(SINS)。选择了一种合理且实用的十六次序双轴转位方案，并对其调制原理和误差进行了分析。初始对准技术是捷联惯导系统的一项重要技术，其对准精度直接决定了后续导航的精度。在粗对准完成后，当姿态误差角较大时，后续的精对准误差模型呈非线性特性，故选择了滤波精度高、稳定性强的平方根容积Kalman滤波算法(SCKF)来解决这一问题。考虑到在实际对准过程中，量测噪声的统计特性易发生变化，将SCKF算法与Sage-Husa算法相结合，在传统Sage-Husa SCKF算法的基础上提出了一种改进的自适应滤波算法(ASCKF)。该算法采用QR分解来完成对噪声协方差的平方根矩阵估计，从而避免了传统Sage-Husa SCKF算法中所估噪声协方差矩阵不正定的问题。最后，通过仿真证实了ASCKF算法可被很好地应用于量测噪声统计特性发生变化的初始对准中。     

Alfvén gravity waves in viscous solar plasma: Effect of the background flow

We study the Propagation and damping properties of Alfvén gravity waves in the presence of the vertical magnetic field in the viscous solar plasma under influence of the background flow by deriving a fourth order dispersion relation in terms of the Doppler shifted frequency. We derive the dispersion relation under WKB and Boussinesq approximation. We study the damping of Alfvén gravity waves for the wave frequencies less than and greater than the Brunt-Väisälä frequency. We find that the Brunt-Väisälä frequency divides the frequency ranges where the weakly or strongly damped oscillations occur. The background flow exhibits a strong effect on weakly damped oscillations and a weak effect on the strongly damped oscillations. We also notice that the damping of both the strong and weakly damped oscillations depend on the Brunt-Väisälä frequency and wave number. The effect of the background flow is also being governed by the Brunt-Väisälä frequency and wave number. We also study the properties of gravity wave mode after filtering the Alfvén wave mode by minimizing the magnetic field and noticed that the background flow shows a very strong effect on the gravity wave mode.     

Gravity wave momentum flux generation close to mid-latitude Andes in mesoscale simulations of late 20th and 21st centuries

Adequate representations of diverse dynamical processes in general circulation models (GCM) are necessary to obtain reliable simulations of the present and the future. The parameterization of orographic gravity wave drag (GWD) is one of the critical components of GCM. It is therefore convenient to evaluate whether standard orographic GWD parameterizations are appropriate. One alternative is to study the generation of gravity waves (GW) with horizontal resolutions that are higher than those used in current GCM simulations. Here we assess the seasonal pattern of topographic GW momentum flux (GWMF) generation for the late 20th and 21st centuries in a downscaling using the Rossby Centre regional atmospheric model under the Intergovernmental Panel on Climate Change A1B emission conditions. We focus on one of the world’s strongest extra-tropical GW zones, the Andes Mountains at mid-latitudes in the Southern Hemisphere. The presence of two GCM sub-grid scale structures locally contributing to GWMF (one positive and one negative) is found to the East of the mountains. For the late 21st century the strength of these structures during the GW high season increases around 23% with respect to the late 20th century, but the GWMF average over GCM grid cell scales remains negative and nearly constant around −0.015 Pa. This constitutes a steady significant contribution during GW high season, which is not related to the GWMF released by individual sporadic strong GW events. This characteristic agrees with the fact that no statistically significant variation in GWMF at source level has been observed in recent GCM simulations of atmospheric change induced by increases in greenhouse gases.