星载全球大气波动成像仪研究

在卫星上对中间层顶区域的气辉辐射成像观测, 对于全球大气波动的监测和研究具有重要的意义. 利用TDICCD对O₂A (0-0)气辉进行成像观测, 计算了曝光积分时间、信噪比和能达到的最高空间分辨率, 分析了地球自转对空间分辨率的影响, 在此基础上提出一种星载全球大气波动成像仪方案, 该方案可以观测垂直波长大于10km的大气波动, 最高水平分辨率可以达到0.33km.      

Roe格式中不同类型熵修正性能分析

针对Roe格式中较为流行的3类熵修正:Muller型、Harten-Yee型和Harten-Hyman型熵修正,从理论分析入手, 辅以Euler方程为控制方程的激波管问题,前台阶流动和运动激波的双马赫反射3个数值实验,对不同熵修正的性能做了深入研究,得出如下结论: Muller型和Harten-Yee型熵修正方法作用于激波和非物理的膨胀激波2种情况:激波情况下引入的数值耗散,能根本改善"Carbuncle"现象,膨胀激波时其数值粘性也足以使膨胀激波得以耗散;而类Harten-Hyman型熵修正只对膨胀过程起修正作用,对激波情况无效,不能改善"Carbuncle"现象,该类熵修正的数值粘性较小,不足以使膨胀过程正确求解;直接采用 δ 值代替特征值的特征值修正方法效果好于传统的特征值修正方法.     

A CFD-based numerical virtual flight simulator and its application in control law design of a maneuverable missile model

A CFD-based Numerical Virtual Flight (NVF) simulator is presented, which integrates an unsteady flow solver on moving hybrid grids, a Rigid-Body Dynamics (RBD) solver and a module of the Flight Control System (FCS). A technique of dynamic hybrid grids is developed to control the active control surfaces with body morphing, with a technique of parallel unstructured dynamic overlapping grids generating proper moving grids over the deflecting control surfaces (e.g. the afterbody rudders of a missile). For the flow/kinematic coupled problems, the 6 Degree-Of-Freedom (DOF) equations are solved by an explicit or implicit method coupled with the URANS CFD solver. The module of the control law is explicitly coupled into the NVF simulator and then improved by the simulation of the pitching maneuver process of a maneuverable missile model. A nonlinear dynamic inversion method is then implemented to design the control law for the pitching process of the maneuverable missile model. Simulations and analysis of the pitching maneuver process are carried out by the NVF simulator to improve the flight control law. Higher control response performance is obtained by adjusting the gain factors and adding an integrator into the control loop.     

液体晃动非线性阻尼的描述方法

采用等效线性化手段研究了液体晃动非线性阻尼特性的描述方法，给出了自由衰减响应的对数衰减率与非线性阻尼比之间的关系，提出了通过自由衰减响应确定非线性阻尼特性参数的两种方法。计算表明，两种方法所得到的结果可以满足工程应用所要求的精度。     

非线性参数识别的相关积分方法及其应用

使用相关积分方法解决单自由度非线性系统的参数识别问题。利用相关积分方法的滤波特性可以有效地抑制测量信号中的噪声影响，提高参数估计的精度。同时可以分别建立非线性阻尼和刚度参数的线性识别方程．实现两类参数的分离识别，有利于弱非性项的参数估计。将这一方法用于贮箱内液体晃动等效力学模型参数的试验确定问题，解决了由于采用防晃装置而产生的非线性晃动阻尼的参数识别问题。     

复杂结构的非线性检测

由于非线性系统的复杂性,现有的各种非线性检测方法都有局限性。从频域、幅域和时域三方面综合考察复杂结构的非线性表现,采用六种方法进行非线性检测,给出一个综合描述系统非线性程度的指标－非线性因子。鉴于非线性系统表现出的非线性强弱与系统所受的激励有直接的关系,将非线性因子定义为与激励的幅值特性和频率特性相关的系数指标。对几种典型非线性系统的仿真模型进行了检测,以验证非线性因子的有效性。     

矩形悬臂板的非线性弯曲

矩形悬臂板的非线性弯曲是板理论中的一个相当困难的课题,至今还没有研究过。给出由三角函数和多项式组成的近似挠度函数ｗ（ｘ,ｙ）和应力函数Ｆ（ｘ,ｙ）,它们满足矩形悬臂板的部分边界条件。然后用广义伽辽金方法得到矩形悬臂板非线性弯曲问题的解。最后给出了算例。     

NVNA谐波相位检验件设计及定标

本文介绍了一种用于检验非线性网络分析仪谐波相位指标的检验件设计方法,并搭建了基于实时示波器的测量系统对谐波相位进行定标。通过高速实时示波器对检验件的输出信号进行采样,利用傅立叶变换提取谐波相位信息。为了得到高准确度的测量结果,采用去缠绕、最小二乘等算法对相位结果进行优化处理。实验结果表明,该方法可以作为NVNA谐波相位指标的验证手段对NVNA的谐波相位进行验证。     

A comparative and numerical study of effects of gravity waves in small miss-distance and miss-time GPS radio occultation temperature profiles

The Global Positioning System (GPS) Radio Occultation (RO) technique has global coverage and is capable of generating high vertical resolution temperature profiles of the upper troposphere and lower stratosphere with sub-Kelvin accuracy and long-term stability, regardless of weather conditions. In this work, we take advantage of the anomalously high density of occultation events at the eastern side of the highest Andes Mountains during the initial mission months of COSMIC (Constellation Observing System for Meteorology, Ionosphere and Climate). This region is well-known for its high wave activity. We choose to study two pairs of GPS RO, both containing two occultations that occurred close in time and space. One pair shows significant differences between both temperature profiles. Numerical simulations with a mesoscale model were performed, in order to understand this discrepancy. It is attributed to the presence of a horizontal inhomogeneous structure caused by gravity waves.     

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.