几何非线性机翼本征梁元素模型的高效化改进

 采用Hodges等提出的时间-空间离散化的几何精确非线性本征梁通用模型处理柔性机翼结构动力学问题时,当离散化的节点数增大时,该方法的未知数数量成倍地增长,而且方程组是严重病态的,因此数值模拟计算的速度非常缓慢。针对机翼中最常见的悬臂梁结构,根据空间离散化的边界条件,提出了空间缩聚法把空间离散差分方程缩聚为常系数矩阵格式,得到了只与时间相关的微分方程组,进一步推导得到了该方程组的雅可比矩阵,因而大大减少了方程组的数量以及求解过程的循环和迭代步数。采用Gear方法分别求解了原始的本征梁元素模型和本文提出的缩聚模型,结果表明空间缩聚模型在相同条件下可提高运算速度约5.1倍,而且对不同类型的外载荷都具有较好的通用性、稳定性和高效性。     

飞翼布局无人机进排气效应风洞试验研究

飞机进排气会对全机气动性能产生明显的影响.采用引射式动力模拟器对飞翼布局无人机开展进排气效应模拟,分析进排气对全机气动特性的影响.试验结果表明:进排气对飞翼布局升力影响不明显,对阻力影响量比较大,可使全机最大升阻比降低1～4左右,而喷流能使全机最大升阻比下降1～1.8左右,进排气效应使得全机俯仰力矩增加,但纵向静安定度基本不变;进排气对全机横航向特性影响不大,对襟翼效率影响也甚微.可作为飞翼无人机气动布局设计的参考.     

弹舱对飞翼布局飞机气动特性影响及其控制

以高速风洞气动力测量为研究手段,开展了弹舱开启对飞翼布局飞机气动特性影响及其流动控制试验研究。试验结果表明,对于飞翼布局飞机,弹舱开启主要影响飞机阻力特性,巡航状态下,弹舱开启后使得全机阻力增加60%～110%,Ma=0.8时全机升阻比降低34%。通过在弹舱前缘安装扰流片,对弹舱腔口剪切层施加流动控制,巡航状态下弹舱开启附加阻力最多降低20%,Ma=0.8时全机升阻比提高12.6%。     

飞机带翼尖弹着陆响应研究

某型飞机机翼挂装翼尖导弹对机翼结构设计和结构分析提出了诸多全新课题 ,如结构的振动响应和气动弹性动响应。本文就某型飞机着陆时的结构振动响应作了初步分析。     

从多格薄壁盒模型结构优化设计想到的问题

通过构建简单模型来揭示飞行器翼面复杂结构中存在值得探讨的专题,是本文要研究的内容。以结构稳定性条件作为切入点,利用多格薄壁盒作为简化模型来模拟翼面结构的主要承力部分,巧妙地降低了问题的复杂性。其图形曲线特征表明:该优化问题的目标函数非凸不连续,而且还具有多个局部最优解;进一步的计算指出:无论是替换材料还是增减载荷大小或者改变几何参数的尺寸,此模型的最优结构拓扑形式均要发生变化。从本文所做的工作可以推知:无论从学术研究角度还是工程应用方面,基于稳定性约束的翼面结构优化设计均是一个值得研究的专题。     

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.     

Real-Time Specifications of the Geospace Environment

We report the recent progress in our joint program of real-time mapping of ionospheric electric fields and currents and field-aligned currents through the Geospace Environment Data Analysis System (GEDAS) at the Solar-Terrestrial Environment Laboratory and similar computer systems in the world. Data from individual ground magnetometers as well as from the solar wind are collected by these systems and are used as input for the KRM and AMIE magnetogram-inversion algorithms, which calculate the two-dimensional distribution of the ionospheric parameters. One of the goals of this program is to specify the solar-terrestrial environment in terms of ionospheric processes, providing the scientific community with more than what geomagnetic activity indices and statistical models provide. This revised version was published online in August 2006 with corrections to the Cover Date.     

Modelling of the electromagnetic field in the interplanetary space and in the Earth's magnetosphere

A magnetohydrodynamic model of the solar wind flow is constructed using a kinematic approach. It is shown that a phenomenological conductivity of the solar wind plasma plays a key role in the forming of the interplanetary magnetic field (IMF) component normal to the ecliptic plane. This component is mostly important for the magnetospheric dynamics which is controlled by the solar wind electric field. A simple analytical solution for the problem of the solar wind flow past the magnetosphere is presented. In this approach the magnetopause and the Earth's bow shock are approximated by the paraboloids of revolution. Superposition of the effects of the bulk solar wind plasma motion and the magnetic field diffusion results in an incomplete screening of the IMF by the magnetopause. It is shown that the normal to the magnetopause component of the solar wind magnetic field and the tangential component of the electric field penetrated into the magnetosphere are determined by the quarter square of the magnetic Reynolds number. In final, a dynamic model of the magnetospheric magnetic field is constructed. This model can describe the magnetosphere in the course of the severe magnetic storm. The conditions under which the magnetospheric magnetic flux structure is unstable and can drive the magnetospheric substorm are discussed. The model calculations are compared with the observational data for September 24–26, 1998 magnetic storm (Dst _min=−205 nT) and substorm occurred at 02:30 UT on January 10, 1997. This revised version was published online in August 2006 with corrections to the Cover Date.     

双三角翼大迎角绕流的并行计算

本文在ＬＵ－ＳＧＳ方法求解可压缩Ｎａｖｉｅｒ－Ｓｔｏｋｅｓ方程的串行程序基础上,发展了适合ＭＰＰ系统类型的并行计算机的并行算法程序,并针对双三角翼大迎角绕流问题,就不同的并行计算方法进行了对比研究,探讨了优化并行策略,提高计算效率和计算加速比等问题。     

三角翼俯仰振荡中若干参数影响的实验研究

本文研究一个 6 0°三角翼以不同振荡频率 ,不同振幅从不同起始迎角进行俯仰振荡的纵向气动力特性 ,研究发现跨越具有不同时间尺度的流态的振荡会产生明显的气动力迟滞现象 ,这一迟滞现象随减缩频率的增大有一个极限值 ;在同一种流态下振荡 ,气动力迟滞现象不明显 ,这一结果对充分利用非定常气动力有指导意义。