空间尘埃的充电过程及与等离子体参数的关系

考虑了地球附近的彗星、行星环、行星际介质等空间尘埃等离子体环境中尘埃颗粒的充电问题.应用典型的空间尘埃等离子体参数,计算了不同种类的尘埃颗粒,以及不同等离子体成分下等离子体中尘粒的平衡电势,得到了尘埃颗粒的平衡电势与尘埃等离子体成分、温度,及其他等离子体参数之间的相互关系.     

太阳F10.7指数准27天振荡的小波分析

利用1956-2003年的F10.7日均值数据,采用Morlet小波变换方法,分析了准27天振荡的特征及与太阳活动11年周期(Schwabe周期)的关系.结果表明,F10.7的准27天振荡的幅度和周期存在明显的短期变化现象,不同年里变化的程度差别很大,有些年里起伏非常剧烈,在几天到几十天的很短时间里,幅度变化达十几倍,周期可变化数天,甚至发生十几天的突变;有些年里,幅度变化很大但起伏很小,周期也比较稳定.准27天振荡的年平均幅度存在明显的逐年变化,与太阳活动显著相关.一般说来,F10.7越高,准27天振荡的幅度就越大,然而在太阳活动19周峰年,F10.7比其他活动周的值都高,但准27天振荡的幅度却比其他活动周低.准27天振荡的周期也有明显的逐年变化,除了个别年(如1987年),年平均周期在24至31天之间变化,与太阳活动周期没有明显的关系.48年的平均周期为27.3天.从总体看,周期有逐渐缩短的趋势,48年里周期大约减少了1.5天.造成准27天振荡起伏的因素非常复杂,有待深入研究.     

考虑弹体柔性振荡的全捷联导引头制导信息提取

随着拦截导弹弹体长细比的增加和直接侧向力的作用,拦截导弹上全捷联导引头量测信息严重受到弹体弹性振荡和控制力矩激励的影响,从而造成导弹制导精度的下降。针对现有惯导安装在弹体质心附近的振荡波腹处无法敏感导引头振荡的不足,提出了一种在导引头安装微机电陀螺器件测量振荡角速率,构造差分观测量的新状态模型,通过交互式多模型的容积卡尔曼滤波算法实现对视线角速度的解耦和精确提取。通过构建导弹六自由度制导与控制仿真模型,采用蒙特卡洛打靶仿真验证了算法的有效性。仿真结果表明模型重构后的滤波算法可以将弹体振荡的均方根误差压缩到0.5°以内并有效跟踪弹目视线角速率。     

4m×3m风洞无人机模型振动抑制系统研制

在4m×3m低速风洞大展弦比无人机试验中,出现了纵向大振幅振动问题.通过试验观察和支撑系统的有限元计算,在不破坏风洞结构和不改变原模型姿态角变化范围的条件下,气动中心低速所研制了一套抑振装置.该装置成功应用于多个无人机型号试验,有效地抑制了纵向大振幅振动,提高了大展弦比无人机低速风洞试验数据的精准度.     

利用气动弹性的柔性振翼模型建立及分析(英文)

Making use of modal characteristics of the natural vibration of flexible structure to design the oscillating wing aircraft is proposed. A series of equations concerning the oscillating wing of flexible structures are derived. The kinetic equation for aerodynamic force coupled with elastic movement is set up, and relevant formulae are derived. The unsteady aerodynamic one in that formulae is revised. The design principle, design process and range of application of such oscillating wing analytical method are elaborated. A flexible structural oscillating wing model is set up, and relevant time response analysis and frequency response analysis are conducted. The analytical results indicate that adopting the new-type driving way for the oscillating wing will not have flutter problems and will be able to produce propulsive force. Furthermore, it will consume much less power than the fixed wing for generating the same lift.     

模化比对直升机用红外抑制器红外辐射特性的影响

对波瓣喷管一弯曲混合管构成的直升机用红外抑制器壁面和尾焰的红外辐射特性进行了一系列的数值研究,旨在将三维流场数值计算、壁温计算与红外辐射计算结合起来综合分析抑制器红外辐射特性,与相关实验数据的对比验证表明计算结果与实验结果仅相差15%左右,且红外辐射强度空问分布规律一致;通过对不同缩比模型的数值计算,揭示了模化比对壁面及尾焰的红外辐射特性的影响规律:(1)几何相似的红外抑制器在主流入口速度、温度相同时,壁面红外辐射强度与几何模化比的2次方成正比;(2)尾焰红外辐射强度与几何模化比的2.32次方成正比.      

平板射流中大尺度涡的理论模型

根据流动稳定性理论,提出了一种解释平板射流中大尺度涡产生机理的二维不稳定波理论模型,用这种模型计算所得的流动结构和相干扰动量与实验结果吻合较好.说明不稳定波模型可以较好地描述湍流平板射流中的大尺度涡结构的主要特征.      

运载火箭摇摆发动机与全箭动力学特性耦合关系研究

针对运载火箭“摆动发动机-伺服回路”负载频率低,可能影响全箭弹性模态稳定性的问题,首先建立了包含“发动机-伺服回路”动力学模型的全箭动力学模型,分析了“发动机－伺服回路”负载频率对伺服机构传递函数和控制系统开环传递函数特性的影响,指出了“发动机－伺服回路”负载频率与箭体弹性模态之间的动力学耦合关系,给出了保证弹性模态稳定的谐振频率判据,最后计算了保证全箭弹性模态稳定的负载频率边界值,并通过仿真算例验证了结果的正确性。研究结果表明,“发动机－伺服回路”局部的负载频率通过惯性负载力矩作用与全箭弹性模态形成耦合,当负载频率位于上、下边界值范围之内时就会导致某些弹性模态不稳定,因此在实际工程中应对负载频率进行限制,以保证运载火箭的飞行安全。
     

Solar Neutrinos

The current status of solar neutrino experiments is reviewed. All the experimental measurements show deficits of solar neutrinos. Non monotonic suppression indicates that the problem may naturally be explained by neutrino oscillations, but not by modifying solar models. A new experiment shows very promising results. We hope that a definite answer to the question of whether solar neutrinos are oscillating will be obtained in the very near future. This revised version was published online in June 2006 with corrections to the Cover Date.     

Shortcomings of the Standard Solar Model

The SSM, invented in early nineteen sixties, remains a useful construction. There are now much larger number of its predictions that may be compared with observations than when it was first introduced. Seismic sounding based on oscillations frequencies provides the best test of the physical input for modelling stellar evolution. The results of the test must be viewed as a support for the standard theory of stellar evolution. However, significant differences in the sound-speed, photospheric He abundance, and other parameters between the Sun and the current models remain. Shortcomings in the EOS and in treatment of convection have been revealed. The differences in the sound-speed in the radiative interior may be explained by small opacity errors but other explanations are possible. Results of seismic sounding support the idea that the element mixing in the outer part of the radiative interior occurred during a significant fraction of the Sun's life. Such mixing is considered as a possible explanation of the deficit of lithium. The shortcomings of SSM cannot explain the deficits of measured neutrino fluxes. This revised version was published online in June 2006 with corrections to the Cover Date.