风切变场中直升机前飞状态动态响应

为解决复杂风切变场中直升机运动的数值仿真,把握非线性直升机模型在风场中的响应特性,建立了一维、二维的风切变模型,采用直升机非线性飞行动力学模型,考虑直升机的控制系统,用四阶龙格－库塔法数值仿真直升机在风场中的前飞运动.对水平风和铅垂风的各个梯度场对响应的影响进行比较.结果表明,水平风和铅垂风的各个梯度场对响应的影响是不同的,此研究中二维空间的组合梯度场构成更为危险的飞行环境;在不同的情况下其作用是不可忽略的,尤其注意在低空飞行状态下对直升机飞行性能的影响.也进一步说明此数值仿真法对非线性直升机模型在复杂风场中响应研究实用有效.     

Study of Solar Corona in China

Considerable progress for the study of solar corona physics has been achieved by China's space physics community. It involves the theoretical study of coronal process of solar active phenomena, solar wind origin, acceleration of solar wind and coronal mass ejections, observational and numerical study of these problems and prediction methods of solar eruptive activities (such as flares/CMEs). Here is a brief summary of the progress in this area. Main progress is put upon the following three topics: corona and solar wind, numerical method, prediction method.     

厦门机场低空风切变产生的地理成因分析

厦门机场航班飞行遭遇低空风切变的频次较高,危及飞行安全。产生风切变的原因主要有两大类,一是大气运动本身的变化,一是地理、环境因素。本文着重分析因厦门机场地理环境及环境变化导致风切变产生的原因。     

被动型星载氢钟H型气体电离模型及参数优化

针对被动型星载氢钟气体电离装置低功耗、低电磁干扰的设计要求,设计了一种基于平面盘绕馈能天线的H型电离系统,并建立该电离方法的数学模型。首先,由Maxwell方程出发,推导出了电离泡中的电场和磁场的分布模型,得到气体电离机制;再由电磁场的分布方程推导出氢气击穿判据表达式,建立了气体电离条件的数学模型;最后,利用电离击穿条件判据方程优化了电离装置的设计参数。数值仿真与测试表明该模型是有效的,采用优化的设计参数可以使电离功耗和电磁干扰特性得到改善,且电离直流电源总功率可小于2W。     

低雷诺数下离心压气机性能及流动影响的数值研究

对高空低雷诺数条件下低压离心压气机进行了全三维数值模拟,分析了雷诺数对其内部流场的影响.结果表明:随着雷诺数降低,离心压气机的效率、裕度和流通能力下降;影响叶片表面负荷分布,使得转子叶片的做功能力下降;叶片前缘分离区范围增大,二次流增强,分流叶片叶尖泄漏损失增大,主叶片吸力面通道的低速区明显增大,起始位置也向前移动,对展向的影响区域也随之增加.      

Universal scaling laws for fully-developed magnetic field turbulence near and far upstream of the Earth’s bow shock

We analyze the multifractal scaling of the modulus of the interplanetary magnetic field near and far upstream of the Earth’s bow shock, measured by Cluster and ACE, respectively, from 1 to 3 February 2002. The maximum order of the structure function is carefully estimated for each time series using two different techniques, to ensure the validity of our high-order statistics. The first technique consists of plotting the integrand of the pth order structure function, and the second technique is a quantitative method which relies on the power-law scaling of the extreme events. We compare the scaling exponents computed from the structure functions of magnetic field differences with the predictions obtained by the She–Lévêque model of intermittency in anisotropic magnetohydrodynamic turbulence. Our results show a good agreement between the model and the observations near and far upstream of the Earth’s bow shock, rendering support for the modelling of universal scaling laws based on the Kolmogorov phenomenology in the presence of sheet-like dissipative structures.     

Periodic Variations of Drag Coefficient for the ANDE Spherical Satellites During its Lifetime

A drag coefficient (C_D) inversion method is introduced to study the variations of the drag coefficient for orbital satellites with spherical geometry. Drag coefficients of the four micro satellites in the Atmospheric Neutral Density Experiment (ANDE) are compiled out with this new method. The Lomb-Scargle Periodgram (LSP) analysis of the four ANDE satellites' C_D series has shown that there are obvious 5, 7, 9, and 27 days' period in those data. Interesting results are found through comparing the LSP analysis with series of the daily solar radio flux at 10.7 cm (F_10.7 index), the Ap index, and the daily averaged solar wind speed at 1AU. All series in the same time interval have an obvious period of about 27 days, which has already been explained as the association with the 27 days' solar rotation. The oscillating periods less than 27 days are found in series of C_D, Ap and solar wind speed at 1AU, e.g., the 5, 7, 9 days period. However, these short periods disappeared in the time series of F_10.7 index. The same periodicities of 5, 7, 9 days in Ap and solar wind are presented at the same time interval during the declining phase of solar cycle 23. While in the ascending phase of solar cycle 24, these short oscillations are not so obvious as that in the declining phase of solar cycle 23. These results provide definite evidence that the C_D variations with period of 5, 7 and 9 days are produced by a combination of space weather effects caused by the solar wind and geomagnetic activity.      

乙烯和汽油多循环脉冲爆震发动机起爆特性比较

为了研究脉冲爆震发动机(PDE)结构对其工作性能的影响,在内径为40mm、长为1050mm的气动阀式脉冲爆震发动机样机上,进行了气态乙烯/空气和液态汽油/空气的多循环起爆特性试验研究.研究结果表明:在25,30Hz和40Hz下都能在乙烯/空气中成功触发爆震波,40Hz下产生C-J(Chapman-Jouguet)爆震波,传播速度为1724m/s(低于C-J爆震波速度理论值1832.45m/s的5.6%),峰值压力为3.01MPa(高于C-J爆震波压力理论值2.79MPa的7.88%).在相同结构下,汽油/空气未能完成由缓燃向爆震转变的过程.通过对比两种燃料下的试验结果发现:相对于气态燃料,液态燃料受其蒸发过程的影响,在爆震管内的火焰加速缓慢,需要更多的强化燃烧装置来加速火焰,带来的总压损失也更大.因此,对于液态燃料改善雾化和蒸发,提高可爆混气的质量是其实现低阻起爆的关键.      

用自助加权范数法评估三参数威布尔分布可靠性最优置信区间

提出自助加权范数法,以评估三参数威布尔分布可靠性的最优置信区间.基于可靠性经验值与理论值的差异,通过6个最小加权范数准则,构建出威布尔分布的最优参数信息向量.对最优参数信息向量进行自助再抽样,获得生成参数信息向量,用于模拟参数的概率密度函数.在给定置信水平下,求解出参数的估计真值及其置信区间,并据此建立可靠性的估计真值函数及其最优置信区间函数.滚动轴承性能寿命案例、直升机部件失效案例与某试件疲劳寿命案例的研究表明:使用自助加权范数法,估计真值函数与可靠性经验值相一致,最优置信区间函数能描述试验结果的真实状态.      

一种实用的运输类飞机机翼/发动机短舱一体化优化设计方法

发展了一套基于遗传算法优化/Navier-Stokes方程分析的运输类飞机机翼/发动机短舱一体化设计方法,提出了一系列保证该方法工程实用性的解决方案,其中包括设计变量模块化、局部优化全机分析、超临界压力分布约束条件等。通过采用适当的计算网格、并行算法及数值方法,使得基于遗传算法优化/Navier-Stakes方程分析设计方法的运算时间在工程上能够接受。运用该设计方法对下单翼运输类飞机机翼/发动机短舱一体化设计开展了单点优化和两点优化,结合二者结果对比验证了该方法的有效性和工程实用性。单点优化得到的机翼压力分布呈现无激波特点,阻力系数随马赫数变化比较剧烈;两点优化得到的机翼压力分布为弱激波形态,阻力随马赫数变化比较缓和,所设计的机翼具有更好的鲁棒性和工程实用性。