吸附式压气机叶型和抽吸方案优化设计

将智能优化算法与准三维叶栅计算程序相结合,对某吸附式压气机叶型进行了优化设计,对优化设计前后的流场进行了详细分析.优化设计之后叶型总压损失下降40%,静压升提高0.6%.优化得到最佳抽吸位置位于分离区起始点上游,优化叶型具有更均匀的负荷分布,并且优化后叶型的性能在全攻角范围内均得到了提升.结果表明:更均匀的负荷分布会提高叶型的性能,减小叶型分离,降低抽吸所需要的能量.对于在尾缘处存在轻微分离的叶型其最优抽吸位置位于分离区上游.     

基于序列采样算法的轮盘减质优化

介绍了一种基于蒙特卡罗表述的空间缩减策略和局部边界线搜索的序列采样算法,该算法利用已有样本点的信息缩减原有设计空间,使得在缩减设计空间上生成的新样本点能够同时具有良好的空间填充特性和投影特性.与已有的序列采样算法的比较结果表明,该算法具有较高的采样效率和采样质量.采用此序列采样算法结合Kriging模型和遗传算法进行轮盘减质优化,优化结果减质10%.该序列采样算法为工程结构的优化提供了一条灵活有效的途径.      

射流控制反推力装置流场数值研究

针对涵道比为8的涡扇发动机无阻流门叶栅式反推装置,利用CFD技术,计算分析了二次射流孔的位置、角度、孔数以及流量对反推力性能和外涵通道内流场流动特征的影响。计算结果表明:外涵流体与二次射流相互作用后,在二次射流下游产生了一个主涡和副涡,阻碍外涵气体向下游流动;射流孔位置对涡扇发动机的影响不仅体现在反推力效率,而且影响上游风扇后的气体压力不均匀度和背压;二次流射流角度对反推力性能的影响在诸多影响因素中占主导地位,存在一个最佳射流角度;二次流质量流量增加,反推力效率呈增加趋势;二次流入射孔的个数关系到相邻入射气流在周向的覆盖程度,从而影响反推效率;二次流射流位置、角度以及流量对反推性能的影响是相互耦合的,在反推力装置设计时需要综合考虑三者间的相互影响;在研究参数范围内,最佳的射流孔位置范围L=110mm~150mm,最佳射流角度α在10°~20°范围内。     

基于自适应网格加密的超声速可燃气热射流起爆详细反应数值模拟

采用块结构自适应网格加密开源程序AMROC,在高性能计算集群中,进行氢气、氧气、氮气详细反应机理的二维超声速热射流爆震起爆自适应网格精细数值模拟,研究在热射流的持续喷射作用下超声速可燃气热射流爆震起爆,以及形成的精细的爆震胞格结构.结果表明:超声速可燃气流中热射流类似气动斜劈,形成局部激波诱导燃烧.超声速可燃气中持续的热射流喷射会形成过驱爆震,并导致不规则爆震胞格的生成.热射流的扰动压缩作用对过驱爆震的形成以及不规则爆震胞格的产起着关键的作用.热射流的扰动压缩波以当地声速通过爆震波后的亚声速区域作用于爆震波,使爆震波处于持续过驱状态,并形成不规则的爆震胞格结构.     

轮体结构颗粒阻尼器设计方法

利用离散元法及正交设计方法,对典型轮体结构发生伞形振动时的二维等效振动模型进行了空腔尺寸及颗粒填充方案的数值设计,并结合振动试验结果给出了轮体结构颗粒阻尼器的设计流程及设计准则.研究表明:1建立的二维等效振动模型在能够反映轮体结构伞形振动基本特征的同时,也可以较为准确地模拟内部颗粒运动对结构产生的影响;2颗粒阻尼对轮体结构的振动有明显的改善作用,但填充不同材质的颗粒,其减振效果会有较为明显的区别;3空腔的尺寸及颗粒的质量率对颗粒阻尼的影响显著,应首先保证的是较高的颗粒质量率;4由于碰撞间隙的作用,对于固定规格的空腔和颗粒,存在最佳颗粒体积填充率使得颗粒阻尼的减振效果最佳.由试验与数值模拟的最佳方案的一致性可知,发展的设计方法可以较为准确地给出轮体结构颗粒阻尼器的最优空腔尺寸及其对应的最佳填充方法,可用于轮体结构伞形振动减振方案的前期设计.     

A novel optimal design for an application-oriented synthetic jet actuator

The evaluation indicator for the performance of a synthetic jet actuator （SJA） is well-defined because of its various applications, which require optimal design to improve its performance and extend its field of application. This paper presents a novel approach to the optimal design of an SJA applied to enhance fuel/air mixture. It optimizes the combination of an actuator＇s geometric parameters by selecting the strength of vortex pairs as the evaluation indicator, coupled with orthogonal experiments and analysis of variance （AOV）. The results indicate that slot width is the most notable factor influencing the strength of vortex pairs, followed by cavity height and slot depth. The optimal value of the strength of vortex pairs increases by 32.5%over the experimental data of the base case, and more than 8.4%compared with the simulation results of the orthogonal experiments. It is concluded that the optimal method can effectively improve the performance of an SJA applied in mixing enhancement, reducing the test numbers and the associated design cycle and cost.     

小间距单孔冲击凸面靶板流场结构实验

利用烟线法研究了小间距、单孔冲击凸面靶板的流场结构.实验中,改变冲击雷诺数Re、冲击间距和冲击孔直径之比H/d以及冲击靶面相对曲率d/D等参数,通过拍摄流场形态,分析气流分离角度和涡旋结构随上述参数的变化规律.研究结果表明当Re,H/d较大时,在凸面靶板周向两侧形成了稳定的旋流结构.随着Re,H/d的增加,冲击射流与靶面分离处对应的圆心角增大,分离推迟.实验中还发现当d/D减小,流体与靶面的分离提前,其相对应的圆心角呈现减小的趋势.      

An empirical relation to correct storm-time thermospheric mass density modeled by NRLMSISE-00 with CHAMP satellite air drag data

With the help of STAR (Spatial Triaxial Accelerometer for Research) accelerometer measurements on board CHAMP (Challenging Minisatellite Payload), the global distributions of total mass density changes at about 400 km height during major magnetic storms are studied, aiming to improve the capability of current thermospheric model for predicting the storm-time mass density distribution. The density calculated by the NRLMSISE-00 model without using the geomagnetic active index as input is taken as a reference on top of which the storm-time changes are added. In total 19 storm events during 2001–2004 are used to perform a comprehensive statistical analysis. A relative calibration of drag coefficient along with accelerometer calibration parameters is made by fitting the CHAMP observed initial mass densities in with the NRLMSISE-00 model on quiet days before each storm. The dependences of the storm-time changes in mass density on both the total global Joule heating power, ∑_Qj$\sum Q_{\text{j}}$ and the high-resolution ring current index, Sym-H, are investigated. The lag times of mass density changes with respect to the Joule heating and Sym-H variation are obtained as a function of latitude and sunlight. By using a multiple linear regression analysis with proper time shift, an empirical relation connecting storm-time changes in mass density for 400 km height with the two parameters, ∑_Qj$\sum Q_{\text{j}}$ and Sym-H, has been worked out for different latitude and sunlight conditions (day-side or night-side). Adding a correction calculated from the empirical relation to the NRLMSISE-00 model reference leads to a better prediction of storm-time thermospheric mass density distribution.     

两类DBL码的性能比较

设计出扩展的Large area Synchronization地址码(LS码)——Daoben Lab地址码(DBL码).DBL码由基本LS码与矩阵左、右直积生成,分别称为DBL左乘码和DBL右乘码,两类DBL码各有特点.DBL右乘码特点是把码字分组,码组间码字存在更大的零相关窗,增加了可用码字数,码组内码字非周期相关性与扩展矩阵行向量的相关性相同;DBL左乘码也是把码字分组,码组间的零相关窗长度不变,没有增加可用码字数,但当以正交矩阵扩展时,码组内有和原LS码同样长度的零相关窗.计算机仿真验证了两类DBL地址码的性质.      

Kuafu and the studies of CME initiation

We first briefly review the current trend in the studies of coronal mass ejections (CMEs), then summarize some recent efforts in understanding the CME initiation. Emphasis has been put on the studies of Earth-directed CMEs whose associated surface activity and large scale magnetic source have been well identified. The data analysis by combining the MDI full disc magnetograms, vector magnetograms of active regions, EUV waves and dimmings, non-thermal radio sources, and the SOHO LASCO observations has shed new light in understanding the CME magnetism. However, the current studies seem to invoke new observations in a few aspects: (1) The observations which enable us to trace CMEs from the earliest associated surface activity to its initial acceleration and key development in the low corona in the height of 1–3 R; (2) The imaging spectroscopic observations which can be used to diagnose the early plasma outflow and the line-of-sight velocity in understanding the kinematics of CMEs; (3) The accurate timing from primary magnetic energy release, manifested by chromospheric activity, non-thermal radio bursts, and EUV, X-ray and γ-ray emissions, to the CME initiation, early acceleration and propagation, and the consequences in the interplanetary space and magnetosphere. The Kuafu Mission will meet the basic requirement for the new observations in CME initiation studies and serve as a monitor of space weather of the Sun–Earth system.