近地小推力转移轨道的加权组合制导策略

 研究了近地小推力转移轨道的制导问题，给出了一种基于局部最优控制律的自主制导算法。推导出了各改进春分点根数对应的局部最优控制律；通过最优推力分配和目标偏差两个策略，对各局部最优控制律进行动态加权组合，从而有效减少了制导律的设计参数。在此基础上，针对燃料最省转移轨道，定义了一种新的发动机开关函数。采用遗传/逐次二次规划混合优化算法计算了最优制导参数。与传统算法相比，该制导算法是一种闭环制导算法，能够实现飞行器的自主制导，并且制导过程中无需对制导参数进行更新。以地球低轨到高轨的小推力转移为例，采用该方法分别求解了时间和燃料最省转移问题，并与传统算法进行了比较分析。数值结果验证了该算法的有效性。     

圆柱壳热应力的理论与实验研究

本文根据薄壳的经典理论,导出了在受有轴对称的多项式温度分布条件下,圆柱壳的位移、内力和热应力的理论公式。并以三次多项式温度分布为例,计算了三种边界条件(自由端、固支端、简支端)下,理论的和有限元的热应力曲线,对固支端进行了热应力实验,绘制了实验曲线。最后,对三种情况作了分析对比,结果表明,理论与有限元计算曲线相当吻合,计算与实验曲线分布趋势一致。     

Principal components in the PG-X-ray QSO sample

We have performed a spectral principal component analysis for a complete sample of 22 low redshift QSOs with spectra from Ly to H, and found three significant principal components, which account for 78% of the spectrum-to-spectrum variance. We present strong arguments that the first principal component represents the Baldwin effect, relating equivalent widths to the luminosity (i.e. accretion rate). The second component represents continuum variations, probably dominated by intrinsic reddening. The third principal component is directly related to broad emission-line width and X-ray spectral index, and therefore probably driven by Eddington accretion ratio, L/L_Edd. The third set of relationships tie directly to the optical Principal Component 1 found by Boroson and Green [Boroson, T., Green, R.F., Astrophys. J. Suppl. 80, 109, 1992 (BG92)], and are the primary cause of scatter in the Baldwin relationships.     

考虑流固耦合作用的一维供应管路-喷嘴系统动力学特性

为了更加深入地研究供应管路-喷嘴系统的动态特性,在喷嘴动力学理论的基础上,建立了考虑供应管路流固耦合作用的传递矩阵组合计算模型。针对三种典型液体火箭发动机喷嘴与一维供应管路组成的系统,开展了两端固定边界的系统动力学特性数值模拟。结果表明:管路结构谐振与管内流体谐振所导致的喷嘴出口位置流体速度振荡量级相当,管路流固耦合作用对系统动态特性的影响不能忽略;管路结构谐振是造成其固定位置应力的频率响应幅值较高的主要因素;当流体与结构的谐振频率接近时,会产生一个大带宽、高幅值的应力耦合振荡区间,随着管壁厚度的增大,耦合振荡的带宽也随之增大;对于文中算例,流固耦合作用对流体谐振造成的系统振荡具有约5%的降频作用。     

一类滞后不确定相似组合系统的分散控制

本文给出了一个使滞后的相似组合大系统镇定的分散鲁棒控制器的设计方法。不确定性是时变的,是以不确定参数出现在每个子系统中,而存在于互联项中的不确定性假设可能知道它的边界,当系统具有某种特征时,简化了一般控制器的设计。     

激光功率与底面状态对选区激光熔化球化的影响

为研究激光功率与底面状态对选区激光熔化熔池流动的影响，基于离散单元法建立了选区激光熔化铺粉模型，采用粒径分布与实验相符的马氏体时效钢粉末分别铺展到平坦底面和增材底面上，将计算获得的粉末分布导入到基于有限体积法建立的选区激光熔化熔池计算流体力学模型中，研究激光功率和基板底面粗糙度对熔池流动和熔道表面形貌的影响。采用激光单道扫描实验验证铺粉模型和选区激光熔化模型。结果表明：随着激光功率的降低，单位长度的球化数量增加；由于增材底面使熔池润湿性变差，同时又对熔池流动行为产生扰动，使得增材粗糙底面上熔道的球化数量增加。选区激光熔化铺粉模拟及激光单道扫描模拟结果与实验结果吻合较好。本研究可为选区激光熔化工艺中工艺参数的选择提供理论指导。     

A practical nonlinear robust control approach of electro-hydraulic load simulator

This paper studies a nonlinear robust control algorithm of the electro-hydraulic load simulator （EHLS）. The tracking performance of the EHLS is mainly limited by the actuator＇s motion disturbance, flow nonlinearity, and friction, etc. The developed controller is developed based on the nonlinear motion loading model. The problems of the actuator＇s disturbance and flow nonlinearity are considered. To address the friction problem, the friction model of the loading motor is identified experimentally. The friction disturbance is compensated using the obtained friction model. Therefore, this paper considers the main three factors comprehensively. The developed algorithm is easy to apply since the controller can be obtained just with one step back-stepping design. The stability of the developed algorithm is proven via Lyapunov analysis. Both co-simulation and experiments are performed to verify the effectiveness of this method.     

Indicators of black-hole mass and Eddington accretion ratio from QSO X-ray and UV spectra

The evolution of luminous QSOs is linked to the evolution of massive galaxies. We know this because the relic black-holes found locally have masses dependent on the properties of the host galaxy’s bulge. An important way to explore this evolution would be to measure dependences of black-hole masses and Eddington accretion ratios over a range of redshifts, i.e., with cosmological age. For low redshift QSOs (and their lower luminosity Seyfert galaxy counterparts) it has been possible to infer black-hole masses from the luminosities and velocity dispersions of their host-galaxy bulges. These masses agree with those virial black-hole masses calculated from the Doppler widths of the broad Hβ emission lines. The latter method can then be extended to more distant and luminous QSOs, up to redshifts of 0.6 with ground-based optical observations. We discuss ways to extend these explorations to higher redshifts – up to 3 using the widths of QSOs’ broad UV emission lines, and in principle, and to redshifts near 4 from ground-based infrared observations of rest-frame Hβ at 2.5 μm. We discuss the possibility of investigating the accretion history of the higher redshift QSOs using measures of Eddington accretion ratio – the soft X-ray spectral index and the eigenvectors of Principal Components Analyses of QSOs’ UV emission-line spectra.     

强海杂波背景下目标检测方法综述

高频地波雷达被广泛应用于海面目标的检测,而由于海杂波的分布散射具有很强的动态特性,通常情况下成为了海面目标检测的主要干扰成分.因此,在强海杂波背景下进行目标检测的关键在于如何有效抑制海杂波.从循环对消、子空间分解、模型预测以及分形特征这几方面对海杂波抑制技术进行综述、分析和总结,为后续对海面目标检测提供参考.     

同轴离心式喷嘴热声不稳定性递归分析

为获得同轴离心式喷嘴燃烧动力学特性，开展了喷注单元稳定性试验研究。试验中燃料流量不变，随氧化剂流量增加，热声系统依次经历了燃烧噪声状态、阵发状态和准周期振荡状态。采用递归方法对实验结果进行分析。首先，利用交互信息法和虚假最邻近法分别求解最优延迟时间和嵌入维数，获得了典型工况下的相空间轨迹图。其次，递归图分析表明系统出现了第II类阵发现象，意味着系统发生了亚临界Hopf分叉，与实验结果一致。最后，递归量化分析表明，确定率可以将阵发状态和准周期振荡状态与燃烧噪声状态区分出来，并可以对热声振荡进行预报。