跨介质航行器波浪环境入水流场演变和运动特性研究

跨介质航行器是一种既可以在空中飞行又可以在水下潜航的新概念航行器,基于仿生学原理,提出一种通过改变外形实现水空介质跨越的航行器模型,通过入水试验装置和计算流体动力学方法,对航行器带攻角从空气到水的介质跨越过程进行了试验和数值仿真研究,得到了跨介质入水过程航行器的运动姿态和入水空泡形态,并通过数值仿真得到了航行器的升力、阻力、速度和加速度演化规律。同时基于数值模拟方法对有波浪情况和静水情况下航行器入水过程空泡演变以及运动特性进行对比。结果表明:提出的航行器构型在水中具有较好的姿态调整能力,波浪的有无和波高的不同都会对航行体入水运动特性造成影响。     

工艺参数对砂布轮柔性抛光力影响规律的分析

为了掌握砂布轮抛光工艺参数对抛光力的影响规律，提高抛光质量，设计了四因素三水平正交试验，利用试验结果建立了抛光力预测模型，验证了模型的显著性；分析了工艺参数对抛光力耦合影响规律，结果表明：抛光力随砂布轮初始半径和粒度的减小而增大，随转速和压缩量的增大而增大；对叶片进气边的抛光实验效果表明：通过控制压缩量可以获得稳定的抛光力，进而获得理想的抛光效果。     

Ultrasound assisted solidification process of ternary Cu–Sn–Sb alloy

It is well-known that the application of ultrasound during liquid to solid transitions for alloys can refine the solidification microstructure and thus improves the mechanical properties. How-ever, most published work focuses on single phase dendritic growth, whereas little has been con-ducted on the multiphase alloys with complicated phase transformations during solidification. In this work, the solidification process of ternary Cu40Sn45Sb15 alloy was realized within intensive ultra-sonic field with a resonant frequency of 20 kHz and ultrasound power from 0 W to 1000 W. The ultrasound refines the size of the primary e(Cu3Sn) intermetallic compound by two orders of mag-nitudes. If the ultrasound power increases to 1000 W, g(Cu6Sn5) phase nucleates and grows directly from parent liquid phase without the occurrence of peri-eutectic reaction on the top of the alloy sam-ple where the ultrasound intensity is sufficiently high. These microstructural variations lead to the enhancement of compressive strength and elasticity modulus of ternary Cu40Sn45Sb15 alloy.     

A constitutive model coupling damage and material anisotropy for wide stress triaxiality

A constitutive model that can describe the damage evolution of anisotropic metal sheets during the complex forming processes which experience wide stress triaxiality history is essential to accurately predict the deformation and rupture behaviors of the processes. In this study, a modified Lemaitre damage criterion which couples with the anisotropic Barlat 89 yield function is established. The effects of stress triaxiality, Lode parameter and shear stress on damage accumulation are considered in the constitutive model. The model is numerically implemented and applied to fracture prediction in tensile tests with different stress triaxialities and a complex deformation process with wide stress triaxiality history. The good consistency of predictions and experiments indicates that the modified Lemaitre damage model has excellent fracture prediction ability. Finally, the accuracy of the model is analyzed and discussed.     

A concept mission for the Stellar Population and Evolution with Cubesats (SPEC)

Binary or multiple stellar systems, constituting almost a third of the content of the Milky Way, represent a high priority astronomical target due to their repercussions on the stellar dynamical and evolutionary parameters. Moreover the spectral study of such class of stars allows to better constrain the evolutionary theories of the Galactic stellar populations. By resolving the members of stellar systems through photometric observations we are able to perform more detailed measurements to infer their mass. In this paper we investigate the feasibility of a cubesat based mission including an optical payload to directly optically discriminate the members of a selected sample of binary systems. The scientific targets, consisting 11?M class dwarf stars binary systems, have been extracted from the already studied Riaz catalogue. These subset has been selected considering the star distance, the members angular separation, and the distance from the Galactic plane (due to limit the background and foreground contamination). The satellite concept is based on a 6 unit Cubesat embedding some commercial off the shelf components and an ad hoc designed optical payload occupying almost 4 units. The optical configuration has been chosen in order to fit the angular resolution requirements, as derived from the target characteristics. Moreover, according to the optical analysis and the computed field of view some requirements on the attitude control system have been inferred and fulfilled by the component selection. The paper is organized as in the following: a brief scientific introduction is made; consequently the project is described with particular attention to the optical design and the standard sub-systems; finally the conclusions are drawn and the future perspectives are investigated.     

热处理对激光增材制造Ti2AlNb基合金组织及性能的影响

利用激光增材制造技术制备出Ti-22Al-25Nb合金薄壁试样,分析了沉积态和热处理态试样的宏观形貌、相组成和显微组织,以及不同制度热处理态试样的组织和室温拉伸性能.结果表明,沉积态试样相组成沿沉积高度方向呈现由B2+O+α2→B2+O→B2的变化趋势;热处理态试样的微观组织和相组成均匀,由B2、O、α23相组成;经930℃保温2h空冷的固溶处理和800℃保温24h空冷的时效处理后,合金室温拉伸性能好,抗拉强度为1017MPa,断后伸长率为6.0％.     

基于优化智能网络的发动机推力指令模型

针对航空发动机性能退化缓解控制中推力指令模型输入量有限问题,提出1种双智能网络串联的推力指令建模方法.其中子模型Ⅰ采用BP网络映射与推力密切相关的气路参数,其输出作为子模型Ⅱ的输入;子模型Ⅱ采用优化极端学习机(ELM)算法,输出为额定发动机推力,并以此推力为性能蜕化缓解控制指令.为了减小ELM网络规模,提高推力指令模型实时性,采用微分进化算法(DE)优化ELM初始网络参数.数字仿真验证表明:各飞行包线内推力指令模型预测值最大相对误差小于4‰,远优于单一神经网络最大8.17％和单一极端学习机最大14.5％的误差,模型推力指令计算时间仅需0.64ms,实时性好,验证了该推力指令模型的有效性.     

基于蒙特卡罗方法的冷原子干涉仪物理仿真

由于现有的噪声分析方法无法很好地评估在复杂环境下冷原子干涉仪的输出特性,本文提出了一种新的冷原子干涉仪仿真方法,可以模拟大动态条件下各项噪声及其之间的耦合对冷原子干涉仪的影响。利用单粒子波包演化的处理方式对冷原子干涉仪进行全过程物理建模,并采取蒙特卡罗方法对大量确定初态的原子进行全过程统计,最终得到冷原子干涉仪在多种噪声同时存在的情况下的响应。该方法主要优势体现在能够对噪声耦合情形进行高精度仿真,并且可以根据实际数据对干涉仪输出进行实时处理,以提升冷原子干涉仪的性能指标。     

开放逻辑及其实现技术

定义了一个建立在一阶谓词基础上的开放的逻辑系统,它由证明演算和假设演算组成。本文在文献[1]的基础之上对假设演算进行了某些扩充,使得假设演算中所构造的删除规则集是完备的;并说明了对任一语句的可判定性。为便于机器实现,文中引入了删除推演序列的概念;并给出了如何构造删除规则的与或树以及如何生成删除推演序列的步骤。最后,讨论了开放逻辑系统的具体实现技术。     

Halo White Dwarfs and Baryonic Dark Matter

We describe the formation of hot intergalactic gas along with baryonic remnants in galaxy halos. In this scenario, the mass and metallicity of the hot intracluster and intragroup gas relates directly to the production of baryonic remnants during the collapse of galactic halos. We construct a schematic but self-consistent model in which early bursts of star formation lead to a large remnant population in the halo, and to the outflow of stellar ejecta into the halo and ultimately the Local Group. We consider local as well as high redshift constraints on this scenario. This study suggests that the microlensing objects in the Galactic halo may predominantly be 0.5M white dwarfs, assuming that the initial mass function for early star formation favored the formation of intermediate mass stars with m 1M. However, the bulk of the baryonic dark matter in this scenario is associated with the ejecta of the white dwarf progenitors, and resides in the hot intergalactic medium.