Effect of blade tip winglet on the performance of a highly loaded transonic compressor rotor

The tip leakage flow has an important influence on the performance of transonic com-pressor. Blade tip winglet has been proved to be an effective method to control the tip leakage flow in compressor, while the physical mechanisms of blade tip winglet have been poorly understood. A numerical study for a highly loaded transonic compressor rotor has been conducted to understand the effect of varying the location of blade tip winglet on the performance of the rotor. Two kinds of tip winglet were designed and investigated. The effects of blade tip winglet on the compressor over-all performance, stability and tip flow structure were presented and discussed. It is found that the interaction of the tip winglet with the flow in the tip region is different when the winglet is located at suction-side or pressure-side of the blade tip. Results indicate that the suction-side winglet (SW) is ineffective to improve the performance of compressor rotor. In addition, a significant stall range extension equivalent to 33.74% with a very small penalty in efficiency can be obtained by the pressure-side winglet (PW). An attempt has been made to explain the fundamental mechanisms of blade tip winglet in detail.     

高超声速钝头体边界层转捩试验

为研究高超声钝头体边界层转捩以及头部钝度对转捩的影响,在FD-14和FD-14A两座激波风洞中开展了热流、压力扰动和高速纹影显示等综合测量。试验结果表明,转捩雷诺数关于钝度雷诺数的变化显示出转捩反转的趋势。压力扰动的功率谱密度（PSD）分析结果以流向离散分布云图形式显示,边界层高速纹影图像显示了第二模态波的发展、湍流的生成和熵层对边界层结构的显著影响。大头部钝度带来的强熵梯度熵层流动对边界层压力扰动频谱特性和流动结构影响显著,在转捩反转机理中起到重要作用。此外,马赫数对转捩的影响不容忽视。     

基于模型的装备维修性设计控制技术

伴随数字化设计方法日趋成熟,飞机装备维修性设计面临如何与三维数字化设计环境下功能性能设计同步的难题。对比分析了数字化环境维修性设计与传统维修性设计的主要差别,提出了基于飞机装备数字化设计环境维修性设计流程,研究了维修性设计参数的表达模型以及维修性参数信息在三维设计数字环境中的转化、集成与利用方式。基于图论和网络节点框图,提出了一种以节点网络图、单节点维修时间模型、维修过程时间模型为表征的飞机装备维修性设计与控制方法。经实例验证,提出的这套基于数字模型的维修性设计技术,对装备在数字化设计环境下同步开展维修性设计具有一定的工程指导价值。     

脉冲爆震燃烧室出口燃气能量分布特性

为了提高脉冲爆震燃烧室出口燃气能量转换效率,采用数值计算方法,研究了带气动阀和爆震增强结构的脉冲爆震燃烧室出口燃气能量分布特性,结果表明:脉冲爆震燃气的膨胀过程先后经历一次膨胀、二次膨胀和过度膨胀3个阶段,单个周期内二次膨胀阶段的时间和能量占比最大;燃烧室出口燃气压力势能、动能、内能和能流密度的分布主要受燃气压力的影响,且变化规律与燃气压力一致;一次膨胀阶段燃气增加的压力势能、动能、内能分别占单个周期的479%、259%、251%;二次膨胀阶段燃气增加的压力势能、动能、内能分别占单个周期的502%、576%、581%。     

二维三角晶格的Peierls相变前后的声子色散曲面的研究

利用晶格动力学理论计算了二维三角晶格的Peierls相变前后的声子能谱。并且在第一布里渊区绘制了声子色散曲面。通过对Peierls相变前后的声子能谱比较可知，随其对称性降低，声子能谱的简并度被破缺。二维三角晶格的Peierls相变前只有两支声频支声子能谱，Peierls相变后有两支声频支声子能谱与两支光频支声子能谱，并且声频支声子能谱与光频支声子能谱不相交，两支光频支声子沿ky轴平缓地变化。     

Progress of continuously rotating detonation engines

Continuously rotating detonation engine (CRDE) is a focus for concern in the field of aerospace propulsion. It has several advantages, including one-initiation, high thermal efficiency and simple structure. Due to these characteristics, it is expected to bring revolutionary advance-ments to aviation and aerospace propulsion systems and now has drawn much attention throughout the world. In this paper, an overview of the development of CRDE is given from several aspects:basic concepts, applications, experimental studies, numerical simulations, and so on. Representative results and outstanding contributions are summarized and the unresolved issues for further engi-neering applications of CRDE are provided.     

Cosmic ray acceleration by supernova shocks

We analyse the results of recent measurements of nonthermal emission from individual supernova remnants (SNRs) and their correspondence to the nonlinear kinetic theory of cosmic ray (CR) acceleration in SNRs. It is shown that the theory fits these data in a satisfactory way and provides the strong evidences for the efficient CR production in SNRs accompanied by significant magnetic field amplification. Magnetic field amplification leads to considerable increase of CR maximum energy so that the spectrum of CRs accelerated in SNRs is consistent with the requirements for the formation of Galactic CR spectrum up to the energy ∼10¹⁷ eV.     

建构主义教学模式对大学生学习方式影响研究

建构主义教学模式对大学生学习方式有重要影响,通过实证研究方法,研究了课堂环境下建构主义教学模式与大学生学习方式之间的内在关系。研究结果表明：以互动性、自主性为特征的建构主义教学模式与深层学习方式显著正相关,教学模式中的自主性对深层动机和策略的影响均显著高于互动性,且自主性可以更为有效地促使学生采用深层学习方式。     

New evidence for strong non-thermal effects in Tycho’s supernova remnant

For the case of Tycho’s supernova remnant (SNR), we present the relation between the blast wave and contact discontinuity radii calculated within the nonlinear kinetic theory of cosmic ray (CR) acceleration in SNRs. It is demonstrated that these radii are confirmed by recently published Chandra measurements which show that the observed contact discontinuity radius is very close to the shock radius. Therefore a consistent explanation of these observations can be given in terms of efficient CR acceleration which makes the medium more compressible.     

现代远程教育的媒体素材构建方法

本文阐述了媒体素材的采集及处理方法 ,对现代远程教育工程建设可提供有效的帮助