TC11合金高温变形行为及其机理

采用Gleeble-1500热模拟机研究了TC11合金在800～1 050℃、应变速率0.005～5/s条件下的高温变形行为.根据动力学分析,确定了不同温度区间的热激活能和热变形方程.结合变形微观组织观察确定了TC11合金的高温变形机制.结果显示:TC11合金在(α β)两相区和β相区的热变形激活能分别为285.38和141.98 kJ/mol,表明不同温度区间的热变形机理不同;在两相区变形主要发生片状组织的球化,在β相区变形时低应变速率下(0.005～0.05/s)主要发生β相的动态再结晶,高应变速率下(0.05～5/s)主要发生动态回复.研究结果为确定该合金的最佳变形工艺参数提供了理论依据.     

AZ91镁合金搅拌摩擦加工后的组织与性能

采用400rpm-100mm/min,800rpm-100mm/min,800rpm-200mm/min三种工艺参数对铸态AZ91镁合金进行搅拌摩擦加工(FSP)处理,并对合金加工前后的显微组织和拉伸性能及微观断裂机制进行分析。结果表明,经800rpm-100mm/min工艺FSP处理后,合金的显微组织明显细化,延伸率和抗拉强度显著提高,综合拉伸性能最好,且拉伸断口主要表现为韧性断裂的特征。这主要是由于在FSP过程中合金发生动态再结晶,使合金晶粒显著细化及粗大β相的溶解和破碎所致。     

发动机线性模型在动态过程中的应用研究

本文分析了发动机线性模型在动态过程中的应用研究,建立了发动机线性变参数模型,并进行了仿真验证,获得了较好的动态性能。这样,在发动机整个工作过程中,可通过线性变参数模型将发动机的稳态和动态过程描述出来,方便了控制器的设计。     

镁合金在卫星铝蜂窝夹层结构板中的应用

为满足卫星轻量化的要求,选用轻质合金替代卫星铝蜂窝夹层结构板中的铝合金埋件.对比铝-铝、碳/环氧-镁和铝-镁的剪切试验和拉脱试验的试验结果,结合卫星铝蜂窝夹层结构板的结构特点,分析镁合金埋件替代铝合金埋件的可行性.     

应用PIV技术测试模型环形燃烧室流场

采用粒子图像测速仪(PIV)测量带双级旋流器模型环形燃烧室内冷态和燃烧流场,试验研究不同进口气流温度对其冷态和燃烧流场内回流区的形成以及气流速度分布的影响,试验结果表明:燃烧室燃烧流场内回流区长度要比冷态流场短,燃烧流场的脉动速度明显大于冷态流场;另外随着进口气流温度增加,燃烧室冷态和燃烧流场的回流区长度都稍有减少.      

无轴承开关磁阻电机平均悬浮力控制策略

 无轴承开关磁阻电机是一个复杂的非线性系统,因此其控制策略的研究非常重要。高速时由于反电势的增加,使悬浮绕组开通时刻电流难以跟踪,导致瞬时悬浮力难以控制,因此有必要研究基于平均悬浮力和平均转矩的无轴承开关磁阻电机控制策略。根据无轴承开关磁阻电机的悬浮原理和数学模型,设计平均悬浮力和平均转矩的控制策略。主绕组电流和悬浮绕组电流均采用方波控制。推导了平均悬浮力与绕组电流之间的关系,以及主绕组电流和悬浮绕组电流的计算公式。给出了超前角和绕组电流的计算流程。针对12/8结构的无轴承开关磁阻电机,设计了以数字信号处理器TMS320C2812为核心的控制系统。通过实验给出了绕组电流波形和转子位移波形。实验结果显示了电机的稳定悬浮,验证了此控制策略的可行性。     

The Plasma and Suprathermal Ion Composition (PLASTIC) Investigation on the STEREO Observatories

The Plasma and Suprathermal Ion Composition (PLASTIC) investigation provides the in situ solar wind and low energy heliospheric ion measurements for the NASA Solar Terrestrial Relations Observatory Mission, which consists of two spacecraft (STEREO-A, STEREO-B). PLASTIC-A and PLASTIC-B are identical. Each PLASTIC is a time-of-flight/energy mass spectrometer designed to determine the elemental composition, ionic charge states, and bulk flow parameters of major solar wind ions in the mass range from hydrogen to iron. PLASTIC has nearly complete angular coverage in the ecliptic plane and an energy range from ～0.3 to 80 keV/e, from which the distribution functions of suprathermal ions, including those ions created in pick-up and local shock acceleration processes, are also provided.     

The THEMIS Array of Ground-based Observatories for the Study of Auroral Substorms

The NASA Time History of Events and Macroscale Interactions during Substorms (THEMIS) project is intended to investigate magnetospheric substorm phenomena, which are the manifestations of a basic instability of the magnetosphere and a dominant mechanism of plasma transport and explosive energy release. The major controversy in substorm science is the uncertainty as to whether the instability is initiated near the Earth, or in the more distant >20 Re magnetic tail. THEMIS will discriminate between the two possibilities by using five in-situ satellites and ground-based all-sky imagers and magnetometers, and inferring the propagation direction by timing the observation of the substorm initiation at multiple locations in the magnetosphere. An array of stations, consisting of 20 all-sky imagers (ASIs) and 30-plus magnetometers, has been developed and deployed in the North American continent, from Alaska to Labrador, for the broad coverage of the nightside magnetosphere. Each ground-based observatory (GBO) contains a white light imager that takes auroral images at a 3-second repetition rate (“cadence”) and a magnetometer that records the 3 axis variation of the magnetic field at 2 Hz frequency. The stations return compressed images, “thumbnails,” to two central databases: one located at UC Berkeley and the other at the University of Calgary, Canada. The full images are recorded at each station on hard drives, and these devices are physically returned to the two data centers for data copying. All data are made available for public use by scientists in “browse products,” accessible by using internet browsers or in the form of downloadable CDF data files (the “browse products” are described in detail in a later section). Twenty all-sky imager stations are installed and running at the time of this publication. An example of a substorm was observed on the 23rd of December 2006, and from the THEMIS GBO data, we found that the substorm onset brightening of the equatorward arc was a gradual process (>27 seconds), with minimal morphology changes until the arc breaks up. The breakup was timed to the nearest frame (<3 s) and located to the nearest latitude degree at about ±3^oE in longitude. The data also showed that a similar breakup occurred in Alaska ～10 minutes later, highlighting the need for an array to distinguish prime onset.     

高空高速液体燃料亚燃冲压发动机动力特性研究

本文介绍了一种液体燃料亚燃冲压发动机的变比热性能计算方法,并对某型亚燃冲压发动机进行了性能计算,分析讨论了设计参数对发动机性能的影响.本文计算方法可用于液体燃料亚燃冲压发动机总体方案设计阶段的参数选择和性能分析.     

仪器收发系统瓶颈问题解决方案研究

在计量技术机构的仪器收发系统中,仪器信息的录入是比较繁琐的过程。对于每次几十台甚至上百台的送检仪器,采用传统的手动录入方式耗时长、效率低,成为制约仪器收发效率的瓶颈问题。通过对目前仪器收发系统信息录入常用的数据库技术、网络技术、条形码技术进行分析归纳,提出了一种基于软件录入技术的实现方案,所介绍的方法可以实现仪器收发过程中的信息快速录入,较大程度上提高了仪器收发效率,缩短了委托方的等待时间,有效降低了工作中的差错。