基于CAN总线改进的机车数据采集系统

介绍了基于CAN总线改过的机车数据采集系统.采用内嵌CAN控制器的微处理器(P87C591)来改进传统模拟仪表,使它们成为具有相互通讯能力的智能仪表(节点),通过CAN总线和上位机通讯,对各仪表测量数据采集、存储、分析和管理来监测机车运行状况,保证机车的正常运行.具有记录面广、存储容量大、数据处理灵活等优点,有广泛的应用前景.     

原位合成TiC/Ti基复合材料氧化行为

研究了TiC/Ti基复合材料在550℃,600℃和650℃空气中恒温氧化行为.分析了增强体TiC对钛基复合材料氧化动力学行为的影响,并用X射线衍射仪(XRD)和配有能谱仪(EDS)的扫描电子显微镜(SEM)对氧化层表面的相组成、形貌以及氧化层剖面的显微结构进行了分析.结果表明:TiC/Ti基复合材料的氧化层由金红石型的氧化物TiO2组成;增强体TiC能够提高钛基复合材料的抗氧化性,而且随着TiC增强体含量的增加,钛基复合材料的抗氧化性增加;这主要是因为TiC增强体能够促进致密氧化膜的生成.氧化动力学曲线为抛物线类型.     

涡流管结构参数对其性能的影响

用实验方法研究了热端管管长、分离室直径、冷孔板孔径等主要结构参数对涡流管的制冷制热性能的影响。实验中以空气为介质分别对不同结构参数涡流管的性能进行了研究,得出了热端管管长、分离室直径以及冷孔板孔径等参数对涡流管制冷制热性能的影响规律。研究结果表明:在一定范围内增加热端管长度有利于涡流管的能量分离;在大冷流率下,大直径涡流管的制冷性能优于小直径涡流管;冷孔板孔径愈小,涡流管的制冷制热效应都愈好,在冷孔板孔径与热端管内径之比为50%时,取得最佳的制冷制热效应。      

变截面U形通道内肋高对换热特性影响的实验

采用实验方法研究了在定常状态下, 肋的高度对横肋变截面U形通道内的换热特性的影响。通道内肋间距为15 mm, 肋的宽度均为2 mm, 肋的高度分别为1, 1.5, 2 mm和2.5 mm。雷诺数在12 000到56 000之间变化, 采用单元分析法, 以相同形状的无肋通道作为基准, 研究了肋的高度对肋间距为15 mm通道的换热效果及阻力影响, 得到了包括几何参数在内的经验关联式。结果表明, 有肋的通道换热都得到了增强;肋高度的变化对变截面蛇形通道换热的影响不是单调的, 而是呈多峰分布;肋的高度对阻力系数的影响却是随着肋高的增大而增大的。      

局部催化特性差异对气动热环境影响的计算分析

高温气体非平衡效应及其壁面催化效应对高超声速飞行器气动热环境造成显著影响,是当前高超声速飞行器气动热环境预测和热防护设计的关键问题之一。考虑高温空气离解与电离等化学反应、气体分子热力学激发、流动中的非平衡效应和壁面催化效应,通过数值求解三维热化学非平衡Navier-Stokes方程和壁面处质量、能量平衡关系,完善了高温气体热化学非平衡流场有限催化气动热环境数值计算方法和计算程序,采用典型算例进行了考核验证。在此基础上,开展了不同条件下高超声速飞行器热化学非平衡流场气动热环境数值模拟,分析局部催化特性差异对气动热环境的影响。研究表明：所建立的高超声速飞行器热化学非平衡流场有限催化气动热环境数值计算方法及程序,其数值模拟结果与飞行试验、文献符合;局部催化特性差异会导致热流跳变,其热流跳变量与催化特性差异量、材料分布方式等有关;催化特性差异较大时,局部区域热流可能远远高于飞行器全表面完全催化的热流结果,此时将飞行器在全表面完全催化（FCW）和完全非催化（NCW）条件下的数值模拟结果作为实际飞行过程中表面热流的上、下限这一简化处理方式,是不可取的。     

双流制窄轨电力机车用异步牵引电机设计

将牵引电机应用于双流制窄轨电力机车时,由于窄轨机车轨距小,所以牵引电机安装空间异常狭小,比一般牵引电机在安装空间、电机结构、电磁负荷等方面的要求更加苛刻。针对窄轨双流制电力机车的运用特点和特殊要求进行了分析,提出了牵引电机的设计要求和关键技术难点,并对关键技术难点给出了相应的分析和解决措施。对该牵引电机的制造过程及电机试验测试情况进行了论述。试验结果表明,该牵引电机达到了设计预期,完全能满足设计要求。     

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.     

The gas pixel detector as a solar X-ray polarimeter and imager

The Sun is the nearest astrophysical source with a very intense emission in the X-ray band. The study of energetic events, such as solar flares, can help us to understand the behaviour of the magnetic field of our star. There are in the literature numerous studies published about polarization predictions, for a wide range of solar flares models involving the emission from thermal and/or non-thermal processes, but observations in the X-ray band have never been exhaustive.The gas pixel detector (GPD) was designed to achieve X-ray polarimetric measurements as well as X-ray images for far astrophysical sources. Here we present the possibility to employ this instrument for the observation of our Sun in the X-ray band.     

Fast Probabilistic Particle Identification algorithm using silicon strip detectors

Active detectors used as radiation monitors in space are not usually able to perform Particle Identification (PID). Common techniques need energy loss spectra with high statistics to estimate ion abundances. The ALTEA-space detector system is a set of silicon strip particle telescopes monitoring the radiation environment on board the International Space Station since July 2006 with real-time telemetry capabilities. Its large geometrical factor due to the concurrent use of six detectors permits the acquisition of good energy loss spectra even in a short period of observation. In this paper we present a novel Fast Probabilistic Particle Identification (FPPI) algorithm developed for the ALTEA data analysis in order to perform nuclear identification with low statistics and, with some limitations, also in real time.