电子技术课程教学方法探讨

电子技术基础是一门理论性与实践都比较强的一门课程,探索适时的教学途径是电子技术专业教员必须考虑的问题,本文就电子技术基础课程教学方法进行了探讨。     

Solar cycle and latitude dependence of high-beta suprathermal plasma conditions in interplanetary space between 1.3 and 5.4 AU

The analysis of energetic particles and magnetic field measurements from the Ulysses spacecraft has shown that in a series of events, the energy density contained in the suprathermal tail particle distribution is comparable to or larger than that of the magnetic field, creating conditions of high-beta plasma. In this work we analyze periods of high-beta suprathermal plasma occurrences (β_ep > 1) in interplanetary space, using the ratio (β_ep) of the energetic particle (20 keV to ∼5 MeV) and magnetic field energy densities from measurements covering the entire Ulysses mission lifetime (1990–2009) in order to reveal new or to reconfirm some recently defined interesting characteristics. The main key-results of the work are summarized as follows: (i) we verify that high-beta events are detected within well identified regions corresponding mainly to the vicinity of shock surfaces and magnetic structures, and associated with energetic particle intensity enhancements due to (a) reacceleration at shock-fronts and (b) unusually large magnetic field depressions. (ii) We define three considerable features for the high-beta events, concentrated on the next points: (a) there is an appreciable solar-activity influence on the high-beta events, during the maximum and middle solar-cycle phase, (b) the annual peak magnitude and the number of occurrences of high events are well correlated with the sunspot number, (c) the high-beta suprathermal plasma events present a spatial distribution in heliographic latitudes (HL) up to ∼±80°, and a specific important concentration on the low (−25° ? HL < −6°, 6° < HL ? 25°) and median (−45° ? HL < −25°, 25° < HL ? 45°) latitudes. We also reconfirm by a statistical analysis the results of Marhavilas and Sarris (2011), that the high-beta suprathermal plasma (β_ep > 1) events are characterized by a very large parameter β_ep (up to 1732.5), a great total duration (406 days) and a large percentage of the Ulysses-mission lifetime (which is equal to 6.34% of the total duration with usable measurements, and 11.3% of the duration in presence of suprathermal particles events).     

梯型螺纹量规在航天产品检测中的应用

介绍了梯形螺纹量规的的工艺性能,从外观、相互作用、螺距半角和中径的测量等方面分析了梯形螺纹量规检测技术,并对其应用规划加以阐述,以提升航天军工产品的工艺技术水平和使用可靠性。     

航天光学遥感器光学装调技术现状与展望

航天光学遥感器工作于太空中,长期恶劣的空间环境及短暂发射入轨时的状态对光学系统的设计与装调提出了苛刻的要求,确保光学系统在轨像质优异是航天光学遥感器研制的关键技术.文章结合国际上航天光学遥感器的发展需求对光学系统装调技术及发展现状进行了分析、总结,提出了中国后续航天光学遥感器装调与测试技术的突破方向.     

Plasma and electromagnetic wave simulations of meteors

Every day billions of meteoroids impact and disintegrate in the Earth’s atmosphere. Current estimates for this global meteor flux vary from 2000 to 200,000 tons per year, and estimates for the average velocity range between 10 km/s and 70 km/s. The basic properties of this global meteor flux, such as the average mass, velocity, and chemical composition remain poorly constrained. We believe much of the mystery surrounding the basic parameters of the interplanetary meteor flux exists for the following reason, the unknown sampling characteristics of different radar meteor observation techniques, which are used to derive or constrain most models. We believe this arises due to poorly understood radio scattering characteristics of the meteor plasma, especially in light of recent work showing that plasma turbulence and instability greatly influences meteor trail properties at every stage of evolution. We present our results on meteor plasmas simulations of head echoes using particle in cell (PIC) ions, which show that electric fields strongly influence early stage meteor plasma evolution, by accelerating ions away from the meteoroid body. We also present the results of finite difference time domain electromagnetic simulations (FDTD), which can calculate the radar cross section of the simulated meteor plasmas. These simulations have shown that the radar cross section depends in a complex manner on a number of parameters. These include the angle between radar and meteor entry, a large dependence on radar frequency, which shows that for a given meteor plasma size and density, the reflectivity as a function of probing radar frequency varies, but typically peaks below 100 MHz.     

浅谈量块新标准的变化

介绍了量块新标准与旧标准的差异和新标准变化的原因、目的及其对量块加工带来的影响。     

高速走丝电火花线切割表面条纹的成因研究

分析了高速走丝电火花线切割加工时可通过电极丝空间位置稳定性的改善及选用具有良好洗涤能力的工作介质进行条纹消除的机理.并研究指出在大能量切割时,选用复合工作液以喷射的方式进行冷却,可以大大提高极间的洗涤性能,达到消除表面烧伤纹的目的.     

基于分布式管理架构的应用型网管系统的设计与研究

根据当前IT应用的普及情况,分析了大中型企业中网络资源管理存在的问题,研究了网管软件的相关技术并设计了一套符合当前应用需求的分布式管理架构的应用型网管系统。该系统不但可监测各类操作系统的性能,还可对数据库、WEB服务等应用服务器的性能进行监控。结合网管软件的发展动态,展示了该应用型网管系统的工程应用价值。     

战术导弹折叠翼两种展开方法及测试结果比较

为了满足型号设计的需要,掌握战术导弹折叠尾翼在发射初始时的展开特性,对两种折叠翼快速展开的测试技术进行了试验研究。详细说明了两种测试方法的原理、测试量之间的比较、测试结果的分析。两种方案均在北京空气动力研究所(BIA)的一座低速风洞中进行了多次重复试验比较,测试结果表明两种方法均成熟可靠,可以用于战术导弹的实际设计中。     

探索教改途径 促进教改深化——我院机制工艺专业教改总结与探讨

我院机制工艺专业改革试点工作已走过了五个循环。通过对毕业生跟踪调查，试点专业毕业生的确表现出许多优异之处，受到用人单位的好评，但同时也发现还存在一些不足，本文提出了改进建议。