Aermet100钢制坯工艺对微观组织和力学性能的影响

针对Aermet100钢研究了大规格棒材锻造工艺对微观组织和力学性能的影响.研究结果表明:细化锻造过程的晶粒度有利于获得较高的断裂韧度.细化晶粒度的途径主要有锻造加工温度控制在再结晶区间和增大总变形比.Aermet 100钢锻造温度区间应控制在950～1100℃之间进行,终锻温度控制在950～1000℃;总变形比之和应大于20.     

A-100钢电子束熔丝成形件超声相控阵检测应用初探

初步研究了超声相控阵检测技术在A-100钢电子束熔丝成形制件中的应用.结果表明:超声相控阵检测技术在A-100钢电子束熔丝成形制件微裂纹检测和大厚度制件检测中有较好的应用效果;与成形路径等因素相关的微观组织结构对检测技术的应用有较大影响;超声波入射方向和角度选择对微裂纹的识别非常关键;制件内部微裂纹存在与平行于逐层生长方向的某端面呈现小倾角或近似平行的断续拐弯状的分布趋势.     

一种较简单的低循环疲劳寿命预测法

 <正> 1。引言 局部应力应变法是目前预测结构裂纹起始寿命的一种行之有效的方法。根据局部应力应变法的原理,可以用计算的方法来预测构件裂纹起始寿命。在计算中,从载荷谱得到局部应变谱,可利用有限元法分析结构的局部应力应变响应。当然还可利用半经验公式(如Neuber法等)。在计算中若考虑材料的记忆特性和循环σ-ε曲线,这无疑对真实地反映受载构件的局部应力应变响应是有利的。但要做到这一点,用有限元分析所需的机时相当可观,因为它要对整个寿命期间的载荷历程进行分析计算,至少也要针对一个典型谱分析计算。 计算中材料的循环应力应变曲线一般可采用下式     

Modeling M(3000)F2 based on extreme learning machine

This paper presents an novel extreme learning machine (ELM)-based prediction model for the ionospheric propagation factor M(3000)F2 at Darwin station (12.4°S, 131.5°E; −44.5°dip) in Australia. The proposed ELM model is trained with hourly daily values of M(3000)F2 from the period 1998–2014 except 2001 and 2009. The hourly daily values of 2001 (high solar activity) and 2009 (low solar activity) are used for validating the prediction accuracy. The proposed ELM for modeling M(3000)F2 can achieve faster training process and similar testing accuracy compared with backward propagation neural network (BPNN). In addition, the performance of the ELM is verified by comparing the predicted values of M(3000)F2 with observed values and the international reference ionosphere (IRI −2016) model predicted values. Based on the error differences (the root mean square error (RMSE) and the M(3000)F2 percentage improvement values M(3000)F2_IMP(%)), the result demonstrates the effectiveness of the ELM model compared with the IRI-2016 model at hourly, daily, monthly, and yearly in high (2001) and low (2009) solar activity years. The ELM also shows good agreement with observations compared with the IRI during disturbed magnetic activity.     

Investigation of Satellite Trace (ST) and Multi-reflected Echo (MRE) ionogram signatures and its possible correlation to nighttime spread F development from Cyprus over the solar mini-max (2009–2016)

Multi-reflected echoes (MREs) and satellite traces (STs) are referred in literature as ionogram signatures of Travelling Ionospheric Disturbances (TIDs) which is a phenomenon that apparently drives spread F development mainly at nighttime mid-latitude ionosphere. A long-term statistical study has been undertaken to investigate the morphological aspect of these signatures over the lower midlatitude European station of Nicosia, Cyprus (35.19°N, 33.38°E geographic; magnetic dip. 29.38°N) by inspecting all ionograms recorded by the DPS-4D digisonde in the interval 2009–2016. The results underline the systematic manifestation of these TID signatures over Cyprus with a possible (although not quite clear) solar activity dependence and a distinctive seasonal and diurnal occurrence rate with a seasonal peak of STs during summer and of MREs during January to April. Based on the experimental results of the present study, the seasonal occurrence rate of MREs and STs is found to increase by 75% and 56% during high solar activity periods. Satellite traces are well known ionogram signatures of TIDs and mostly correlated to the nighttime spread F formation. The occurrence of mid-latitude spread Fs over European longitude sector normally increases during summer. The occurrences of TIDs are also prominent at this interval of the year over nighttime mid-latitude ionosphere. The presence of MREs as an ionogram signature of TIDs over mid-latitude ionosphere is unique in nature.     

Space Weather in the Equatorial Ionosphere

The ‘scintillations’ observed on signals received in the equatorial region from GPS satellites are due to plasma instabilities in the F region of the ionosphere, also detected as spread F. These instabilities give rise to depletions of ionisation or ‘bubbles’. The occurrence of these events and their relation to the equatorial electrojet are reviewed. Possibilities of short-term forecasting are examined with particular attention to problems encountered in modelling the equatorial electrojet. This revised version was published online in August 2006 with corrections to the Cover Date.     

基于TMS320F2812生成移相PWM的2种办法

移相 PWM波是很多开关电源常用的驱动脉冲信号。双向全桥直流变换器(Bidirectional-Full-Bridge DCDC Converter,BDC)在双重移相控制方式下时需要 4组两两互补的移相 PWM波。文章基于 TMS320F2812型 DSP(Digital Signal Processor)分析了 2种生成移相 PWM的方法。为提高双向全桥直流变换器工作的安全性和可靠性,为移相 PWM波设置死区时间。对所提出的方法进行测试后结果良好,对于双向全桥直流变换器闭环控制系统的构建具有重要意义。     

Effect of the seed perturbation amplitude on the equatorial spread F initiation during solar minimum

The contribution of gravity wave (GW) to the initiation/development of spread F during a solar minimum year was investigated through the comparison of the observed precursory parameters and characteristics of the corresponding equatorial spread F (ESF) events. The ionospheric parameters were recorded at the magnetic equatorial station Sao Luis (2.3°S, 44°W, dip latitude 2°S) during March and October 2010. These data were used to estimate the influence of the relative gravity wave amplitude and the ambient ionospheric condition on the diurnal variation of the spread F initiation. The vertical velocity drift indicated a clear control and defines the threshold for the seasonal variability of the ESF occurrence. However, it was insufficient to solely determine or predict the day to day variation of ESF occurrence. Thus, few days with contrasting ambient ionospheric condition and magnitude of GW amplitude were analysed in order to investigate the role of the different precursory factors in the observed diurnal variation of the plasma irregularity development. The density scale length and gravity wave amplitude were shown to immensely contribute to the linear instability growth rate, especially during the days with a low post-sunset rise. Thus, the experimental observations have demonstrated the strong inter-dependence between the precursory factors and they have also highlighted the probable control of the ESF morphology.     

固液动力探空火箭箭载数据采集系统设计

针对固液动力探空火箭在进行测试、飞行试验时,需要实时测量并记录推力、燃料供给速率以及吹除系统工况信息的问题,设计并工程实现了对箭载重要设备输出信号进行监控和采集记录的数据采集系统.以STM32F103RB微控制器为核心,完成了数据采集、存储、传输等电路的设计,并在Real View MDK集成开发环境下,运用C语言完成了控制、测试程序的编写.最后,通过Real View ULINKR仿真器实现了软硬件的联合测试,验证了系统的供电控制、采样频率、工况记录等功能都满足设计要求,完成了对箭载重要设备监控和采集记录的任务.只需修改微控制器内的操控程序,就可将此数据采集系统应用于不同型号的固液动力探空火箭.      

基于TMS320F2812的CAN总线接口通用电模拟器研制

基于TMS320F2812及其内置CAN总线控制器,开发了一套适合多种CAN总线接口配置要求 的通用电模拟器硬件系统,用于某型卫星地面电联试系统中敏感器电模拟器的研制,取得了 良好效果。该电模拟器硬件系统具有CAN总线接口配置灵活、数据处理能力强、应用程序开 发方便、通用性强等特点,可用于卫星地面电联试系统中的多种电模拟器开发研制。