基于PROFIBUS总线的控制器智能从站设计

针对控制器智能化、网络化的发展趋势,为了使具有RS485/RS232接口的控制器方便地接入PROFIBUS现场总线网络,基于C8051F020单片机,研制了以西门子公司的协议芯片SPC3为基础的PROFIBUS-DP从站。首先介绍了PROFIBUS通信的基本原理,然后详细论述了硬件的几个组成部分的功能,对软件的整体结构及部分模块进行了论述,同时还给出了抗干扰的几种措施,最后给出了实验结果。实验结果表明设备间通信正常,可以应用于设备数据采集、执行和控制等,实现RS485/RS232设备与PROFIBUS现场总线的无缝互联。     

一种多SAM模块的低功耗IC卡读卡器设计与实现

CPU卡可以有效地杜绝IC卡被克隆，防止机密信息被修改，得到广泛使用，每个CPU卡具有相应的SAM(Safe Authentication Module)，不同的CPU卡需要的密钥不同，所以有不同的SAM模块。为了使读卡器能够识别多种CPU卡，提出了通过使用多SAM卡模块的循坏扫描对多种SAM卡进行认证管理，实现渎卡器对不同型号IC卡的支持，使用MSP430F149和多个SAM模块，设汁实现了一种新型IC卡读卡器。详细介绍了IC卡和读卡器的工作原理、功能、硬软件设计。经过测试证明，读卡器具有功耗低、体积小、性能稳定等特点。     

具有电磁屏蔽性能的金属/织物复合材料

用化学镀铜和化学镀镍的方法对纤维织物进行改性,制备出有优良电磁波屏蔽性能的金属 /织物复合材料。该复合织物在 1 0 k Hz～ 1 2 GHz范围内可以获得 50～ 70 d B的优良屏蔽效果和良好的环境稳定性,成本低、结合力好,适用于丝绸、棉布、化纤布和玻璃纤维布等多种织物改性,有良好的应用前景。     

基于FPGA的V/F转换电路温度补偿技术研究

针对温度对V/F转换电路工作性能的影响,分析了主要电子元器件的温度影响因子,阐述了转换电路的温度补偿原理.在电路中采用基于FPGA的数字式温度补偿方案进行温度补偿的标定、设计与试验,结果表明采用数字式温度补偿方式改善了温度因素对V/F转换电路的影响,使得电路满足温度稳定性要求.     

武器用光纤捷联惯导系统温度模型的研究

本文从光纤陀螺仪和加速度计两方面,对武器用光纤陀螺捷联惯导系统温度模型进行研究.论文首先对光纤陀螺仪温度模型构建的一般过程进行研究,并对加速度计及其I/F转换电路板串联系统的物理模型和数学模型进行了分析,最后对组合温度模型进行了实物验证和适应性验证,验证效果良好.     

FJ44发动机关键性能参数趋势分析

以FJ44型发动机为研究对象,选择采集该型发动机的几个关键性能参数,对数据平滑处理后进行趋势分析,监控发动机状态,并为其故障诊断提供参考。     

IC10合金本构关系的神经网络模型

为研究IC10合金在不同温度、不同应变率下的流变规律,本文利用材料试验机(MTS809)测得IC10合金在很宽的温度范围(25~800°C)和不同应变率(10-5~10-2s-1)内的应力-应变曲线。试验结果表明,在小于800°C及小应变率条件下IC10合金的流变行为表现为应变硬化。基于试验数据,本文建立了IC10合金本构关系的BP神经网络模型,该模型以应变值、应变率及温度作为输入量,流变应力为输出量。与试验结果比较表明,BP神经网络模型的预测精度较高,说明该模型可以精确地预测IC10合金在不同温度、不同应变率下的流变行为。     

EB-PVD热障涂层对IC10合金力学性能的影响

采用电弧离子镀技术在IC20合金基体上制备NiCrAlYSi粘结层,利用电子束物理气相沉积（EB—PVD）技术在粘结层上制备YSZ陶瓷面层。研究了YSZ热障涂层对IC10合金拉伸、持久、疲劳性能的影响。结果表明：IC10合金沉积YSZ热障涂层后,980℃／200MPa高温持久寿命与IC10合金相当;900℃高温抗拉强度σb、屈服强度σ0.2、伸长率占和断面收缩率砂与基体相比,基本保持不变;室温抗拉强度σb。屈服强度σ0.2：与基体相比稍有下降;800℃／447MPa疲劳寿命与基体合金相当。因此,IC10合金沉积TBCs涂层后,对IC10合金力学性能无明显影响,不影响合金的实际使用。     

Behavior of the equivalent slab thickness over three European stations

The total electron content (TEC) derived from the global positioning system (GPS) and the F2-layer peak electron density obtained from Digisonde data have been used to study the diurnal, seasonal and solar activity variations of the ionospheric equivalent slab thickness (τ) over three European stations located at Pruhonice (50.0°N, 15.0°E), Ebro (40.8°N, 0.5°E) and El Arenosillo (37.1°N, 353.3°E). The diurnal variation of the τ is characterized by daytime values lower than nighttime ones for all seasons at low solar activity while daytime values larger than nighttime characterizes the diurnal variation for summer at high solar activity. A double peak is noticeable at dusk and at dawn, better expressed for winter at low solar activity. The seasonal variations of τ depend on local time and solar activity, the daytime values of τ increases from winter to summer whereas nighttime values of τ show the opposite. The effect of the solar activity on τ depends on local time and season, there being very sensitive for winter nighttime values of τ. The results of this study are compared with those presented by other authors.     

Comparative study of foF2 measurements with IRI-2007 model predictions during extended solar minimum

The unusually deep and extended solar minimum of cycle 23/24 made it very difficult to predict the solar indices 1 or 2 years into the future. Most of the predictions were proven wrong by the actual observed indices. IRI gets its solar, magnetic, and ionospheric indices from an indices file that is updated twice a year. In recent years, due to the unusual solar minimum, predictions had to be corrected downward with every new indices update. In this paper we analyse how much the uncertainties in the predictability of solar activity indices affect the IRI outcome and how the IRI values calculated with predicted and observed indices compared to the actual measurements. Monthly median values of F2 layer critical frequency (foF2) derived from the ionosonde measurements at the mid-latitude ionospheric station Juliusruh were compared with the International Reference Ionosphere (IRI-2007) model predictions. The analysis found that IRI provides reliable results that compare well with actual measurements, when the definite (observed and adjusted) indices of solar activity are used, while IRI values based on earlier predictions of these indices noticeably overestimated the measurements during the solar minimum. One of the principal objectives of this paper is to direct attention of IRI users to update their solar activity indices files regularly. Use of an older index file can lead to serious IRI overestimations of F-region electron density during the recent extended solar minimum.