一种微内核分区操作系统C库的适配验证方法

针对传统C库的开发和适配方法存在的局限性问题,提出一种基于微内核架构的嵌入式分区操作系统新C库的适配验证方法,依次对基于微内核架构的嵌入式分区操作系统之上C库的总体部署方案、初始化过程、典型功能模块的适配开发方法进行了详细阐述;搭建相应的硬件测试环境,在恩智浦公司的四种硬件平台上对开发和适配的C库进行了相应的功能测试和验证,提出了三个创新点.     

基于测控系统的质量信息监测系统设计与应用

在测控试验现场,针对测控设备状态和测控数据的质量信息,采用智能自动监测技术对设备和测控数据进行实时监视以及动态分析,提出了科学的异常判决方法和处理方案,开发了试验质量信息综合分析实时监测系统,实现了测控流程智能化管控、测控信息自动分析处理和质量信息自动化管理。在多颗卫星的跟踪验证中,质量信息监测系统对卫星长期管理的宏参数宏配置下发、标校和目标捕获与跟踪等任务过程能够进行准确监视,可以及时监测到测控数据和测控时间的异常并报警,并能够自动生成任务实施登记表等测控质量报表。实验表明,质量信息监测系统软硬件设计完善、状态监测点设置合理、判读测控事件方法有效。     

一种2812内部FLASH程序远程更新的新方法

仿真器连接DSP进行程序升级给软件维护带来巨大麻烦.利用TMS320F2812芯片的内部丰富资源和支持在线编程的特点,介绍一种应用软件远程更新方法.包括一个通用的BOOT程序和两种生成可烧写文件的方法,满足了TMS320F2812产品的应用开发以及更新维护等需求.方法已应用于多个产品研制中,实验结果表明方法操作方便、加载结果稳定可靠.     

测控中的星载计算机快速切换

针对低轨卫星长期管理与测控中的星载计算机所需要的切换、维护的测控时间相对较长的问题,在分析原有主、备星载计算机的时间比对方法的基础上,直接针对备机建立新的时间同步模型,并进行公式推导和理论误差分析;然后建立新的测控事件调度模型,实现时间同步数据与主备机一致性数据的同时注入,优化工作流程,并有效缩短测控时间;最后编写新的遥控作业,在测控中进行实践.应用结果表明,采用新方法可以在一个测控圈次内完成在轨星载计算机的切换与维护,MTTR(Mean Time To Repair,平均恢复时间)小于8 min,时间同步精度优于1 ms,所需测控圈次相对于原方法减少83％以上,适用于在轨卫星长期管理与测控.     

基于I~2C总线的CPU温度监控系统

随着高性能、高功耗器件在嵌入式领域中广泛应用,温度监控已成为高可靠嵌入式领域研究的热点,采用ADI公司的测温电路ADT7461设计了面向高性能PowerPC处理器的温度监控系统。介绍了ADT7461芯片的功能原理,描述了整个硬件电路的结构。在软件部分阐述了I2C总线协议以及基于I2C总线协议实现的ADT7461寄存器读/写基本操作,针对应用中会面临的实际问题给出了具体解决方法。设计方法对于同类温度监控系统设计有一定的参考意义。     

基于ARM的移动机器人红外测距系统的设计

为实现机器人安全蔽障,设计了一种基于S3C2440A微控制器的红外测距系统,具体介绍了该测距系统的硬件结构、软件设计及其工作原理。S3C2440A内部具有8路模拟信号输入的10位ADC,将红外测距系统测得的模拟信号输入,通过A/D转换后输出。     

通用化测控应答机的设计

文章介绍了测控应答机的现状及研究背景，并对研制中的困难及今后的发展需求进行了分析，提出了通用化测控应答机的设计方案及关键技术，可供通用化测控应答机设计和批量生产参考。     

Comparison of peak characteristics of F2 ionospheric layer over Tehran region at a low solar activity period with IRI-2001 and IRI-2007 models predictions

In the present work values of peak electron density (NmF2) and height of F2 ionospheric layer (hmF2) over Tehran region at a low solar activity period are compared with the predictions of the International Reference Ionosphere models (IRI-2001 and IRI-2007). Data measured by a digital ionosonde at the ionospheric station of the Institute of Geophysics, University of Tehran from July 2006 to June 2007 are used to perform the calculations. Formulations proposed by  and  are utilized to calculate the hmF2. The International Union of Radio Science (URSI) and International Radio Consultative Committee (CCIR) options are employed to run the IRI-2001 and IRI-2007 models. Results show that both IRI-2007 and IRI-2001 can successfully predict the NmF2 and hmF2 over Tehran region. In addition, the study shows that predictions of IRI-2007 model with CCIR coefficient has closer values to the observations. Furthermore, it is found that the monthly average of the percentage deviation between the IRI models predictions and the values of hmF2 and NmF2 parameters are less than 10% and 21%, respectively.     

Variation in the ionospheric propagating factor M(3000)F2 at Ouagadougou,Burkina Faso

We use hourly monthly median values of propagation factor M(3000)F2 data observed at Ouagadougou Ionospheric Observatory (geographic12.4°N, 1.5°W; 5.9^o dip), Burkina Faso (West Africa) during the years Januar1987–December1988 (average F10.7 < 130 × 10⁻²² W/m²/Hz, representative of low solar flux conditions) and for January 1989–December1990 (average F10.7 ? 130 × 10⁻²² W/m²/Hz, representative of high solar epoch) for magnetically quiet conditions to describe local time, seasonal and solar cycle variations of equatorial ionospheric propagation factor M(3000)F2 in the African region. We show that that seasonal trend between solar maximum and solar minimum curves display simple patterns for all seasons and exhibits reasonable disparity with root mean square error (RMSE) of about 0.31, 0.29 and 0.26 for December solstice, June solstice and equinox, respectively. Variability Σ defined by the percentage ratio of the absolute standard deviation to the mean indicates significant dissimilarity for the two solar flux levels. Solar maximum day (10–14 LT) and night (22–02 LT) values show considerable variations than the solar minimum day and night values. We compare our observations with those of the IRI 2007 to validate the prediction capacity of the empirical model. We find that the IRI model tends to underestimate and overestimate the observed values of M(3000)F2, in particular, during June solstice season. There are large discrepancies, mainly during high solar flux equinox and December solstice between dawn and local midnight. On the other hand, IRI provides a slightly better predictions for M(3000)F2 between 0900 and 1500 LT during equinox low and high solar activity and equinox high sunspot number. Our data are of great importance in the area of short-wave telecommunication and ionospheric modeling.     

重量的一种遥测式监测系统

本文提出一种重量信号的无线传输和测量方法。重量信号经传感顺转换成电信号，再经Ｖ／Ｆ变换后调频发射，接收信号解调后单片机处理。单片机的信号处理采用电子计数器测频方法，经过计算送显示单元，实现重量信号的遥测。