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.      

一种多代路径通量分析化学机理简化方法

基于路径通量分析,在考虑组分间直接和间接多代相关反应的基础上,建立了一种新型化学机理简化方法。以预选组分为基础,通过计算预选组分直接参与,以及第二代、第三代和第四代间接参与的所有生成反应与消耗反应中其它组分相对于预选组分的路径通量之和,以此决定相关组分及其所参与反应的取舍。用该多代路径通量分析简化法对甲烷及正庚烷反应机理进行了简化,计算结果与详细化学机理、直接关系图简化法简化结果、二代路径通量分析简化法简化结果进行了对比,结果证明了该多代路径通量分析简化法具有更高的简化精度。多代路径通量分析简化法为反应流模拟中大型化学机理的精确简化提供了一种新的解决思路。     

中南地区协同流量管理系统设计研究

本文从我国民航空管的实际情况出发,指出了我国建设协同流量管理系统的必要性,并以中南地区为例在其现有流量管理系统的基础上,初步规划了中南地区协同流量管理系统的总体构架及建设步骤,详细设计了系统的主要功能程序及其数据处理流程,为完善建设中南地区流量管理系统拓展了思路,为我国空管全面引入协同决策理念提供了借鉴和参考.     

机械系统故障树分析

故障树分析就是基于系统工程分析方法在系统设计过程中,通过对可能造成系统故障的各种因素进行分析,运用离散数学、数理统计方法确定系统的故障率,并找出相应的纠正措施以提高系统可靠性的一种设计方法.     

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。
     

某型导弹伸缩翼展开可靠性评估

与固定翼相比,伸缩翼能够有效减少飞机弹仓的空间占用,但由于伸缩翼存在运动机构,其带来的可靠性下降成为不可忽视的问题。为探究新型机构的可靠度,本文从理论方面计算某型伸缩翼展开机构的定位可靠性;采用 Adams 对伸缩翼展开过程进行仿真,结合 Adams/Insight 模块计算在考虑摩擦力条件下的卡滞可靠性,并对伸缩翼卡滞失效原因进行分析。结果表明：异物的存在使伸缩翼的定位可靠性显著降低,适当增加上下翼弹簧的预载荷能够有效减小伸缩翼展开机构的卡滞失效,上下翼弹簧在上翼质心产生的附加力矩会降低伸缩翼的卡滞可靠性。     

Heat storage and electricity generation in the Moon during the lunar night

One of the biggest challenges of the exploration of the Moon is the survival of the crew and the lunar assets during the lunar night. The environmental conditions on the lunar surface and its cycle, with long periods of darkness, make any long mission in need of specific amounts of heat and electricity to be successful. We have analyzed two different systems to produce heat and electricity on the Moon's surface. The first system consists of Thermal Wadis, sources of thermal power that can be used to supply heat to protect the exploration systems from the extreme cold during periods of darkness. Previous results showed that Wadis can supply enough heat to keep lunar devices such as rovers above their minimum operating temperature (approximately 243 K). The second system studied here is the Thermal Energy Storage (TES), which is able to run a heat engine during the lunar night to produce electricity. When the Sun is shining on the Moon's surface, the system can run the engine directly using the solar power and simultaneously heat a thermal mass. This thermal mass is used as a high temperature source to run the heat engine during the night. We present analytical and numerical calculations for the determination of an appropriate thermal mass for the TES system.     

一种高效低成本的视频压缩方法实现

文章提出了一种基于DSP的高效低成本的视频压缩方法的实现.硬件采用TI公司DM642 DSP,其具有成本低的特点,视频压缩采用MPEG4算法,实现复杂度适中,可高效满足用户需求.文章通过研究DSP的硬件架构,软件上采用调整程序结构、存储器优化、流水线技术、线性汇编等优化方法对移植成功的MPEG4 C语言程序进行优化.经测试,该系统优化前为2秒一帧,经优化后达到了标清25帧每秒的压缩任务,可满足军用或民用视频压缩领域的高效低成本应用需求.     

Equatorial Ionospheric Anomaly (EIA) and comparison with IRI model during descending phase of solar activity (2005–2009)

The ionospheric variability at equatorial and low latitude region is known to be extreme as compared to mid latitude region. In this study the ionospheric total electron content (TEC), is derived by analyzing dual frequency Global Positioning System (GPS) data recorded at two stations separated by 325 km near the Indian equatorial anomaly region, Varanasi (Geog latitude 25°, 16^/ N, longitude 82°, 59^/ E, Geomagnetic latitude 16°, 08^/ N) and Kanpur (Geog latitude 26°, 18^/ N, longitude 80°, 12^/ E, Geomagnetic latitude 17°, 18^/ N). Specifically, we studied monthly, seasonal and annual variations as well as solar and geomagnetic effects on the equatorial ionospheric anomaly (EIA) during the descending phase of solar activity from 2005 to 2009. It is found that the maximum TEC (EIA) near equatorial anomaly crest yield their maximum values during the equinox months and their minimum values during the summer. Using monthly averaged peak magnitude of TEC, a clear semi-annual variation is seen with two maxima occurring in both spring and autumn. Results also showed the presence of winter anomaly or seasonal anomaly in the EIA crest throughout the period 2005–2009 only except during the deep solar minimum year 2007–2008. The correlation analysis indicate that the variation of EIA crest is more affected by solar activity compared to geomagnetic activity with maximum dependence on the solar EUV flux, which is attributed to direct link of EUV flux on the formation of ionosphere and main agent of the ionization. The statistical mean occurrence of EIA crest in TEC during the year from 2005 to 2009 is found to around 12:54 LT hour and at 21.12° N geographic latitude. The crest of EIA shifts towards lower latitudes and the rate of shift of the crest latitude during this period is found to be 0.87° N/per year. The comparison between IRI models with observation during this period has been made and comparison is poor with increasing solar activity with maximum difference during the year 2005.