量化拆包的综合显示控制系统软件设计与实现

综合显示处理机与多功能显示器接口模块之间通信采用HDLC传输协议,此时综合显示处理机与多功能显示器字符板模块之间通信采用DF指令格式.但是当画面显示数据的DF指令长度超过HDLC协议设置的带宽或设定的缓存区大小时,综合显示控制系统将无法实现信息显示.为此本文提出了主动量化拆包的解决方法,可支持大数据量显示的综合显示控制...     

基于SOC的ACAS无线电高度信号激励测试的设计

本文介绍了一种以SOC为核心芯片用于机载防撞系统(ACAS)中符合ARINC552A标准无线电高度信号激励测试的软硬件设计方法.采用C8051F020型SOC芯片及OPA552等芯片搭建仿真电路,利用PDIUSBD12接口芯片建立与工控机的通讯,依据ARINC552A标准,用C51编写仿真控制程序,将仿真的ACAS无线...     

航空通信中基于PN码的信道估计算法研究

航空移动通信系统（空空信道）中,大的多径时延和多普勒频移会造成非常严重的符号间干扰,高速宽带下尤为突出,使得传统的频域信道估计算法不得不通过提高运算长度和复杂度来实现性能,而航空通信对实时性的要求使其难以工程实现。本文针对空空信道时延长而衰落小的条件,提出一种基于PN码的时域信道估计算法,连续发送N段m序列作为训练序列...     

复合材料帽形加筋结构稳定性研究

建立了复合材料帽形加筋结构的参数化有限元模型,给出了两种进行层板结合处的模拟计算方法,通过计算得到了模型的屈曲载荷并总结了加筋结构几何参数对结构稳定性的影响,给出了模型的收敛性分析,对比了模型网格密度对于计算结果的影响,找到最佳的网格密度,提高了模型计算的效率和准确性,为实际的结构设计提供了重要参考,为结构分析提供了依据。     

深空通信中继文件传输协议设计

深空通信极远的传输距离导致链路误码率高,使文件的可靠传输需要较多的重传次数,而其传播时延长的特点,进一步加大了文件传输时延。研究以CCSDS(空间数据系统咨询委员会)文件传输协议的存储-转发机制,提出一种R-CFDP(中继型CFDP协议),设计了3种中继"存储-转发"策略,并数学建模推导了R-CFDP协议的文件传输时延理论计算式。仿真证明R-CFDP协议相对于CFDP(CCSDS文件传输协议)协议在传输时延方面具有优势。     

连续体结构拓扑优化方法评述

连续体结构拓扑优化在优化中能产生新的构型,对实现自动化智能结构设计具有重要意义。目前,连续体结构拓扑优化方法主要有：均匀化方法、变厚度法、变密度法、渐进结构优化方法、水平集法、独立连续映射方法。本文首先系统回顾了以上方法的发展历程,介绍了它们的研究现状。其次,通过对比以上拓扑优化方法对若干典型算例的优化结果,表明以上方法都有较好的减重效果。最后,对以上方法进行了总结,列出了它们的优缺点和发展方向。     

航空专用测试设备校准问题的研究

简要介绍了航空专用测试设备的概念,在计量、校准中遇到的问题以及解决问题的途径。     

DEMETER卫星探测到的强震前O^＋浓度变化

利用DEMETER卫星观测数据,采用level-2图像目视解译的方法和重访轨道对比方法,对2006年5月3日发生在汤加群岛的7．9级地震进行分析．从震前6天、震前2天、震前1天和震后2天的level-2图像可看到,电场和等离子体参量在震中上空偏北的位置出现扰动信号,震前的扰动信号幅度随地震时间临近有所增强,扰动持续时间也相应增加;震后2天扰动信号依然存在,其幅度并未减弱．通过对比震前1天的轨道在2006年至2008年内的重访轨道,发现O^＋浓度存在三类较规律的变化特征,即在夏季时,北半球的值高于南半球;冬季时则相反;二分季节时,南北半球含量相当．本文给出了地震和磁暴对O^＋浓度的不同影响,地震影响最靠近震中位置轨道上的O^＋浓度,而磁暴影响全球轨道上O^＋浓度分布．同时获取了DEMETER卫星上朗缪尔探针在上述重访轨道同步探测的电子浓度数据,发现电子浓度与O^＋浓度存在同步增加．等离子体浓度增加的现象可能与地震产生异常电场进而影响电离层结构有关．     

Low-dose carbon ion irradiation effects on DNA damage and oxidative stress in the mouse testis

To investigate the effects of low-dose carbon ion irradiation on reproductive system of mice, the testes of outbred Kunming strain mice were whole-body irradiated with 0, 0.05, 0.1, 0.5 and 1 Gy, respectively. We measured DNA double-strand breaks (DNA DSBs) and oxidative stress parameters including malondialdehyde (MDA) content, superoxide dismutase (SOD) activity, and testis weight and sperm count at 12 h, 21 d and 35 d after irradiation in mouse testis. At 12 h postirradiation, a significant increase in DNA DSB level but no pronounced alterations in MDA content or SOD activity were observed in 0.5 and 1 Gy groups compared with the control group. At 21 d postirradiation, there was a significant reduction in sperm count and distinct enhancements of DSB level and MDA content in 0.5 and 1 Gy groups in comparison with control. At 35 d postirradiation, the levels of DNA DSBs and MDA, and SOD activity returned to the baseline except for the MDA content in 1 Gy (P < 0.05), while extreme falls of sperm count were still observed in 0.5 (P < 0.01) and 1 Gy (P < 0.01) groups. For the 0.05 or 0.1 Gy group, no differences were found in DNA DSB level and MDA content between control and at 12 h, 21 d and 35 d after irradiation, indicating that lower doses of carbon ion irradiation have no significant influence on spermatogenesis processes. In this study, male germ cells irradiated with over 0.5 Gy of carbon ions are difficult to repair completely marked by the sperm count. Furthermore, these data suggest that the deleterious effects may be chronic or delayed in reproductive system after whole-body exposure to acute high-dose carbon ions.     

Characteristics of field line resonance type geomagnetic pulsations and variations of plasmaspheric plasma density distribution

The period of field line resonance (FLR) type geomagnetic pulsations depends on the length of the field line and on the plasma density in the inner magnetosphere (plasmasphere), where field lines are closed. Here as FLR period, the period belonging to the maximum occurrence frequency of the occurrence frequency spectrum (equivalent resonance curve) of pulsations has been considered. The resonance system may be replaced by an equivalent resonant circuit. The plasma density would correspond to the ohmic load. The plasma in the plasmasphere originates from the ionosphere, thus FLR period, occurrence frequency are also affected by the maximum electron density in the ionosphere. The FLR period has shown an enhancement with increasing F region electron density, while the occurrence frequency indicated diminishing trend (possible damping effect). Thus, the increased plasma density may be the cause of the decreased occurrence of FLR type pulsations in the winter months of solar activity maximum years (winter anomaly).