焊接工艺对钛合金焊接接头冲击韧性的影响

介绍了俄罗斯对钛及其钛合金焊接接头冲击韧性最大值的影响因素的研究工作,以对相关航空研究作参考作用。     

外国电影名称翻译标准

以电影名称的四个主要功能为出发点,提出衡量外国电影名称翻译的四条标准,通过一些成功的外国电影名称翻译证明了该标准的准确性。借助这四条标准对一些不成功的外国电影名称翻译提出了不同的建议。     

倾转旋翼机传动系统多状态响应特性研究

以倾转旋翼机发动机短舱内的传动系统为研究对象,根据设计的传动结构建立了它的动力学模型和动态响应方程,分析了倾转旋翼机旋翼在起降、巡航和过渡三种状态下的激励特性,并针对三种状态下旋翼激励的特点对传动系统动态响应进行了数值求解,最后研究了传动系统中齿轮啮合的动载系数的变化特点,并对系统的共振频率进行了探讨.研究工作对倾转旋翼机的传动系统的可靠性分析和动态优化设计等均有参考意义.      

能量效率准则在导弹拦截系统评估中的应用

将能量效率物理准则引入对导弹系统的评估.系统的效率取决于总的能量资源和对能量流的控制,通过对导弹武器系统形态的描述,给出了能量效率准则在导弹拦截系统中的应用,对于导弹武器系统作战效能评估及实际应用具有参考价值.     

一种基于分组截短PN码的SOFDM信道估计方法

基于PN序列的信道估计方法的特点是计算过程简明,已被广泛应用在地面无线局域网系统中。在卫星正交频分多路复用传输体制(SOFDM)系统中引入传统PN序列信道估计方法的主要问题在于卫星信道的多径延时远大于SOFDM数据符号的持续时间,信道特性比较复杂,使得传统方法的估计精度严重下降。提出了一种改进的方法,根据信道的近似周期特性对数据帧进行合理的等长度分组,并把长PN序列改为短PN码来跟踪信道局部特性的变化,再对分组后的数据子帧分别进行信道估计。对该方法的设计思想进行了理论分析,并通过仿真验证了该方法的估计精度比传统方法至少提高了10倍。     

Solar flux effects on equatorial ionization anomaly and total electron content over Brazil: Observational results versus IRI representations

The F layer critical frequency (foF2) as measured by Digisondes in the equatorial and low latitude locations in Brazil is analyzed to investigate the seasonal and solar flux controls of the intensity of the equatorial ionization anomaly (EIA) in the equinoctial month of March. The analysis also included the total electron content (TEC) as measured by a GPS receiver operated at the EIA crest location. The foF2 data set covered a period of large solar flux variation from 1996 to 2003, while the GPS TEC data was for a period in 2002–2003 when the solar flux parameter F10.7 underwent large variations, permitting in both cases an examination of the solar flux effects on these parameters. The seasonal variation pattern in TEC shows a maximum in equinoctial months and a minimum in June solstice, with similar variations for foF2. The solar flux dependence of the TEC is a maximum during equinoxes, especially for post-sunset TEC values at times when the latitudinal distribution is controlled by the equatorial evening plasma fountain processes. Significant variations with local time are found in the degree of solar flux dependence for both the TEC and EIA. The EIA intensity shows large dependence on F10.7 during post-sunset to midnight hours. These results are discussed in comparison with their corresponding IRI representations.     

A new modeling method of solar energetic proton events for ISO specification

Solar energetic protons degrade performance and reliability of spacecraft systems due to single-event effects, total dose effects and displacement damage in electronics components including solar cells. On designing a solar cell panel, a total fluence of solar energetic protons (SEPs) which cause solar cell damage is needed to estimate power loss of the solar cells over mission life. Nowadays a solar panel area of spacecraft is increasing as spacecraft mission life becomes longer (15–18 years). Thus an accurate SEP model is strongly required for the cost-minimum design from the aerospace industry. The SEP model, JPL-91 proposed by Feynman et al., is currently used widely for solar cell designing. However, it is known that the JPL-91 model predicts higher fluences of protons than values actually experienced in space, especially after 7 years on orbit. In addition, the model is based on several assumptions, and also needs Monte-Carlo simulations for calculating fluences. In this study, we propose a new method for modeling SEPs especially focused on solar cell degradation. The newly-proposed method is empirical, which constructs a model based directly upon proton flux measurement data taken by instruments onboard spacecraft. This method has neither assumptions nor dependence on SEP event selection, both of which are needed in JPL-91. The model fluences derived from this method show lower fluences in longer missions compared to JPL-91. This method has been proposed to ISO (International Organization for Standardization) and has been discussed for a new standard SEP model.     

OFDM系统的自适应低秩信道估计

为了降低正交频分复用OFDM(Orthogonal Frequency division Multiplexing)系统中最小均方误差MMSE(Minimum Mean Square Error)信道估计算法的复杂度,并且改善由于信道的统计特性与先验知识不匹配而导致的MMSE估计性能恶化,提出了一种自适应的低秩信道估计算法.该算法利用信道的时间平均相关取代统计相关,结合了基于特征值分解的低秩建模,从而近似地实现MMSE估计.借助于子空间跟踪,该算法可以自适应地估计信道相关矩阵的主特征空间及噪声方差,以迭代的方式逼近最优的MMSE估计,而且复杂度较低.进一步分析指出基于信道延时子空间跟踪的估计算法是该算法的一种特例,理论分析和仿真结果均表明这种新算法在低信噪比时可以显著改善信道估计的准确性.      

工艺参数对频率选择表面传输特性试验研究

制造加工曲面频率选择表面FSS(Frequency Selective Surface)的工艺参数不同会产生FSS中心谐振频率漂移以及传输系数降低.以有限大平板FSS试件为基础,利用矢量网络分析仪PNA 8363B组成的测试系统,研究了在相同条件下加工工艺、FSS附加导电层以及FSS表面电阻率对有限大平板FSS传输性能的影响规律.结果表明,不同加工方法使得平板FSS的中心谐振频率产生漂移,该差异可能是FSS单元边缘毛刺影响的结果,该影响对FSS在各种入射角条件下的传输损耗等性能也略有影响;导电层表面电阻率对FSS的传输系数有较大影响,方块电阻越大传输系数越低,且FSS中心谐振频率也有差异;附加导电层对FSS传输特性的影响不大.      

MC-CDMA中的RLS-DRMTA算法

多载波码分多址(MC-CDMA)系统是将OFDM技术与CDMA技术结合起来的一种综合技术.MC-CDMA系统中同信道干扰仍然是影响系统性能的主要因素,这就需要使用智能天线来提高系统的性能.介绍一种适用于MC-CDMA系统的自适应阵的盲算法递推最小二乘解扩重扩多目标阵列(RLS-DRMTA)算法,利用扩频码的信息进行波束形成,不需要训练序列,节约了频谱资源;与LS-DRMTA算法相比,RLS-DRMTA算法节省了运算时间;另外仿真表明在正交频分复用(OFDM)解调后进行波束形成,提高了系统的性能;为了降低系统的复杂度,还用到了载波分组技术,但分组技术又会降低系统的性能,所以分组时考虑了系统性能和运算速度的折衷.仿真结果表明RLS-DRMTA算法能使方向图的主波束对准信号方向,而在干扰方向形成零陷,从而达到抑制干扰的目的.