航空发动机数控系统中LVDT传感器信号处理及在线故障检测

通过对线位移差动变压器(LVDT)信号处理电路的深刻研究, 给出了芯片发热、温漂、信号精度等问题的一般解决方法, 提出了一种通过软、硬件结合, 在不增加外围器件的情况下对LVDT传感器进行在线故障检测的定值判断法.发动机台架试验结果表明, 所提出的方法是行之有效的.      

基于遗传算法和空间推进方法的单壁扩张喷管优化设计研究

 将单目标遗传算法和多目标遗传算法（包括NSGA-II和NCGA）,与高效、高精度的空间推进流场数值模拟方法——SSPNS方法相结合,对二维超燃冲压发动机尾喷管即单壁扩张喷管（SERN）进行了气动优化设计研究。在巡航点（Ma=6.0）讨论了推力系数C_T最大单目标模型,推力系数C_T最大升力系数C_L最大两目标模型,以及推力系数C_T最大升力系数C_L最大俯仰力矩系数C_m最小三目标模型,分别得到了喷管的最大推力设计和关于多个目标性能的Pareto最优前沿。结果表明,扩张壁初始扩张角θ_r,i和外罩长度L_c对C_T影响较大;较小的L_c和较大的θ_r,i设计,将降低外罩内表面的负升力作用而使得SERN的C_L较大;较长外罩和较小的θ_r,i,对应Pareto最优设计的C_M较小。     

基于视线角序列的机动目标视线角速率计算

 依据拦截弹与机动目标间的相对位置关系,采用导引头球面模型,基于当前统计模型,实现了强跟踪状态自适应滤波,计算出了可用于制导的视线角速率。该算法利用导引头球面模型,将测角信息转换成距离信息,进行方差自适应调整和卡尔曼滤波。在只给出视线角序列信息的情况下,根据相对状态滤波结果求出所需的视线角速率。     

高维小失效概率下的改进线抽样方法

 针对隐式极限状态方程的可靠性分析,提出了一种基于失效域样本模拟的高效线抽样法。该法采用马尔可夫链来快速得到失效域中的条件样本,利用这些失效域中的样本可以得到线抽样的重要方向,并且这些样本还可以作为线抽样的样本,来得到隐式极限状态方程失效概率的估计值。由于该法可以较准确地得到线抽样方法的重要方向,因此线抽样的效率可以得到提高,另外失效域的样本又可以作为线抽样的样本,从而进一步降低所提方法的计算工作量。算例表明所提算法的计算精度和效率均高于传统线抽样方法。     

China's Space Activities In 2007

THE FOURTH BEIDOU NAVIGATION EXPERIMENTAL SATELLITE LAUNCHED The fourth Beidou experimental navigation satellite was launched into snace aton a LM-3A launch vehicle at Xichang Satellite Launch Center on February 3 at 00:28(Beijing Time).24 minutes later,the satellite separated from the launch vehicle and     

Debut Flight Of LM-3C:Launching Tianlian-1 Successfully

FY-3A,the first satellite of China's new generation of polar-orbiting meteorological satellites,was launched into space atop a modified LM-4C launch vehicle.The satellite separated from the rocket 19 minutes after the takeoff.Flying at an altitude of 807km with an inclination of 98.8 degrees,the satellite circles in polar orbit 14 times everyday,covering the whole globe twice a day. FY-3A has a design lifetime of three years.Weighing 2295kg,the three-axis stabilized satellite is equipped with 11 remote s...     

箭遥时间指令参数实时处理方法研究

火箭遥测数据的实时挑点处理结果是发射中心实时监视火箭飞行状态的重要依据,尤其是时间指令参数的处理结果为判别运载火箭发动机点火、关机、星箭分离等关键事件发生与否提供主要依据。根据某型号运载火箭时间指令参数在遥测帧格式中的波道和码位分配,分析目前箭遥时间指令实时处理方法存在的缺陷,提出"增加判别帧数,充分利用冗余信息",通过分析"时序指令"与"时串指令"间存在的"关联"建立"关联知识库",使用知识库进行辅助判别,实现不错判、不漏判的改进设想。     

Latitudinal variation of the topside electron temperature at different levels of solar activity

A database of electron temperature (T_e) measurements comprising of most of the available satellite measurements in the topside ionosphere is used for studying the solar activity variations of the electron temperature T_e at different latitudes, altitudes, local times and seasons. The T_e data are grouped into three levels of solar activity (low, medium, high) at four altitude ranges, for day and night, and for equinox and solstices. We find that in general T_e changes with solar activity are small and comparable in magnitude with seasonal changes but much smaller than the changes with altitude, latitude, and from day to night. In all cases, except at low altitude during daytime, T_e increases with increasing solar activity. But this increase is not linear as assumed in most empirical T_e models but requires at least a parabolic approximation. At 550 km during daytime negative as well as positive correlation is found with solar activity. Our global data base allows to quantify the latitude range and seasonal conditions for which these correlations occur. A negative correlation with solar activity is found in the invdip latitude range from 20 to 55 degrees during equinox and from 20 degrees onward during winter. In the low latitude (20 to −20 degrees invdip) F-region there is almost no change with solar activity during solstice and a positive correlation during equinox. A positive correlation is also observed during summer from 30 degrees onward.     

A statistical study of C IV regions in 20 Oe-stars

In this paper, using the Gauss-Rotation model (GR model), we analyse the UV C IV resonance lines in the spectra of 20 Oe-stars of different spectral subtypes, in order to detect the structure of C IV region. We study the presence and behavior of absorption clouds and analyse their characteristics. From this analysis we can calculate the values of a group of physical parameters, such as the apparent rotational and radial velocities, the random velocities of the thermal motions of the ions, the Full Width at Half Maximum (FWHM), the optical depth, as well as the absorbed energy and the column density of the independent regions of matter, which produce the main and the satellite clouds of the studied spectral lines. Finally, we present the relations between these physical parameters and the spectral subtypes of the studied stars and we give our results about the structure of the C IV region in their atmosphere.     

Survival and death of the haloarchaeon Natronorubrum strain HG-1 in a simulated martian environment

Halophilic archaea are of interest to astrobiology due to their survival capabilities in desiccated and high salt environments. The detection of remnants of salty pools on Mars stimulated investigations into the response of haloarchaea to martian conditions. Natronorubrum sp. strain HG-1 is an extremely halophilic archaeon with unusual metabolic pathways, growing on acetate and stimulated by tetrathionate. We exposed Natronorubrum strain HG-1 to ultraviolet (UV) radiation, similar to levels currently prevalent on Mars. In addition, the effects of low temperature (4, −20, and −80 °C), desiccation, and exposure to a Mars soil analogue from the Atacama desert on the viability of Natronorubrum strain HG-1 cultures were investigated. The results show that Natronorubrum strain HG-1 cannot survive for more than several hours when exposed to UV radiation equivalent to that at the martian equator. Even when protected from UV radiation, viability is impaired by a combination of desiccation and low temperature. Desiccating Natronorubrum strain HG-1 cells when mixed with a Mars soil analogue impaired growth of the culture to below the detection limit. Overall, we conclude that Natronorubrum strain HG-1 cannot survive the environment currently present on Mars. Since other halophilic microorganisms were reported to survive simulated martian conditions, our results imply that survival capabilities are not necessarily shared between phylogenetically related species.