Ca的掺入对复合氧化物LaFeO3和LaMnO3的结构及电性的影响

用柠檬酸法、固相法制备了替代的复合氧化物Ｌａ１－ｘＣａｘＦｅＯ３及Ｌａ１－ｘＣａｘＭｎＯ３。对样品进行了ＸＲＤ及导电能力测试。结果表明：Ｘ≤０．５,复合氧化物为单相的钙钛矿结构;Ｃａ的掺入,改善了ＬａＦｅＯ３导电性能,使其室温电阻率从６×１０＾４Ω·ｃｍ降低到１０Ω·ｃｍ左右;而对ＬａＭｎＯ３的影响不大,其室温电阻率在１０＾－１Ω·ｃｍ左右。     

TC4钛合金的微动磨损及防护

对Ｔｉ－６Ａｌ－４Ｖ合金在１８℃，１００℃２５０℃下的微动磨损特性及防护工艺进行了研究。表明：该合金微动磨损的主要磨损形式是疲劳脱层，其磨损量随温度升高而下降，高渐微动磨损量与磨损区表面所形成的氧化层的性质及厚度有关。     

CBERS-1卫星CCD相机零级图像处理研究

CCD相机是CBERS - 1卫星上的主要有效载荷之一。利用其接收的可见光和近红外谱段的图像 ,可以在国民经济的各个生产部门 ,诸如国土资源调查、农业、林业、地矿、水利、环境、生态等方面得到广泛应用。但是由于探元和光学系统成像的物理机制和各种干扰等因素影响 ,地面接收到的数据必须经过处理才能应用。文章介绍的内容就是将这种图像数据经图像预处理 ,得到零级图像 ;经过相应的辐射校正 ,得到一级图像 ;经过几何校正 ,得到二级图像产品 ,提供给其它部门加以应用     

测量机连续扫描控制系统设计

利用UCC1控制器作为核心,构建具有三维空间连续扫描功能的测量机控制系统的方法,并简要介绍了UCC1控制器的功能及控制系统硬件电路的设计。     

BMCMC法分析2009年墨西哥H1N1流感病毒与中国流感病毒的进化关系

从GenBank上下载所有1978-2009年在中国分离的H1N1亚型流感病毒的HA和NA基因及所有同期在中国分离的A型流感病毒(宿主包括人、猪和禽)的PB1、PB2、PA、NS、NP和M基因的序列,将这些基因序列与2009年在中国发生的墨西哥H1N1流感病毒的对应基因序列进行BMCMC法分析,绘制BMCMC进化树,结果揭示中国发生的墨西哥H1N1流感病毒的HA和NA基因相对独立于中国季节性H1N1流感病毒;M基因相对独立于中国国内的季节性流感病毒和禽源流感病毒;PB1基因包含在季节性流感病毒的分群内;PB2基因和NS基因与国内重排的流感病毒相关,但相对独立于国内的季节性流感病毒和禽源流感病毒;PA基因包含在国内禽流感病毒的分群内;NP基因则与国内传统的猪流感病毒相关,但相对独立于国内的季节性流感病毒和禽源流感病毒.     

Deep Impact: Working Properties for the Target Nucleus – Comet 9P/Tempel 1

In 1998, Comet 9P/Tempel 1 was chosen as the target of the Deep Impact mission (A’Hearn, M. F., Belton, M. J. S., and Delamere, A., Space Sci. Rev., 2005) even though very little was known about its physical properties. Efforts were immediately begun to improve this situation by the Deep Impact Science Team leading to the founding of a worldwide observing campaign (Meech et al., Space Sci. Rev., 2005a). This campaign has already produced a great deal of information on the global properties of the comet’s nucleus (summarized in Table I) that is vital to the planning and the assessment of the chances of success at the impact and encounter. Since the mission was begun the successful encounters of the Deep Space 1 spacecraft at Comet 19P/Borrelly and the Stardust spacecraft at Comet 81P/Wild 2 have occurred yielding new information on the state of the nuclei of these two comets. This information, together with earlier results on the nucleus of comet 1P/Halley from the European Space Agency’s Giotto, the Soviet Vega mission, and various ground-based observational and theoretical studies, is used as a basis for conjectures on the morphological, geological, mechanical, and compositional properties of the surface and subsurface that Deep Impact may find at 9P/Tempel 1. We adopt the following working values (circa December 2004) for the nucleus parameters of prime importance to Deep Impact as follows: mean effective radius = 3.25± 0.2 km, shape – irregular triaxial ellipsoid with a/b = 3.2± 0.4 and overall dimensions of ∼14.4 × 4.4 × 4.4 km, principal axis rotation with period = 41.85± 0.1 hr, pole directions (RA, Dec, J2000) = 46± 10, 73± 10 deg (Pole 1) or 287± 14, 16.5± 10 deg (Pole 2) (the two poles are photometrically, but not geometrically, equivalent), Kron-Cousins (V-R) color = 0.56± 0.02, V-band geometric albedo = 0.04± 0.01, R-band geometric albedo = 0.05± 0.01, R-band H(1,1,0) = 14.441± 0.067, and mass ∼7×10¹³ kg assuming a bulk density of 500 kg m⁻³. As these are working values, {i.e.}, based on preliminary analyses, it is expected that adjustments to their values may be made before encounter as improved estimates become available through further analysis of the large database being made available by the Deep Impact observing campaign. Given the parameters listed above the impact will occur in an environment where the local gravity is estimated at 0.027–0.04 cm s⁻² and the escape velocity between 1.4 and 2 m s⁻¹. For both of the rotation poles found here, the Deep Impact spacecraft on approach to encounter will find the rotation axis close to the plane of the sky (aspect angles 82.2 and 69.7 deg. for pole 1 and 2, respectively). However, until the rotation period estimate is substantially improved, it will remain uncertain whether the impactor will collide with the broadside or the ends of the nucleus.     

优化的GM(1,1)模型及其适用范围

在已有灰色理论的基础上,利用“最小二乘法”确定GM(1,1)白化权函数的时间响应函数中的常数c,摈弃了传统GM(1,1)把原始序列中x^(0)(1)作为初始条件的欠科学的做法,构建了时间响应函数的优化模型。经大量的数据模拟和预测,发现优化的GM(1,1)模型各项指标均优于传统的GM(1,1)模型,且拓宽了其适用范围。     

嫦娥一号卫星撞月时刻与坐标精确分析

针对CE-1卫星精确的撞月时刻与撞月点坐标,首先通过探测器载波信号的本地相关处理技术,精确分析了载波信号在VLBI各测站的消失时刻,进而推算了卫星的撞月时刻;通过实时单向多普勒频移测量的事后分析,核实了卫星撞月过程中的飞行姿态演化;最后结合VLBI互相关时延与测距资料,经定位归算确定撞月点坐标。分析表明,CE-1卫星撞月时刻的误差为±5μs,撞月点坐标月面切向和三维定位误差分别约为0.274km和0.319km(1σ)。     

非线性逆在ASTOVL控制系统中的应用

研究了先进短距起飞垂直着陆飞机（ASTOVL）的飞行／推进控制系统的控制律，基于解和掌握气动舵面和推力矢量舵面控制下的飞机数学模型，应用非线性动态逆理论，为ASTOVL飞机从巡航到悬停阶段的飞行，设计了推力矢量控制器和俯仰控制器，以合理地分配飞机上的力和力矩，使得俯仰姿态速度和法向速度的控制在推进系统性能包括线范围内是近似线性和解耦的，最后以ASTOVL飞机悬停阶段的数字仿真曲线为例，证明了所设计的两个控制器是可行的，基本上达到了设计要求。     

北斗／罗兰-C组合定位技术

“北斗一号”是我国的卫星导航系统,其有源定位模式使其很难得到广泛应用。为此,提出了一种北斗／罗兰-C组合定位方案以实现无源定位。该方案利用“北斗一号”两颗卫星和地面罗兰-C台站获得的距离差信息实现双曲线相交定位。仿真结果表明,该方案的精度可以满足一般定位要求,具有较强的实用性。