基于最小二乘滤波起始的机动目标被动跟踪方法

针对仅有量测角的机动目标跟踪给出了基于最小二乘法的滤波器起始方法。该方法减少了伪量测估计方法的估计偏差,同时克服了基于最大似然估计算法计算复杂和容易陷入局部极值点的不足。该起始算法与交互式多模型(IMM)算法相结合实现了对机动目标的被动跟踪。计算机仿真验证了该方法的有效性。     

粉煤灰负载TiO2 光催化剂制备及降解亚甲基蓝研究

以粉煤灰为载体,采用溶胶-凝胶法一步合成负载型TiO_2光催化剂,通过SEM、UVVis、XRD对样品进行了表征,并进行了可见光催化降解亚甲基蓝试验,结果显示,Fe的掺杂能抑制TiO_2晶粒的生长,在700 W氙灯下光照120 min,0. 15 g TiO_2:0. 7wt%Fe光催化剂可使30 mL(5 mg/L)的亚甲基蓝溶液脱色95%。     

基于挠度法的有侧移框架临界力计算方法

针对规范计算长度系数法计算框架稳定时,无法考虑同层柱之间的相互支援以及层与层的支援作用的问题,提出一种基于挠度法求解有侧移框架临界力的计算方法.利用挠度法将求解压杆临界力转化为计算压杆挠度这一基本原理,将有侧移框架临界力的求解转化为计算框架的楼层侧移,推导了单层及多层框架结构临界力的计算公式.研究结果表明:算例计算结果和有限元计算结果符合较好,证明这种方法具有较好的精度及准确性,且能够有效地改进规范计算长度系数法无法考虑这两种支援作用的不足,可供工程设计和理论计算使用.     

基于静力学模型对系泊系统参数设计的研究

针对系泊系统中铁桶倾斜角度、锚链形状、浮标的吃水深度和游动区域等参数的设计问题,通过运用物体受力平衡条件、结构微分原理,构建了系泊系统的静力学、基于微分方程的悬链线模型。综合使用了Lingo、Matlab软件编程,求解系泊系统中倾斜角度、锚链形状、浮标的吃水深度和游动区域的大小,探讨系泊系统在不同海面风速条件下的系统形态,绘制出锚链形状曲线图,使水声通讯设备的工作效果达到最佳状态。     

基于模拟退火遗传算法的电液伺服马达超低速性能

针对电液伺服马达超低速运行时局部爬行及振荡现象,分析了密闭工作容腔内流量及压力的连续特性,采用了自适应改进模拟退火遗传算法,对马达超低速性能结构进行寻优解算,得出马达定子预过渡曲线及其包角范围和配油三角缓冲槽理论公式及最佳尺寸.通过仿真及实验研究,结果表明,该方法可以将遗传算法全局规划能力与模拟退火法局部优化特性进行有效结合,并具有良好的邻域特性和初值鲁棒性,其优化结果能够保证新型连续回转电液伺服马达跟踪0.001 °/s超低速斜坡信号和满足0.001 °的公差带要求.     

视觉假体铂铱合金微电极阵列的电场分析

采用有限元法研究用于视神经视觉假体铂铱合金微电极阵列的电场分布情况,在单极和双极电流刺激条件下,分析不同长度微电极的空间电场分布,通过在体动物实验验证了铂铱合金微电极阵列在体工作的有效性.结果表明,经过100μA的单极和双极电流刺激后,铂铱合金电极的最大电场强度均发生在电极材料和绝缘材料的交界处.以电场强度最大点为原点,单极和双极电流刺激的有效半径分别约为21和24μm.     

准噶尔盆地低渗油藏地层测试技术研究

低渗储层的流体渗流具有明显的非达西渗流特性,在试油过程中,即使地层没有受到污染,流体也需要克服一定的阻力之后才能开始流动。因此,对于低渗油气藏的试油,不仅准确求取产能难度大,而且获取稳定的地层压力和储层参数更是十分困难。通过有针对性的测试工艺技术研究,采用合理分配测试时间方案、积极推广分层跨隔测试技术、利用测试技术进行压裂效果评价等,圆满地解决了低渗透储层试油测试中获取资料困难的问题。     

端板型螺栓连接钢节点设计方法

利用有限元软件ANSYS对端板型螺栓连接钢节点进行了弹塑性有限元计算,分析了节点中端板厚度的变化对螺栓内力及变形的影响,讨论了螺栓实际受力与设计方法的关系.进而提出了一些在端板型钢节点设计时值得思考的问题.     

Transiting circumbinary planets Kepler-34 b and Kepler-35 b

Most Sun-like stars in the Galaxy reside in gravitationally bound pairs of stars (binaries). Although long anticipated, the existence of a 'circumbinary planet' orbiting such a pair of normal stars was not definitively established until the discovery of the planet transiting (that is, passing in front of) Kepler-16. Questions remained, however, about the prevalence of circumbinary planets and their range of orbital and physical properties. Here we report two additional transiting circumbinary planets: Kepler-34 (AB)b and Kepler-35 (AB)b, referred to here as Kepler-34 b and Kepler-35 b, respectively. Each is a low-density gas-giant planet on an orbit closely aligned with that of its parent stars. Kepler-34 b orbits two Sun-like stars every 289?days, whereas Kepler-35 b orbits a pair of smaller stars (89% and 81% of the Sun's mass) every 131?days. The planets experience large multi-periodic variations in incident stellar radiation arising from the orbital motion of the stars. The observed rate of circumbinary planets in our sample implies that more than ～1% of close binary stars have giant planets in nearly coplanar orbits, yielding a Galactic population of at least several million.     

Fast core rotation in red-giant stars as revealed by gravity-dominated mixed modes

When the core hydrogen is exhausted during stellar evolution, the central region of a star contracts and the outer envelope expands and cools, giving rise to a red giant. Convection takes place over much of the star's radius. Conservation of angular momentum requires that the cores of these stars rotate faster than their envelopes; indirect evidence supports this. Information about the angular-momentum distribution is inaccessible to direct observations, but it can be extracted from the effect of rotation on oscillation modes that probe the stellar interior. Here we report an increasing rotation rate from the surface of the star to the stellar core in the interiors of red giants, obtained using the rotational frequency splitting of recently detected 'mixed modes'. By comparison with theoretical stellar models, we conclude that the core must rotate at least ten times faster than the surface. This observational result confirms the theoretical prediction of a steep gradient in the rotation profile towards the deep stellar interior.