评估法兰结构螺栓松动的改进损伤指标研究

基于压电阻抗法的采用统计学参数作为损伤指标评估螺栓松动的方法有着广泛的应用，然而采用该方法的试验对象多数为实验室条件下的板等结构，并非真实结构。因此，针对真实的法兰结构，这些损伤指标是否适用、是否需要改进仍需进一步研究。通过实验，得出不同损伤指标与法兰结构螺栓松动之间的规律:螺栓松动的程度越大位置越近，均方根偏差（RMSD）、平均绝对百分比偏差（MAPD）、相关系数差（CCD）的值越大，而指标R_y/R_x因无显著规律不适合作为评估法兰结构螺栓松动的损伤指标。通过对比结果发现:结构差异对前3个损伤指标均有不同程度的影响，改进后的损伤指标均方根变化率（RMSCR）只与法兰结构螺栓松动的位置和程度有关，受结构差异影响小。因此，RMSCR具有重要实践意义:当任一压电片损坏时只需更换为同型号的压电片即可，无需更新损伤指标库。通过实验验证了上述结果的正确性与基于RMSCR的法兰结构螺栓松动检测方法的适用性。      

Temporal variation of the arterial pressure in healthy young people and its relation to geomagnetic activity in Mexico

We present a study of the temporal behavior of the systolic (SBP) and diastolic (DBP) blood pressure for a sample of 51 normotensive, healthy volunteers, 18 men and 33 women with an average age of 19 years old in Mexico City, Mexico, during April and May, 2008. We divided the data by sex along the circadian rhythm. Three geomagnetic storms occurred during the studied time-span. The strongest one, a moderate storm, is attributed to a coronal hole border that reached the Earth. The ANOVA test applied to the strongest storm showed that even though we are dealing with a moderate geomagnetic storm, there are statistically significant responses of the blood pressure. The superposed epoch analysis during a three-day window around the strongest storm shows that on average the largest changes occurred for the SBP. Moreover, the SBP largest increases occurred two days before and one day after this storm, and women are the most sensitive group as they present larger SBP and DBP average changes than men. Finally, given the small size of the sample, we cannot generalize our results.     

Internet2—未来的Internet

介绍了Internet2的发展、基本结构和网络互连等问题，描述了与Internet2紧密相关的gigaPoP的组成，说明了必须考虑的参数和约束条件，阐明了所要采用的路由和服务质量协议。     

超声速机翼－尾翼对突风动态响应的数值方法

本文以Ｇｒｅｅｎ函数为基础的边界元法，结合时间历程法，计算机翼－尾翼组合体对突风动态响应的气动性能。本文介绍的方法，特别适于研究、分析各类飞行器非定常动态响应，为飞行器的设计及其非定常气动特性分析提供了一个行之有效的计算方法。编制的计算程序快捷、精度好。本文提供了单个机翼对突风动态响应的几个算例，有的与Ｌｏｍａｘ解进行了比较，吻合得很好，说明本文所使用的方法是可行的，程序是成功的。对于机翼－尾翼组合体的数值结果，则进一步提供了尾翼受机翼洗流影响的过程。     

固体火箭发动机燃烧不稳定性预估

本文以Culick线性理论为基础,提出预估固体火箭发动机燃烧不稳定性的方法,并给出一个算例.讨论了提高微粒阻尼预估精度和考虑平均流动影响的问题.首次提出用统计方法评定燃烧不稳定性、给出发生燃烧不稳定概率的方法,并讨论了这种统计方法的合理性和可行性.     

固体发动机试车燃气的扩散及对环境的影响

对地处复杂山区的固体火箭发动机试车站的燃气组成及燃气在大气中的扩散和对环境的影响,采用理论预测、数学模式和监测相结合的方法进行了系统研究,配合进行了同步的气象特征研究.评估了不同大气稳定度下污染浓度的分布,提出了有效的防污染措施.     

Geophysical Constraints on the Evolution of Mars

The evolution of Mars is discussed using results from the recent Mars Global Surveyor (MGS) and Mars Pathfinder missions together with results from mantle convection and thermal history models and the chemistry of Martian meteorites. The new MGS topography and gravity data and the data on the rotation of Mars from Mars Pathfinder constrain models of the present interior structure and allow estimates of present crust thickness and thickness variations. The data also allow estimates of lithosphere thickness variation and heat flow assuming that the base of the lithosphere is an isotherm. Although the interpretation is not unambiguous, it can be concluded that Mars has a substantial crust. It may be about 50 km thick on average with thickness variations of another ±50 km. Alternatively, the crust may be substantially thicker with smaller thickness variations. The former estimate of crust thickness can be shown to be in agreement with estimates of volcanic production rates from geologic mapping using data from the camera on MGS and previous missions. According to these estimates most of the crust was produced in the Noachian, roughly the first Gyr of evolution. A substantial part of the lava generated during this time apparently poured onto the surface to produce the Tharsis bulge, the largest tectonic unit in the solar system and the major volcanic center of Mars. Models of crust growth that couple crust growth to mantle convection and thermal evolution are consistent with an early 1 Gyr long phase of vigorous volcanic activity. The simplest explanation for the remnant magnetization of crustal units of mostly the southern hemisphere calls for an active dynamo in the Noachian, again consistent with thermal history calculations that predict the core to become stably stratified after some hundred Myr of convective cooling and dynamo action. The isotope record of the Martian meteorites suggest that the core formed early and rapidly within a few tens of Myr. These data also suggest that the silicate rock component of the planet was partially molten during that time. The isotope data suggest that heterogeneity resulted from core formation and early differentiation and persisted to the recent past. This is often taken as evidence against vigorous mantle convection and early plate tectonics on Mars although the latter assumption can most easily explain the early magnetic field. The physics of mantle convection suggests that there may be a few hundred km thick stagnant, near surface layer in the mantle that would have formed rapidly and may have provided the reservoirs required to explain the isotope data. The relation between the planform of mantle convection and the tectonic features on the surface is difficult to entangle. Models call for long wavelength forms of flow and possibly a few strong plumes in the very early evolution. These plumes may have dissolved with time as the core cooled and may have died off by the end of the Noachian.     

飞机配电系统中交流模拟固态功率控制器设计

主要介绍了一种交流模拟固态功率控制器（SSPC）的设计和实现。它主要使用了在嵌入式系统中广泛应用的单片机，来实现SSPC的基本功能。从核心器件到对负载电流通断控制以及对采入信号的调理都进行了详细的介绍与说明。     

用固体火箭发动机抛放飞机座舱盖的探索

文中对用固体火箭发动机应急打开并抛弃座舱盖方案进行了探索。并根据飞机座舱盖抛放总体方案的要求,确定了固体火箭发动机的设计参数。通过地面试验说明该方案是切实可行的。所设计的固体火箭发动机,其性能满足总体要求。     

The Marginal Rao-Blackwellized Particle Filter for Mixed Linear/Nonlinear State Space Models

In this paper, the marginal Rao-Blackwellized particle filter （MRBPF）, which fuses the Rao-Blackwellized particle filter （RBPF） algorithm and the marginal particle filter （MPF） algorithm, is presented. The state space is divided into linear and non-linear parts, which can be estimated separately by the MPF and the optional Kalman filter. Through simulation in the terrain aided navigation （TAN） domain, it is demonstrated that, compared with the RBPF, the root mean square errors （RMSE） and the error variance of the nonlinear state estimations by the proposed MRBPF are respectively reduced by 29% and 96%, while the unique particle count is increased by 80%. It is also found that the MRBPF has better convergence properties, and analysis has shown that the existing RBPF is nothing more than a special case of the MRBPF.