陶瓷纤维梯度增强活塞的梯度方程研究

 功能梯度材料零件具有单质材料零件无法比拟的理化性能优势,然而由于材料分布复杂以及对功能梯度材料本身性能研究不充分,使性能分析存在很多困难。论文应用复合材料热性能理论,采用有限元分析软件ADINA,分析陶瓷纤维梯度增强活塞（材料梯度方程的参数不同）的温度分布和应力分布,结果表明陶瓷纤维梯度层可以明显改变活塞温度分布,缓和由于热膨胀系数不匹配,在陶瓷纤维增强层与活塞本体交界处产生的应力。根据计算结果拟合出温度峰值、整体应力峰值和层间应力峰值与方程系数之间的曲线,并加以验证。     

模型烧蚀对尾迹电子特性影响的计算和实验研究

 基于气动物理研究的需要,针对高焓风洞的来流特点,采用计算和实验相结合的方法研究聚丙烯烧蚀对尾迹电子密度的影响。结果表明：计算结果可以有效模拟实验状态,电子密度的模拟精度有很大提高,误差在一个量级内;聚丙烯烧蚀可以降低尾迹的电子密度,但幅度不大,在2倍左右,其与选择模型材料的催化特性降低幅度相当;对电弧风洞的成功改进和非稀薄流静电探针诊断技术的应用,是尾迹电子密度测试的前提保障。     

铆钉连接件细节应力分析及疲劳裂纹形成寿命预估

 首先建立简化的力学模型模拟复杂的铆钉连接件结构,并用有限元软件对所建立的模型进行细节应力分析。然后利用损伤力学守恒积分原理得到计及损伤耦合效应的集中应力表达式。在此基础上,根据由热力学原理导出的以损伤驱动力表示的损伤演化方程,给出裂纹形成寿命与载荷关系的解析表达式。进一步,按照某种材料的部分标准试件的中值疲劳曲线拟合损伤演化方程中的材质参量,并利用同类材料的其他标准试件的中值疲劳曲线进行寿命预估方法验证。最后,给出了国产某型客机危险部位具有不同存活率的疲劳裂纹形成寿命。     

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。     

基于多目标优化的星空认知网络鲁棒波束成形算法

卫星通信(SC)网和无人机(UAV)通信网之间频谱共享、相互融合,能较大提升频谱效率,有望成为第6代移动通信的关键技术之一。与现有文献不同,本文在系统非完美信道状态信息(CSI)的条件下,考虑了次级用户可达速率最大化和发射功率最小化2种准则,利用加权切比雪夫方法构建满足概率约束的多目标优化问题(MOO);由于该问题较为非凸,利用概率公式、半正定松弛等方法将其转化为凸问题,并进一步通过半正定规划(SDP)求解,得到鲁棒波束成形权矢量,获得2种性能指标间的帕累托最优权衡。计算机仿真验证了所提鲁棒波束成形算法的有效性和优越性。     

秦皇岛古代旅游诗歌整理及其对旅游的作用

秦皇岛作为历史悠久的旅游城市,拥有着大量的古代旅游诗歌,这些旅游诗歌对于传播秦皇岛的历史文化,推动旅游事业的发展起到了很大的作用。本文拟就秦皇岛古代的旅游诗歌整理分析及其在旅游中的作用三个方面展开论述。     

基于自适应Kriging代理模型的交叉熵重要抽样法

对于复杂失效域和小失效概率耦合的可靠性分析问题,本文提出了一种交叉熵重要抽样（CE-IS）方法结合自适应Kriging （AK）代理模型的求解方法（CE-IS-AK）。所提方法基于交叉熵原理,用混合高斯模型逐步逼近最优重要抽样密度函数,并采用AK模型协助逼近过程中混合高斯模型的参数的更新,从而提高了CE-IS方法的计算效率。另外,本文还改进了CE-IS方法的收敛准则,避免了方法的冗余迭代,扩大了方法的适用范围。由于在CE-IS方法中引入了AK模型,因此,本文方法所构建的重要抽样函数在保证精度的基础上提高了效率。相较于AK-MCS方法,本文方法中引入了重要抽样的思想,因此在Kriging训练点数目基本相同的情况下,大幅缩减小失效概率计算时样本池规模,并且由于利用了混合高斯模型,因而对多失效域具有较好的适用性。算例分析也证明了本文所提方法的优越性。     

Study of maximum electron density NmF2 at Karachi and Islamabad during solar minimum (1996) and solar maximum (2000) and its comparison with IRI

The monthly hourly medians of maximum electron density, N_mF₂, at two Pakistani ionospheric stations, Karachi and Islamabad, have been determined for solar minimum (1996) and solar maximum (2000) and compared with IRI predictions using the URSI coefficients. At night and pre-noon period the N_mF₂ values at both stations are almost equal during the 2 years. However, at post-noon the values at Karachi are considerably larger than those at Islamabad due to the equatorial or geomagnetic anomaly. Karachi (geomag. coord. 16.44°N, 139.08°E) lies near the region of the equatorial anomaly (+20 and −20 geomagnetic latitude), so most of the N_mF₂ values at Karachi are larger than those at Islamabad (geomag. coord. 24.46°N, 145.67°E). The maximum monthly values of N_mF₂ show a semi-annual variation at Karachi and Islamabad both during 1996 and 2000 as predicted by IRI.     

微纳InSAR卫星总体技术研究

微纳合成孔径雷达干涉(Synthetic Aperture Radar Interferometry, InSAR)卫星是对地定量化遥感的重要手段。开展了微纳InSAR卫星系统总体技术研究,给出了使得干涉测量覆盖范围最大的双星编队构型设计方法,建立了低燃料消耗双星轨道参数设计准则,提出高功能密度比InSAR卫星系统的设计方法,包括载荷平台一体化、卫星高集成模块化等总体设计方法,并给出了相应的设计实例。     

A global survey of COSMIC ionospheric peak electron density and its height: A comparison with ground-based ionosonde measurements

With a network of ground-based ionosondes distributed around the world, the ionospheric peak electron density and its height measured by FORMOSAT-3/COSMIC satellites in terms of GPS radio occultation technique are extensively examined in this article. It is found that, in spite of the latitude, the mean values of the peak electron density measured by COSMIC satellites are systematically smaller than those observed by ground-based ionosondes. The discrepancy between them is dependent on the latitude, namely, it is small in low and mid-latitudes and large in high-latitude region. Moreover, statistical analysis shows that the slopes of the regression line that is best fitted to the scatter diagram of occultation-retrieved peak electron density (ordinate axis) versus ionosonde-observed peak density (abscissa axis) are universally less than one. This feature is believed to be the result of path average effect of non-uniform distribution of the electron density along the GSP ray during the occultation. A comparison between COSMIC-measured peak height and ionosonde-derived peak height hmF2 indicates that the former is systematically higher than the latter. The difference in the two can be as large as 20% or more in equatorial and low-latitude regions. This result implies that the peak height hmF2 derived from the virtual height through true height analysis based on Titheridge method seems to underestimate the true peak height. The correlation between COSMIC and ionosonde peak electron densities is analyzed and the result reveals that correlation coefficient seems to be dependent on the fluctuation of the occultation-retrieved electron density profile. The correlation will be higher (lower) for the electron density profiles with smaller (larger) fluctuations. This feature suggests that the inhomogeneous distribution of the electron density along the GPS ray path during the occultation plays an important role affecting the correlation between COSMIC and ionosonde measurements.