基于相关系数AR模型的陀螺随机漂移分析方法

陀螺漂移序列的均值和方差随时间不断变化,不属于传统的相关函数平稳序列,因此采用传统的平稳序列分析方法对其处理必然导致较大的误差．通过对大量陀螺漂移数据分析发现,大多数陀螺漂移序列的相关系数并不随时问的平移而变化,是时间间隔的单变量函数,因此,它们属于相关系数平稳序列．在此基础上,建立了基于相关系数AR模型的陀螺漂移分析方法．该方法首先对陀螺漂移数据是否属于相关系数平稳序列进行判别,然后采用相关系数AR模型建模并给出模型参数的估计方法,最后可根据得到的相关系数AR模型对陀螺漂移进行估计和补偿．由于相关系数平稳序列能够对陀螺漂移序列的本质特征进行描述,因此较传统方法具有更高的建模精度和补偿精度．     

准晶材料的摩擦磨损性能研究

本文对准晶材料与类金刚石涂层在干摩擦条件下的摩擦磨损性能进行了研究，分别就磨损载荷、摩擦速度、气氛、温度等因素对准晶材料摩擦磨损特性的影响进行了讨论，采用扫描电镜和Ｘ－射线衍射仪等对表面形貌进行了观察，结果表明，随着磨损载荷、摩擦速度的增加，摩擦系数有所减小，温度对准晶材料表面的摩擦系数影响明显比其他因素大，温度的增加明显提高地表面摩擦系数。准晶材料在３５０℃下的磨擦磨损机制为剥落磨损，明显不同与室温下的磨损机制，形貌观察表明准晶材料摩擦表面均形成不了同程度的微裂纹，本文对上述结果进行了讨论。     

回归模型在房地产市场方面的应用

本文通过建立的回归模型，对商品住宅的销售量进行了预测。     

上海电视塔风载试验研究

通过风洞试验研究了上海电视塔的风载分布情况，给出了塔体压力分布、体型系数、局部压力增大系数等风载设计数据，并考查了周围地貌及风向的影响。     

动力系统试验吹除系统调试问题分析

新一代运载火箭动力系统试验台首次承担某型号动力系统试验任务,在发动机燃料头腔（燃气腔）吹除调试过程中发现吹除压力偏低,难以满足试验要求.介绍了吹除系统组成及利用孔板模拟发动机吹除路背压的调试方案,分析了引起吹除路压力偏低可能原因是孔板模拟的额定吹除流量或供气管路的阻力系数偏大.因此,通过模拟孔板流量系数标定和管路流阻特性计算,最终确定供气管路阻力系数偏大是引起吹除压力值偏低的主要影响因素,并通过制定加大供气管路内径、减少系统阀门数量等针对性改进措施,优化了地面配气工艺系统.经试验验证：吹除压力偏低的原因分析是正确性的,采取改进措施后供气管路的流阻损失降低了47％.同时确定了试前气源的容积及充气压力,保证了试验的顺利进行.     

考虑来流边界条件不确定性的数值模拟方法

针对气动热力学边界条件不确定性的数值模拟方法,进行了考虑来流边界条件不确定性对流体流动影响研究。算例中提取来流边界条件为设计变量,采用拉丁超立方抽样方法对设计变量进行采样,运用CFD软件对所有样本进行数值模拟计算后得到响应变量,最后分析得到来流边界条件对流体的影响规律。结果表明:来流边界条件中湍流度的不确定性对压力系数的影响大于来流速度的不确定性对压力系数的影响。     

NASTRAN在压力系数分布形态分析中的应用

针对机翼压力系数分布形态分析工作存在辨识困难的问题，通过对压力系数数据格式的变换处理，利用MSC．NASTRAN for Windows2．0的图形显示功能，将压力系数分布的分析辨识工作由分析数据文件变为查看在电脑屏幕上可视化的分布图形，极大地提高了压力系数分布分析工作的效率。     

基于定常N-S方程的导弹滚转数值模拟研究

基于商业CFD软件FLUENT定常N-S方程,在不同计算资源下数值模拟了某标准导弹在不同飞行马赫数、滚转速度和迎角时的滚转特性,并与AEDC报告实验结果进行了对比。计算结果验证了定常算法数值模拟滚转阻尼系数的可行性及其在不同计算资源下计算精度的可优化性,而且定常算法与非定常计算相比消耗更少的计算资源。     

Transponder calibration of the Envisat RA-2 altimeter Ku band sigma naught

Although the history of spaceborne altimeters goes back to the early seventies, the absolute calibration of the backscattering coefficient has never been deeply investigated. This information has been primarily used to infer the wind speed via an empirical model, and the intercalibration among different satellite altimeters has revealed to be suitable for this purpose, being the wind retrieval based on an empirical relationship. As far as Ku band system is concerned, the sigma naught absolute calibration of the Envisat altimeter (RA-2) has been performed using an active reference target provided by a transponder. This has been exploited during the 6-month Commissioning phase to generate early calibration results. In order to monitor the RA-2 backscatter calibration during the Envisat lifetime, a continuous calibration effort has been carried out by operating the transponder as much as possible. This paper aims to review the entire effort for calibrating the RA-2 sigma naught measurements, which lasted for almost seven years. It presents in detail the adopted methodology and the final outcome of the activity, providing the users with the correction (bias) to get the calibrated sigma naught and analyzing its stability during almost the entire Envisat lifetime. Specifically, it is concluded that the RA-2 backscatter measurements were quite stable, even if a bias of about 1 dB should be considered with respect to the actually released product. Some small changes in the bias as function of time can be identified during most of the Envisat lifetime, consisting in a slight increase in the first two years, followed by a more stable period and a final drop observed at the end of 2009, until the conclusion of the calibration activity (corresponding to the change in Envisat orbit).     

Navigating BepiColombo during the weak-stability capture at Mercury

BepiColombo is scheduled for launch in August 2013 and to arrive after a nearly six-year long transfer at Mercury in June 2019. The trajectory has a number of challenging elements: a launch with Soyuz/Fregat into a geostationary transfer orbit, followed by a lunar flyby, long low-thrust arcs and five more planetary flybys (one at the Earth, two at Venus and two at Mercury). At arrival the low thrust arcs reduce the approach velocity so much that BepiColombo passes by the Sun–Mercury Lagrange points L₁ and L₂ and gets weakly captured in a highly eccentric orbit around Mercury in case the orbit insertion manoeuvre would fail.This paper describes the navigation strategy during the final phase. Five trajectory correction manouevres during the last 65 days requiring up to 20 m/s (3σ) are proposed. With this strategy it is possible to navigate BepiColombo safely through the weak-stability boundary of Mercury and to reach the target periherm with a precision of 11 km.