Information space of sensor networks: Lagrangian,energy-momentum tensor,and applications

It is a challenge to investigate the interrelationship between the geometric structure and performance of sensor networks due to the increasingly complex and diverse architecture of them. This paper presents two new formulations for the information space of sensor networks, including Lagrangian and energy–momentum tensor, which are expected to integrate sensor networks target tracking and performance evaluation from a unified perspective. The proposed method presents two geometric objects to represent the dynamic state and manifold structure of the information space of sensor networks. Based on that, the authors conduct the property analysis and target tracking of sensor networks. To the best of our knowledge, it is the first time to investigate and analyze the information energy–momentum tensor of sensor networks and evaluate the performance of sensor networks in the context of target tracking. Simulations and examples confirm the competitive performance of the proposed method.     

刚性基体高应变复合材料在空间可展结构中的应用及发展

梳理了空间可展结构的分类及发展趋势,从铰接可展结构-带簧铰链、杆状可展结构、面状可展结构及体可展结构四个方面调研了刚性基体高应变复合材料在空间可展结构中的应用现状,从力学和黏弹性特性方面提出了其在可展结构中的应用优势及需要考虑的问题。高模量、低密度、低膨胀系数的刚性基体高应变复合材料是空间可展结构的应用方向,而刚性基体高应变复合材料可展结构的设计方法,以及将其用于大尺寸可展结构的低成本和高精度制造工艺仍有很大的探索空间。     

基于退化失效与突发失效竞争的导弹剩余寿命预测

为了提高导弹剩余寿命预测结果的准确性,本文综合利用导弹的性能退化数据和突发失效时间数据,提出了基于退化失效和突发失效竞争的剩余寿命预测方法。在引入状态空间模型评估出整弹退化程度的基础上,采用Gamma过程建立退化失效模型;在假定突发失效概率与整弹性能退化程度相关的前提下,采用Weibull分布建立突发失效模型;进而建立退化失效与突发失效竞争模式下的导弹可靠度模型。案例应用证明了所提方法的有效性,对准确预测导弹剩余寿命,有效开展视情维修具有一定的工程价值。     

高速再入飞行试验再入条件优化设计

飞行器返回再入时将经历极高的气动热环境,因此深空探测返回飞行器,尤其是载人飞船需要通过实际飞行试验验证相关性能,为降低成本和研制风险,通常采用大再入角和相对第二宇宙速度较低的再入速度进行飞行试验。为获得能实现高热流密度验证的最小能量再入任务方案,采用优化设计手段对飞行试验的再入角和速度以及倾侧角控制进行设计,经仿真分析表明,优化结果可达到飞行试验要求的热流密度,并可将再入速度需求降低约2．1 km／s。     

维修可达性建模及其应用分析

通过对飞机维修中的各个因素进行分析,基于波音737系列飞机建立一个维修可达性模型,并对模型中的各个模块分别开展可视性、实体可达性、操作空间分析,进一步验证了该模型的可行性和实用性,可为我国大飞机设计项目提供技术理论方法。     

GPS 双基线载体姿态测量研究

研究了采用双基线方案测量载体的姿态,利用GPS双差相位测量基线矢量,双差伪距观测值辅助解相位整周模糊,双频时引入空间变换缩小置信空间搜索次数,通过实例分析得出了正确解算相位模糊与观测次数、伪距测量精度的关系,并利用误差传播定律对姿态测量精度进行分析,结合卫星星历数据计算表明,在卫星运行周期内航向角和俯仰角平均测量精度在一定条件下优于2mrad.     

Adiabatic demagnetisation refrigerators for future sub-millimetre space missions

Space worthy refrigeration capable of providing a 100 mK and below heat load sink for bolometric detectors will be required for the next generation of sub-millimetre space missions. Adiabatic demagnetisation refrigeration (ADR), being a gravity independent laboratory method for obtaining such temperatures, is a favourable technique for utilisation in space.We show that by considering a 3 salt pill refrigerator rather than the classic single salt pill design the space prohibitive laboratory ADR properties of high magnetic field (6 Tesla) and a<2 K environment (provided by a bath of liquid⁴He) can be alleviated, while maintaining a sufficient low temperature hold time and short recycle time. The additional salt pills, composed of Gadolinium Gallium Garnet (GGG) provide intermediate cooling stages, enabling operation from a 4 K environment provided by a single 4 K mechanical cooler, thereby providing consumable free operation. Such ADRs could operate with fields as low as 1 Tesla allowing the use of high temperature, mechanically cooled superconducting magnets and so effectively remove the risk of quenching.We discuss the possibility of increasing the hold time from 3 hours, for the model presented, to between 40 and 80 hours, plus reducing the number of salt pills to two, through the use of a more efficient Garnet.We believe the technical advances necessitated by the envisaged ADRs are minimal and conclude that such ADRs offer a long orbital life time, consumable free, high efficiency means of milli-Kelvin cooling, requiring relatively little laboratory development.     

三维体视投影图画法基础

主要介绍三维体视投影图的画法,指出作图的基本规律和图形的表现方法。     

三坐标测量机空间误差的快速检定方法

提出了一种使用Ｒｅｎｉｓｈａｗ检查规检定三坐标测量机或数控机床空间误差的快速方法,此方法一次测量即可完成包含Ｘ、Ｙ、Ｚ三个坐标轴的各项误差影响的空间误差的检定,具有速度快、效率高、准确可靠等特点。     

Coronal Mass Ejections

This workshop summary tries to distill the key difficulties and questions in the art of (I)CME physics and strategies to address them. (I)CMEs are multi-dimensional, multi-parameter, and multi-scale phenomena related to the solar dynamo, corona, and heliosphere. This workshop illustrates the immense progress made in describing and modeling these spectacular energetic solar events, but also shows clear shortcomings in our understanding of them.