Measurement of neutron star parameters: A review of methods for low-mass X-ray binaries

Measurement of at least three independent parameters, for example, mass, radius and spin frequency, of a neutron star is probably the only way to understand the nature of its supranuclear core matter. Such a measurement is extremely difficult because of various systematic uncertainties. The lack of knowledge of several system parameter values gives rise to such systematics. Low mass X-ray binaries, which contain neutron stars, provide a number of methods to constrain the stellar parameters. Joint application of these methods has a great potential to significantly reduce the systematic uncertainties, and hence to measure three independent neutron star parameters accurately. Here, we review the methods based on: (1) thermonuclear X-ray bursts; (2) accretion-powered millisecond-period pulsations; (3) kilohertz quasi-periodic oscillations; (4) broad relativistic iron lines; (5) quiescent emissions; and (6) binary orbital motions.     

高精度板料半模成形新工艺

通过三个精密零件的成形实验，介绐了以粘塑性材料作传力介质的板料半模成形工艺的特点，研究了拉延过程中抗延力、压边力、容框内压的变化规律，工艺参数的控制对拉延所成败及产品质量的影响。     

水杨醛缩－5－碘－8－氨基喹啉新西夫碱试剂的合成及其分析应用研究──分光光度法测定痕量镓

本文介绍了水杨醛缩－５－碘－８－氨基喹啉新西夫碱的合成、提纯与鉴定。特别对其性质及其与镓金属离子显色反应的光度特性作了研究，其配合物３．４９×１０４Ｌ·ｍｏｌ（－１）·ｃｍ（－１）．     

仿真模型检验的新工具

本文是从阐述姿控系统仿真模型检测的重要性以及检测手段需不断改进的观点出发,介绍计算机频率特性测试软件(ftsp)的主要优点和用途。     

Mass flows in coronal loops

Although static loop models are often used to describe the structure of coronal loops, it is evident on both observational and theoretical grounds that mass motions play a crucial role in the physics of the corona and transition region. First we review the observations of emission-line broadening and wavelength shifts, which imply the presence of random motions and systematic downflows in coronal loops. Some discrepancies in the observations are discussed. It is argued that velocities due to gas pressure gradients are the most likely explanation for the observed flows. A number of models that have been proposed for these motions are reviewed. The implications of the various models on observations of the corona and transition region by SOHO are discussed.     

Numerical simulations of spicule driving mechanisms

Spicules are known as one of the most prevalent small-scale dynamic phenomena on the sun, which are likely to give considerable contribution to coronal heating and mass supply. We discuss a model of the spicules driven by a train of slow MHD shock waves propagating along a vertical expanding magnetic flux tube. The shocks are initiated due to compression of the tube by the increasing external pressure in the lower chromosphere. Downflow of spicular material depends on radiative cooling and other dissipative processes.     

基于蒙特卡洛树搜索的机载雷达编队策略优化

多机雷达协同探测是飞机协同作战研究的重要内容,编队策略影响着多机雷达协同探测的探测效能针对机载雷达编队策略的优化,基于部分可观察马尔可夫决策过程(POMDP)模型描述了编队策略优化问题,提出了一种基于蒙特卡洛树搜索(MCTS)的最优策略求解方法。以对敌方目标的探测性能为指标,将该方法与多种其他编队方法的结果进行了比较。试验结果表明,该方法很好地平衡了 MCTS 中利用与探索的关系,可以在规模较大的搜索空间内有效完成编队策略优化,在编队探测能力提升方面展示出了比其它方法更加优越的性能。     

关于军用航空认知战的顶层思考

军用航空认知战已成为现代战争的重要组成部分。随着科技的发展和战争形态的变化,认知战已经从传统战争策略中脱颖而出,成为一种具有重要战略意义的武器。旨在探讨军用航空认知战的概念内涵、基本原理、策略、技术,探讨了应对军用航空认知战的策略和措施,包括加强情报收集和分析、提高欺骗识别能力等。最后,总结了军用航空认知战的重要性和挑战性,并提出了未来研究和发展的建议和前景展望。     

航空复杂产品的 CATIA 结构稳健建模方法研究

针对现有建模方法无法有效对航空产品 CATIA 模型进行快速修改与重用的问题,提出了以曲面分割为建模策略的结构稳健性建模方法。该方法通过对父子关系关联传播路径进行分析,找出影响 CATIA 特征模型结果稳健性的因素,即几何元素方向、几何拓扑元素、建模策略。通过研究特征构建时,输人元素的性质和基于此性质的操作方法,实现结构稳健性建模,即通过对外部输人和建模过程中的关键几何元素进行方向控制、创建显式参考代替几何拓扑元素、禁止使用复杂草图、采用基于曲面分割的设计特征模块化建模策略等方式,实现特征模型的快速修改与重用。工程实例证明了所提方法的实用性和可靠性。