面向系统集成的起落架地面运动特性建模方法

大型飞机地面运动特性是飞机性能的重要组成部分,主要涉及到飞机的地面滑跑、转弯以及刹车等过程。地面运动特性的分析涉及到动力学、液压、控制等多领域,是典型的多学科耦合的复杂问题。以某大型民用飞机为研究对象,从主制造商的系统集成性能分析需求出发,通过多学科解耦和模型物理度划分两个角度进行地面特性模型架构的分解与定义,并以飞机刹车系统性能分析为例,验证了本架构的有效性。本文提出的模型架构灵活,既适用于飞机集成商的飞机级性能分析,又适用于特定系统级的性能分析。     

LY12CZ铝合金材料的室温和高温单轴循环变形行为及其时间相关性

 对LY12CZ铝合金室温和高温下的单轴循环变形行为及其时间相关特性进行了实验研究,重点讨论了环境温度、应力水平、加载波形和峰值保持对材料棘轮行为的影响。结果表明：室温和高温下,LY12CZ铝合金体现出循环硬化特性,并具有明显的应变幅值依赖性;材料的棘轮行为不仅依赖于当前的平均应力和应力幅值大小,还与加载历史密切相关。尽管LY12CZ铝合金在单调拉伸时对应变率的变化不敏感,但其循环棘轮行为具有明显的时间相关特性：有峰值保持时产生的棘轮应变明显大于没有保持时的值,并随保持时间的增加而增大;正弦波形下的棘轮应变大于三角波形下的棘轮应变。     

Mesh-dependence of Material with Softening Behavior

The issue of mesh-dependence emerges when the conventional continuum damage model is applied to handling the softening behavior. In order to circumvent the mesh-dependence, the non-local theory is introduced into the conventional damage model and the finite element formulas are derived for two-dimensional gradient-enhanced damage model. A new element is proposed in which the basic unknown quantities are displacement, non-local equivalent strain and the gradient of non-local equivalent strain. The element and constitutive equation proposed in this article are added to the finite element software ABAQUS through user subroutine UEL. Numerical results show that the gradient-enhanced damage model can eliminate the mesh-dependence and is effective for dealing with the issue of softening behavior.     

中国核电厂操作员反应时认知模型的应用(英文)

讨论了一些有关人员行为与时间有依赖关系的可靠性模型;给出了中国核电厂操作员在清华大学培训模型机上的一些可靠性实验结果。此外,还根据已获得的实验数据计算了在ＡＴＷＳ事故条件下人的失误概率。     

Oxygen line mapping of SN 1006 with Suzaku

SN 1006 is one of the supernova remnants (SNRs) with relatively low-temperature electrons, considering the young age of just 1000 years. We carried out SN 1006 mapping observations with the X-ray Imaging Spectrometers (XIS) and the Hard X-ray Detector (HXD) onboard Suzaku, the fifth Japanese X-ray satellite. Thanks to the excellent spectral resolution of XIS in the soft X-ray band, H-like and He-like oxygen emission lines were clearly detected, and we could make a map of the line intensity, and as well as a flux and the photon index of nonthermal component. We found that these parameters have spatial dependences from region to region in the SNR; the north region is bright in nonthermal, while dim in thermal; the east region is bright in both nonthermal and thermal; the inner region shows dim nonthermal and bright thermal emission. The photon index is the smallest in the north region.     

New evidence for strong non-thermal effects in Tycho’s supernova remnant

For the case of Tycho’s supernova remnant (SNR), we present the relation between the blast wave and contact discontinuity radii calculated within the nonlinear kinetic theory of cosmic ray (CR) acceleration in SNRs. It is demonstrated that these radii are confirmed by recently published Chandra measurements which show that the observed contact discontinuity radius is very close to the shock radius. Therefore a consistent explanation of these observations can be given in terms of efficient CR acceleration which makes the medium more compressible.     

Evolution of the periodicities in 2S 0114+650

We have analysed 9 years of data from the All Sky Monitor on the Rossi X-ray Timing Explorer for 2S 0114+650 to study the evolution of its spin, binary, and super-orbital periods. The spin history of the neutron star in this system exhibits torque reversals lasting 1 year. The newly discovered super-orbital period has remained stable over the 9-year span, making 2S 0114+650 the fourth known system to exhibit stable super-orbital modulation. We compare its super-orbital period evolution with those of the other three such systems.     

基于群论的空间可展开结构自由度分析

为了开发构型新颖、生命力强、便于运输和储藏的空间可展开结构,使其满足所处环境的时间、空间等苛刻条件,适应特殊任务的实际需求,亟需开展空间可展开结构的自由度及折展性能分析。由于现有可展结构多具有一定的对称性,基于群论方法,从对称学角度解析结构可动的本质,提出判别对称体系可动性的充分条件。根据几何约束性质,运用矩阵理论和变分原理,推导了可展结构中典型构成单元的位移协调矩阵。利用对称子空间,推导了机构位移模态、自应力模态的对称表示,并以闭合环形可展开结构为研究对象,开展了结构自由度分析。研究工作有助于新型空间可展开结构的研发与设计,为可展结构及其衍生结构的进一步研究与应用提供了理论基础。     

挂滴燃烧中的微汽泡行为和液滴跳动

利用高速显微摄像技术,观察研究了RP-3微尺度挂滴燃烧过程中,微汽泡的核化、生长、聚并和溢出的行为过程及液滴跳动现象.结果得出:①液滴中微汽泡产生的位置;②在蒸发初期时由微汽泡引起液滴体积的膨胀;③在燃烧中由汽泡行为导致液滴的跳动;④液滴燃烧的稳定(不爆裂)现象.分析了表面张力在挂滴燃烧过程中的作用,确定了挂滴稳定燃烧的临界条件下的临界特征体积在2.5~5.0μL.      

RATAN-600 and RadioAstron reveal the neutrino-associated blazar TXS 0506+056 as a typical variable AGN

The possible association with the high-energy neutrino event IceCube-170922A has sparked interest in the blazar TXS 0506+056. We present 72 instantaneous 1–22 GHz spectra measured over the past 20 years with the RATAN-600 telescope and compare them with the results of observations of 700 variable Active Galactic Nuclei (AGN) studied within the same program. The recent radio flare of TXS 0506+056 started from a minimum in 2013 and reached its first peak in December 2017 and a second peak in May-June 2018. This was the third strong radio flare in this source since 1997. The spectrum remains nearly flat during the flares. The spectral shape and variability pattern observed in TXS 0506+056 are typical for variable AGN. RadioAstron Space VLBI observations in 2013–2015 did not detect TXS 0506+056 on space-ground baselines of more than 9 Earth diameters. However, an observation on 23 September 2015 resulted in the detection of interferometric signal on 6 Earth diameter baselines at 18 cm close to the detection limit. We consider the possibility that TXS 0506+056 and other AGN may accelerate relativistic protons more efficiently than electrons. Relativistic protons are necessary to produce both the high-energy neutrinos observed in the IceCube Observatory and the high AGN brightness temperatures implied by the RadioAstron detection. They may also provide the main contribution to the observed synchrotron radiation of parsec-scale AGN jets. This supports the suggestion that relativistic protons may play a much more important part in extragalactic astrophysics than earlier anticipated.