砂土硬化特征的描述及其试验验证

采用不同路径下砂土的三轴拉伸和三轴压缩试验结果,分别选用塑性体积应变、塑性剪应变、清华模型硬化参数、塑性功和统一硬化参数H作为硬化参数,在以上硬化参数和应力比空间里探讨了砂土的硬化规律和应力路径相关性.基于修正剑桥模型的屈服函数,采用塑性体积应变、塑性功和H作为硬化参数,推导了分别对应的本构模型.通过饱和塔克拉玛干沙漠砂的三轴试验结果,表明了H在描述砂土应力应变特性上的适用性.      

Analysis of solar spike events by means of symbolic dynamics methods

We have searched for interrelations of spikes emitted simultaneously at different frequencies during the impulsive phase of flare events (Fig.1). As the spikes are related to the flare energy release and are interpreted as emissions that originate at different sites having different magnetic field strengths, any relation in frequency is interpretated as a relation in space. Quantities of symbolic dynamics, such as mutual information, Shannon information and algorithmic complexity are appropriate to characterize such spatiotemporal patterns, whereas the popular estimate of fractal dimensions can be applied to low-dimensional systems only.The goal is to decide between two possible types of fragmentation depending on the energy release and emission processes, which we callglobal andlocal organization. In the global organization the whole region becomes supercritical, and the energy is released in independent, small regions. The alternative local scenario requires a trigger that spreads from initial localized events and ignites nearby regions.Mutual information which is a generalization of correlation indicates a relation in frequency beyond the bandwidth of individual spikes. The scans in the spectrograms with large mutual information also show a low level of Shannon information and algorithmic complexity, indicating that the simultaneous appearance of spikes at other frequencies is not a completely stochastic phenomenon (white noise). It may be caused by a nonlinear deterministic system or by a Markov process. By means of mutual information we find a memory over frequency intervals up to 60 MHz (Fig. 2). Shannon information and algorithmic complexity, however, describe spike events as a whole, i.e. a global source region. A global organization is also apparent in quasi-periodic changes of the Shannon information and algorithmic complexity in the range of 2–8 seconds (Fig. 3).This findings is compatible with a scenario of local organization in which the information of one spike event spreads spatially and hence triggers further spike events at different places. The region is not an ensemble of independently flashing sources, each representing a system that cascades in energy after an initial trigger. On the contrary, there is a causal connection between the sources at any time.The analysis of four spike events suggests that the simultaneous appearance of spikes is not stochastically independent but a process in which spikes at nearby locations are simultaneously triggered by a common exciter.We have shown in the case in the case of spikes that quantities from nonlinear dynamics used in this paper are helpful in detecting structural properties of complex spatio-temporal patterns. This approach seems to be promising also for several other astrophysical applications.     

关于球形导体外部倾斜赫芝振子辐射场的探讨

本文给出球形导体倾斜赫芝振子辐射场的线极化与圆极化分量表达式,并进行计算,示出典型剖面内的各分量方向图。由此可进一步分析球形导体上线状天线的辐射特性。     

钣料压延数值解

本文采用能量条件的硬化模式,考虑到钣料的厚向异性,导出了压延凸缘区和凹模圆角区数值解所需的理论方程以及压延拉伸失稳条件的数学表达式和压延拉伸失稳临界载荷计算公式,在此基础上,利用电子计算机求解了四种钣料(TA1—M、LY12—M、LF2—M、20钢)的压延载荷和极限压延系数。理论和实验结果取得了很好的一致性。     

不同锯齿对圆转矩形喷管红外辐射特征影响数值模拟

在考虑中心锥、波瓣混合器、火焰稳定器以及加力燃烧室筒体影响的条件下,将轴对称收扩喷管改型设计为圆转矩形基准喷管,进一步在喷管出口进行修型设计.并对不同锯齿喷管流动、换热与红外辐射特征进行了数值分析.得到如下结论:考虑高温部件后,喷管红外辐射强度的方向性特征更加明显;相比圆转矩形基准喷管,采用多个小尺寸锯齿时,射流高温区长度有一定缩短,采用单个大尺寸锯齿时,高温区长度进一步缩短,其正后方红外辐射强度降低;将轴对称收扩喷管改为圆转矩形喷管并加装锯齿后,强化尾喷流与外流掺混,降低其红外辐射强度的同时带来了一定的推力损失.     

H-450 X射线参考辐射质的研建及验证

根据PTB和ISO 4037-1:2019要求,关于高空气比释动能系列（H系列）X射线参考辐射质的推荐数据,外推得出H-450的附加过滤为6.24 mm Cu,第一半值层（HVL_1st）为(5.39~5.52)mm Cu,平均光子能量为(214.25~214.78)keV,剂量率为11.51 Gy/h（距离焦斑为1 m处,管电流为10 mA）。随后,使用PTW32005电离室作为测量器具,采用半值层法建立H-450 X射线参考辐射质,得出HVL_1st为5.37 mm Cu,第二半值层（HVL_2nd）为5.97 mm Cu,同质系数为0.9。最后,使用PTW30013次级标准电离室测量得出H-450 X射线参考辐射质下距离焦斑1 m,管电流为10 mA时的剂量率值为11.98 Gy/h,与理论值的相对误差为4.07 %。采用MCNP 5软件对H-450 X射线参考辐射质进行能谱模拟并计算得出其平均光子能量为200.4 keV。     

屏蔽材料对木星轨道卫星内部介质充电效应的影响研究

在木星轨道的空间辐射环境中,占主导地位的粒子是能量大于1 MeV(甚至高于100 MeV)的高能电子,这可能会产生卫星内部介质充电效应.在卫星的防辐射设计中,通常需要一定厚度的材料来屏蔽这些电子,使得进入卫星内部的电子通量达到安全的水平.利用所建立的GEANT4-RIC(radiation induced conduc...     

模化比对直升机用红外抑制器红外辐射特性的影响

对波瓣喷管一弯曲混合管构成的直升机用红外抑制器壁面和尾焰的红外辐射特性进行了一系列的数值研究,旨在将三维流场数值计算、壁温计算与红外辐射计算结合起来综合分析抑制器红外辐射特性,与相关实验数据的对比验证表明计算结果与实验结果仅相差15%左右,且红外辐射强度空问分布规律一致;通过对不同缩比模型的数值计算,揭示了模化比对壁面及尾焰的红外辐射特性的影响规律:(1)几何相似的红外抑制器在主流入口速度、温度相同时,壁面红外辐射强度与几何模化比的2次方成正比;(2)尾焰红外辐射强度与几何模化比的2.32次方成正比.      

航天员空间活动接受辐射剂量限值的研究

空间生物学辐射效应是由空间辐射环境引起的,空间辐射环境的变化受太阳活动性影响。空间辐射水平比地表面水平高,航天员在空间所接受剂量比地面人员接受的吸收剂量高出100倍甚至更高,并且高能重离子的生物效应显著。文章简要阐述了空间辐射环境、空间辐射生物学效应与航天员的辐射剂量限值等问题。