Low velocity shock-cloud encounters I.

Shocks propagating in the interstellar medium (ISM) play an important role in the life of molecular clouds. Through a theoretical study of interaction between clouds and shocks we can understand, for example, the density distribution of observed molecular clouds and the first steps of star formation. The only way to study of interaction in detail is via a numerical hydrodynamical simulation. In this paper we present the first results of a hydrocode which is able to follow the processes after the collision between the cloud and shock front.Our main theoretical result is that the chemical processes (e.g. H₂ dissociation) can affect the dynamical processes significantly. Global parameters of the cloud are calculated for the comparision of the simulation and the observations.     

Simulation of the full two rigid body problem using polyhedral mutual potential and potential derivatives approach

Herein we investigate the coupled orbital and rotational dynamics of two rigid bodies modelled as polyhedra, under the influence of their mutual gravitational potential. The bodies may possess any arbitrary shape and mass distribution. A method of calculating the mutual potential’s derivatives with respect to relative position and attitude is derived. Relative equations of motion for the two body system are presented and an implementation of the equations of motion with the potential gradients approach is described. Results obtained with this dynamic simulation software package are presented for multiple cases to validate the approach and illustrate its utility. This simulation capability is useful both for addressing questions in dynamical astronomy and for enabling spacecraft missions to binary asteroid systems.     

暗物质粒子探测器触发逻辑测试系统的设计和实现?

作为暗物质粒子探测器(DAMPE, Dark Matter Particle Explorer)的一部分,触发系统主要用于判选所需探测的目标粒子(高能电子和伽玛射线)事例,剔除非目标粒子事例。触发系统由触发探测器和触发判选逻辑电路组成。介绍了触发地检测试系统和宇宙线触发系统的设计和功能实现。触发地检系统实现了对触发判选逻辑电路的电子学验证;另外,配合宇宙线触发系统对部分触发逻辑和触发效率进行了测试。主要介绍了触发系统的测试方法和一些初步测试结果。     

Projections of ocean climate for northwestern Pacific Ocean

The long-term adjustment processes of atmosphere and ocean in response to gradually increased atmospheric CO2 concentration have been analyzed in 70 and 140a integrations with NCAR fully-coupled climate system model (CSM). In these experiments the CO2 concentration has been increased to double and quadruples the initial concentration, respectively. After 70a, at the time of CO2 doubling, the model predicts surface air temperature rises by 1.2 and 1.5K for the globe and the northwestern Pacific Ocean, respectively. The behavior of the quadrupling run is similar: each global and regional mean surface air temperatures increase by 2.8 and 3.0K at the time of CO2 quadrupling. From the experiments, surface air temperature changes in the northwestern Pacific Ocean will be more distinctive compared with the global average, mainly due to exceptionally large warming and sea level change near the entrance of the Kuroshio extension.     

Numerical Simulation of Large Diameter Cylindrical Structure Slamming

The water entry of large diameter cylindrical structure is studied by applying numerical simulation method. The processes of different diameter cyhndrical structures impacting water with various constant velocities are calculated numerically. Thereafter, analyzed are the distribution of slamming pressure on structure during slamming course and the influence of slamming velocity and cylindrical diameter on slamming process. Furthermore, presented herein is an equation being used to forecast the peak slamming force on a large diameter cylindrical structure.     

一种快速的天文图像模拟方法及分析

图像模拟在天文学研究中已经发挥越来越重要的作用,其重要性主要表现在以下几方面:通过模拟可以为准备研制的天文观测设备评估提供重要的依据;通过对模拟数据的处理可以验证数据处理的算法。对图像模拟的整个过程进行描述,并在计算上对图像模拟的局部方法进行优化,使模拟结果能够高效准确的生成。主要工作包含以下几方面:对天体形态的模拟,包括点源(如恒星)和展源(星系),这里主要对展源建模;模拟观测条件,主要是仪器和天光背景等产生的噪声;模拟点扩散函数;从计算和程序的方法对计算流程进行优化;对结果进行分析。采用的数据是哈勃超深空场(HUDF) ACS WFC i(F775)波段的数据,其极限星等达到29等。通过对模拟结果的分析,可以看出该方法能够快速并且较为准确地对星系图像进行模拟。     

北极海冰减少的气候效应研究

本文采用了OSU两层大气环流模式对特定的北极海冰进行数值模拟,研究北极海冰减少的气候效应.试验中海温一律取为气候平均值,北极海冰作为外强迫源影响大气,大气响应完全是环流内部调整的结果.本文对北极海冰减少后的大气环流特征进行了分析,特别是与中国的气温和降水之间的关系.     

青岛浮山湾数值化海区建立的研究--浮山湾波浪模型的建立

在考虑了地形变化,水域开挖,建筑物的掩护,码头和防波堤的反射等对波浪影响的基础上,建立了青岛浮山湾海区波浪模型.计算网格采用矩形网格,为了减少误差,保证计算的精度,计算中均采用正向入射,岸滩按全吸收边界考虑.由模型计算得出各计算点在不同水位和浪向时50年一遇的比波高和波高值.为奥运赛场的建设规划提供了基础依据.     

基于数值模拟的渤海海域地震海啸危险性定量化研究

根据地震海啸产生的条件,结合渤海海域的地形特征、地质构造、地震学特征和历史地震及海啸记录对渤海海域潜在的地震海啸进行了数值模拟研究。分析了渤海可能引发地震海啸的震源区域,讨论了渤海发生海啸灾害的可能性。文中通过数值模拟再现了渤海历史上几次规模较大的地震事件可能引发的海啸情景,研究分析了可能的地震海啸在渤海及周边海域的传播过程及波动特征.地震海啸传播模型采用基于四叉树原理的自适应网格加密技术,有效解决了局部分辨率与计算效率之间的矛盾。数值计算包括地震海啸产生及传播过程。利用该模型对渤海潜在的地震海啸进行了数值计算,基于数值计算结果定量阐述了渤海海域潜在地震海啸对渤海局部岸段及北黄海沿岸的影响,给出了渤海可能地震海啸危险性划分;研究结果将为我国海啸危险性分析和海啸预警技术研究工作提供技术支持。     

GA-BP神经网络在罗源湾口波浪模拟研究中的应用

由于BP神经网络存在收敛速度慢和易于陷入极小值等缺点,引入遗传算法(GA)对网络的权值和阈值加以优化,并采用不同组合的输入因子和样本数,对福建省罗源湾口的波浪进行模拟研究.对输入因子的分析结果表明,研究区域的波浪主要受台湾海峡波浪传播影响,与局地气象因子(风速、风向、海气温差)的相关性较弱.训练样本试验表明,30 d以上的波浪历史数据可使GA-BP神经网络充分学习研究区域的波浪特征,从而实现对波浪要素的高精度模拟.模拟结果显示,对春、夏季实测波浪数据的模拟效果均很好,其中相关性分别为0.967和0.938,均方根误差分别为0.112 m和0.107 m,表明GA-BP神经网络在近岸波浪模拟预报中有较广阔的应用前景.