Galactic outflows and the pollution of the galactic environment by supernovae

We here explore the effects of the SN explosions into the halo of star-forming galaxies like the Milky Way. Successive randomly distributed and clustered SNe explosions cause the formation of hot superbubbles that drive either fountains or galactic winds above the galactic disk, depending on the amount and concentration of energy that is injected by the SNe. In a galactic fountain, the ejected gas is re-captured by the gravitational potential and falls back onto the disk. From 3D non-equilibrium radiative cooling hydrodynamical simulations of these fountains, we find that they may reach altitudes up to about 5 kpc in the halo and thus allow for the formation of the so called intermediate-velocity-clouds (IVCs) which are often observed in the halos of disk galaxies. The high-velocity-clouds that are also observed but at higher altitudes (of up to 12 kpc) require another mechanism to explain their production. We argue that they could be formed either by the capture of gas from the intergalactic medium and/or by the action of magnetic fields that are carried to the halo with the gas in the fountains. Due to angular momentum losses to the halo, we find that the fountain material falls back to smaller radii and is not largely spread over the galactic disk. Instead, the SNe ejecta fall nearby the region where the fountain was produced, a result which is consistent with recent chemical models of the galaxy. The fall back material leads to the formation of new generations of molecular clouds and to supersonic turbulence feedback in the disk.     

A material experiment for small satellites to characterise the behaviour of carbon nanotubes in space – development and ground validation

Over the last years, Carbon Nanotubes (CNT) drew interdisciplinary attention. Regarding space technologies a variety of potential applications were proposed and investigated. However, no complex data on the behaviour and degradation process of carbon nanotubes under space environment exist. Therefore, it is necessary to investigate the performance of these new materials in space environment and to revaluate the application potential of CNTs in space technologies.Hence, CiREX (Carbon Nanotubes – Resistance Experiment) was developed as a part of a student project. It is a small and compact experiment, which is designed for CubeSat class space satellites. These are a class of nanosatellites with a standardized size and shape. The CiREX design, electrical measurements and the satellites interfaces will be discussed in detail. CiREX is the first in-situ space material experiment for CNTs.To evaluate the data obtained from CiREX, ground validation tests are mandatory. As part of an extensive test series the behaviour of CNTs under solar ultra violet light (UV) and vacuum ultraviolet light (VUV) was examined. Single-walled carbon nanotubes (SWNT), multi-walled carbon nanotubes (MWNT) and MWNT/resin composite (ME) were exposed to different light sources. After the exposure, the defect density was investigated with Raman spectroscopy. There is a clear indication that UV and VUV light can increase the defect density of untreated CNTs and influence the electrical behaviour.     

基于P2P的一种负载饱和避免技术研究

在点对点体系结构的分布式虚拟环境系统中,由于客户机节点的计算能力和带宽的异构性,以及发生在客户机程序之间交互信息量的不同,会导致一些客户机出现负载饱和。一台客户机的负载饱和不仅影响本机程序的运行,也会对周围其他的客户机的运行产生影响,这限制了分布式虚拟环境系统的性能。研究提出了一种在点对点体系结构的分布式虚拟环境系统中避免客户机负载饱和的技术,试验结果显示了所提出的方法有效地改进了系统的性能。     

Stagnation temperature effect on the conical shock with application for air

The aim of this work is to realize a new numerical program based on the development of a mathematical model allowing determining the parameters of the supersonic flow through a conical shock under hypothesis at high temperature, in the context of correcting the perfect gas model. In this case, the specific heat at constant pressure does not remain constant and varies with the increase of temperature. The stagnation temperature becomes an important parameter in the calculation. The mathematical model is presented by the numerical resolution of a system of first-order nonlinear differential equations with three coupled unknowns for initial conditions. The numerical resolution is made by adapting the higher order Runge Kutta method. The parameters through the conical shock can be determined by considering a new model of an oblique shock at high temperature. All isentropic parameters of after the shock flow depend on the deviation of the flow from the transverse direction. The comparison of the results is done with the perfect gas model for low stagnation temperatures, upstream Mach number and cone deviation angle. A calculation of the error is made between our high temperature model and the perfect gas model. The application is made for air.     

海洋环境与疲劳载荷联合作用下喷丸超高强度钢损伤机制

舰载机起落架结构既要遭受海洋大气、海上盐雾和海浪飞溅等严酷海洋环境的侵蚀作用,又要承受较大的弹射起飞/拦阻着舰载荷,在海洋环境与疲劳载荷联合作用下超高强度钢起落架结构承载能力显著劣化,对使用安全构成严重挑战。针对超高强度钢喷丸和未喷丸两种试验件,基于舰载机服役的海洋环境,开展了腐蚀+疲劳交替试验和预腐蚀疲劳试验研究,得到了疲劳寿命变化规律,通过粗糙度、晶粒度、显微硬度、残余应力和疲劳断口分析,揭示了喷丸对疲劳寿命增强的作用机制、腐蚀+疲劳损伤交替作用机制和预腐蚀疲劳损伤作用机制。结果表明,喷丸强化后疲劳寿命平均增幅为93.1%;对于喷丸试验件,深度约为20 μm的轻微点蚀,导致疲劳寿命衰减幅度达到30%;喷丸强化与腐蚀两者之间存在着此消彼长的竞争机制;腐蚀+疲劳交替作用损伤机制对该型超高强度钢造成的疲劳寿命衰减要比预腐蚀疲劳损伤机制严重得多,加速腐蚀试验时间相同的条件下前者疲劳寿命为后者的47%~54%。     

复杂电磁环境表征方法

复杂电磁环境表征是电子信息系统复杂电磁环境效应研究的基础性问题之一.基于电磁环境的复杂性特点,提出了一种复杂电磁环境表征方法,该方法从实体环境、电磁信号环境和基于特定电子信息装备的电磁信号环境等三个方面进行参数化描述,为复杂电磁环境认知和模拟奠定基础.     

Development of Space Environment Research in China

Abstract This paper presents the recent research progress on space environment in China. The space environment here includes space environment models, forecast methodology and space environment effects on spacecrafts. Finally the development trends of China's space environment research are discussed.     

导弹轨控喷流气动干扰全空域插值方法研究

导弹侧向喷流气动干扰受海拔高度影响显著,主要原因在于雷诺数和压力比会随海拔高度的变化而变化。受大气参数的影响,雷诺数和压力比的变化规律并不一致。为能在现有气动模型基础上既保证插值精度又减少节点数,通过数值模拟方法研究了雷诺数和压力比对轨控喷流气动干扰的影响。结果表明:海拔高度对喷流气动干扰的影响主要由压力比变化造成,雷诺数变化产生的影响相对较小,且喷流干扰与压力比间存在一定的线性关系。因此,提出了一种基于压力比的喷流气动干扰插值方法。相比于传统的基于高度的插值方法,该方法可显著提高插值精度,并减少节点数,适用于全空域轨控喷流气动建模。     

对地靶射击时飞行安全问题研究

针对目前估算式计算出的退出地靶射击时损失高度比实际小的问题，提出了退出地靶射击损失高度可分三阶段的估算方法，具体计算分析了延迟时间、飞行速度、俯仰角、过载等变化对退出地靶射击损失高度的影响程度，指出俯仰角绝对值大、射击距离近、贪恋观看弹着点、退出时机晚、拉起过载小和拉杆粗猛等是影响地靶射击训练安全的重要因素，明确了退出地靶射击过程正确的驾驶方法，强调了靶场指挥员的重要作用，对提高对靶射击成绩，尤其是保证对地靶射击训练安全有着积极的意义。