高温相变单元管蓄热过程数值模拟

对以高温共晶盐 Li F-Ca F2 为相变材料 (PCM)和以干空气为工质的相变蓄热系统 ,采用焓方法建立了以控制体单元为对象的单管相变蓄热模型。在模拟空间站太阳能吸热 /储热器轨道运行参数下进行了数值计算。计算结果与地面模拟试验数据进行了比较 ,吻合良好。     

混合气体流动的一种数值模拟方法

本文建立一个数值模拟完全气体混合流动的理论模型.该模型首先应用混合气体的Euler方程和每种气体组分的质量分数方程来控制流动.为了消除混合网格内气体组分界面附近出现的非物理振荡,我们假定混合气体的每种组分达到了动力学平衡状态然而尚未达到热力学平衡状态.这种思想导致需要另外给定每种气体组分的总能量方程.为使用高分辨格式来求解这组双曲型偏微分方程并且简化对所需要的Jacobi矩阵的推导,混合气体的压力方程也被耦合起来.Godunov型的波传播方法被采用来离散求解所获得的控制方程.从典型算例结果来看,一维问题的数值解与精确解一致,二维问题的数值解与理论分析一致.这说明本文的理论模型是合理的.     

翼刀附面层控制二次流技术的研究现状及发展前景

翼刀技术是附面层控制技术的一种，主要是通过有效阻断端壁附面层或叶片吸力面附面层近端壁处低能流体的横向迁移或径向迁移以及反向翼刀涡的影响来控制二次流。国外对此项研究起步较早，重点集中在对汽轮机叶栅的实验研究上；而国内在近几年，才开始了对压气机叶栅中应用翼刀技术的实验和计算研究工作。     

形状记忆合金智能结构的主动振动抑制研究

 从形状记忆合金 (SMA)智能结构用于主动振动抑制的构想出发,建立了含SMA非线性本构关系的智能复合材料结构的有限元模型,并结合试验验证了主动振动抑制的效果。试验和计算结果都表明SMA是振动抑制的有效驱动器,通过主动应变能调整 (ASET)的方法对结构固有频率的影响非常显著,这种影响主要体现在基频 (一阶固有频率 )的改变上,对高阶固有频率的影响逐渐减小。     

航天飞机末端区域能量管理段制导技术概述

末端区域能量管理段主要是控制航天飞机的动能和势能．使航天飞机最终达到进场着陆段的初始要求，以保证其最终成功着陆。在最终制导系统引入一个能量基准剖面，通过调整飞行距离、动压或速度制动使航天飞机达到标准的能量状态。将末端区域能量管理段划分为四个飞行段，并对这四个飞行段的基本设计思想、制导技术及过程进行了研究。经过实际的航天飞机飞行验证．证明这种方案具有良好的制导效果。     

太阳能火箭发动机聚光器设计方法

对工程上常用聚光器进行了性能比较,得出了适合于太阳能火箭发动机(STP)的聚光器及其具有的性能优点,研究了此种聚光器的的设计方法,并推出了相关公式和其中的关键技术,这对STP聚光器的工程设计具有重要的指导价值。      

氧化剂含量和粒度对NEPE推进剂燃速影响的模型化

以高能固体推进剂热分解特性和燃烧模型的研究成果为基础,建立了由化学结构参数计算NEPE推进剂的燃速和压强指数的公式,计算了氧化剂组分含量和粒度对燃烧性能的影响。经验证,计算结果与实测燃速值的偏差全部在±20%以内,其中80%的偏差在±10%以内。这说明所建立的模型基本合理,编制的NEPE类推进剂燃速计算程序基本可行。     

A Comparative Study of the Influence of the Active Young Sun on the Early Atmospheres of Earth, Venus, and Mars

Because the solar radiation and particle environment plays a major role in all atmospheric processes such as ionization, dissociation, heating of the upper atmospheres, and thermal and non-thermal atmospheric loss processes, the long-time evolution of planetary atmospheres and their water inventories can only be understood within the context of the evolving Sun. We compare the effect of solar induced X-ray and EUV (XUV) heating on the upper atmospheres of Earth, Venus and Mars since the time when the Sun arrived at the Zero-Age-Main-Sequence (ZAMS) about 4.6 Gyr ago. We apply a diffusive-gravitational equilibrium and thermal balance model for studying heating of the early thermospheres by photodissociation and ionization processes, due to exothermic chemical reactions and cooling by IR-radiating molecules like CO₂, NO, OH, etc. Our model simulations result in extended thermospheres for early Earth, Venus and Mars. The exospheric temperatures obtained for all the three planets during this time period lead to diffusion-limited hydrodynamic escape of atomic hydrogen and high Jeans’ escape rates for heavier species like H₂, He, C, N, O, etc. The duration of this blow-off phase for atomic hydrogen depends essentially on the mixing ratios of CO₂, N₂ and H₂O in the atmospheres and could last from ∼100 to several hundred million years. Furthermore, we study the efficiency of various non-thermal atmospheric loss processes on Venus and Mars and investigate the possible protecting effect of the early martian magnetosphere against solar wind induced ion pick up erosion. We find that the early martian magnetic field could decrease the ion-related non-thermal escape rates by a great amount. It is possible that non-magnetized early Mars could have lost its whole atmosphere due to the combined effect of its extended upper atmosphere and a dense solar wind plasma flow of the young Sun during about 200 Myr after the Sun arrived at the ZAMS. Depending on the solar wind parameters, our model simulations for early Venus show that ion pick up by strong solar wind from a non-magnetized planet could erode up to an equivalent amount of ∼250 bar of O⁺ ions during the first several hundred million years. This accumulated loss corresponds to an equivalent mass of ∼1 terrestrial ocean (TO (1 TO ∼1.39×10²⁴ g or expressed as partial pressure, about 265 bar, which corresponds to ∼2900 m average depth)). Finally, we discuss and compare our findings with the results of preceding studies.     

The Genesis Solar Wind Concentrator Target: Mass Fractionation Characterised by Neon Isotopes

The concentrator on Genesis provided samples of increased fluences of solar wind ions for precise determination of the oxygen isotopic composition. The concentration process caused mass fractionation as a function of the radial target position. This fractionation was measured using Ne released by UV laser ablation and compared with modelled Ne data, obtained from ion-trajectory simulations. Measured data show that the concentrator performed as expected and indicate a radially symmetric concentration process. Measured concentration factors are up to ∼30 at the target centre. The total range of isotopic fractionation along the target radius is 3.8%/amu, with monotonically decreasing ²⁰Ne/²²Ne towards the centre, which differs from model predictions. We discuss potential reasons and propose future attempts to overcome these disagreements.     

基于多体系统动力学的旋翼桨叶响应计算方法

在中等变形梁的基础上引入增广转换矩阵,为解决桨叶动能项推导编程计算较为复杂的问题,建立了一种新的递推计算方法。该方法在原有的转换矩阵基础上进行了增广,建立了相邻运动坐标系间动能项引起的质量、阻尼、刚度和广义力递推计算方法。以法国SA349/2小羚羊直升机的试飞测试数据为依据,验证了方法的有效性。