气热耦合条件下涡轮静叶三维优化

为解决涡轮静叶尾缘烧蚀问题并提升气动效率,采用气热耦合优化的方法对该叶片进行优化,优化分为对叶型优化以及对弯叶片优化两部分。优化结果显示,对叶型进行优化时由于叶型变化以及冷气流量增加2.68%导致叶片平均温度降低4.15%,最高温度下降61.7K,气动效率提升0.17%;对弯叶片进行优化时,顶部正弯效果明显,冷气流量增加0.11%,叶片平均温度下降2.4%,最高温度下降10.6K,气动效率提升0.16%。通过分析,对于该径高比较小的叶片,无论是叶型变化还是弯叶片变化,低能流体由端区进入主流导致的端区损失降低和激波损失的降低是导致气动效率提升的主要原因;冷气流量加大以及端区二次流减弱是造成叶片温度场降低的主要原因。     

Carbon dioxide removal system for closed loop atmosphere revitalization,candidate sorbents screening and test results

Due to the difficulty and expense it costs to resupply manned-spacecraft habitats, a goal is to create a closed loop atmosphere revitalization system, in which precious commodities such as oxygen, carbon dioxide, and water are continuously recycled. Our aim is to test other sorbents for their capacity for future spacecraft missions, such as on the Orion spacecraft, or possibly lunar or Mars mission habitats to see if they would be better than the zeolite sorbents on the 4-bed molecular sieve. Some of the materials being tested are currently used for other industry applications. Studying these sorbents for their specific spacecraft application is different from that for applications on earth because in space, there are certain power, mass, and volume limitations that are not as critical on Earth. In manned-spaceflight missions, the sorbents are exposed to a much lower volume fraction of CO₂ (0.6% volume CO₂) than on Earth.LiLSX was tested for its CO₂ capacity in an atmosphere like that of the ISS. Breakthrough tests were run to establish the capacities of these materials at a partial pressure of CO₂ that is seen on the ISS. This paper discusses experimental results from benchmark materials, such as results previously obtained from tests on Grade 522, and the forementioned candidate materials for the Carbon Dioxide Removal Assembly (CDRA) system.     

一种组合体航天器帆板的光照遮挡计算新方法

提出了一种新的太阳帆板遮挡计算方法,用于组合体航天器的能量平衡分析与计算。根据航天器轴线与帆板转轴垂直的几何关系,将其沿轴线离散化为若干平面的集合,将所分析的帆板离散化为点集,判断离散点沿太阳矢量逆向是否经过离散的舱体平面或其它帆板平面,以此确定遮挡关系。通过仿真计算得到不同入射太阳方向下某组合体对应的遮挡区域,结果表明,新方法适用于轴对称形状组合体航天器的帆板遮挡分析。     

Photonic spin control for solar wind electric sail

The electric solar wind sail (E-sail) is a novel, efficient propellantless propulsion concept which utilises the natural solar wind for spacecraft propulsion with the help of long centrifugally stretched charged tethers. The E-sail requires auxiliary propulsion applied to the tips of the main tethers for creating the initial angular momentum and possibly for modifying the spinrate later during flight to counteract the orbital Coriolis effect and possibly for mission specific reasons. We introduce the possibility of implementing the required auxiliary propulsion by small photonic blades (small radiation pressure solar sails). The blades would be stretched centrifugally. We look into two concepts, one with and one without auxiliary tethers. The use of small photonic sails has the benefit of providing sufficient spin modification capability for any E-sail mission while keeping the technology fully propellantless. We conclude that small photonic sails appear to be a feasible and attractive solution to E-sail spinrate control.     

高超声速飞行器流动特征分析

在非流线型构件或突起物的扰动效应、高马赫数和低雷诺数极限效应、低湍流度环境效应和由激波或摩擦导致的气动加热效应等4个方面的影响下,未来高超声速飞行器涉及的流动主要表现出这样的特点:典型流动结构强度高、尺度大,如强激波和厚边界层;局部流动结构数量多;激波、膨胀波和边界层结构之间相互干扰十分严重;转捩、压力脉动和一些流动结构对细微因素非常敏感;压力、摩擦应力和热流峰值现象普遍;升阻比屏障难以突破;流场同时依赖大量无量纲参数和有量纲参数,导致实验模拟难度大。本文在回顾传统高超声速流动主要流动现象的基础上,对上述7个方面涉及的典型流动现象的基础研究现状、问题本质和因果关系进行综合描述,讨论如何更有效地面对基础研究和工程实际问题。该文既可为解决典型流动现象中尚未解决的基础研究提供帮助,也可为如何合理地利用有限的已知知识解决工程应用问题提供指导。     

测控雷达伺服系统整流电路的建模与仿真

电力电子整流电路是测控雷达伺服系统的重要组成部分。某型测控雷达采用了三相零式反并联可逆整流电路结构。分析了整流电路可逆运行的工作原理以及晶闸管触发电路的控制方式,利用MATLAB/Simulink的建模功能,建立了触发脉冲产生电路和整流电路的模型,仿真得出系统可逆运行时电机的工作状态以及整流电路输出电压波形。仿真结果显示,此整流电路可以实现电机的四象限运行,所建模型正确。利用该模型可以对测控雷达伺服系统的分析和设计起到很好的辅助作用。     

卫星ATM网络中自适应FEC情况下的有效带宽估计

针对采用自适应前向差错控制（AFEC）的卫星异步传递模式（ATM）网络，研究了两种有效带宽估计方法。由于AFEC码率的动态特性使业务实际的传输速率具有不固定性，因此估计有效带宽时要考虑AFEC的影响。首先针对一般卫星时变信道和多码率AFEC情况下的卫星ATM，应用流体近似方法分析了有效带宽的计算，然而该方法要求的条件及计算复杂度均比较高，应用中有局限性。以此方法为基础，提出了采用修正因子的估计方法。数值结果表明采用修正因子的有效带宽估计方法比较简单可靠，适用面较广。     

大功率氧煤燃烧器内湍流气固两相流动数值模拟

本文对新型同轴射流缩口式氧煤枪所组成的大功率氧煤燃烧器内冷态轴对称二维湍流气固两相流动用ｋ－ｅ－ＡＰ两相湍流模型进行了数值预报，揭示了燃烧器内两相流场特征，预报结果和实验结果相符。进一步对相应高炉实际工况高速条件下的冷态两相流场进行了预报，其结果为优选结构尺寸和流动参数提供了重要依据。     

低速溅射小行星表面采样的动力学仿真

开发了适用于小行星环境的大规模三维离散元程序DEMBody,针对低速射弹溅射表层风化层的小行星采样方案,仿真了相同质量不同形状的射弹在微重力环境下垂直射入颗粒床的过程,研究了溅射物质在采样器中的运动历程及最终收集质量与射弹形状的关系。结果表明,90°锥形射弹的采样效率最高。     

Transonic flutter computations for the NLR 7301 supercritical airfoil

A numerical investigation of the transonic steady-state aerodynamics and of the two-degree-of-freedom bending/torsion flutter characteristics of the NLR 7301 section is carried out using a time-domain method. An unsteady, two-dimensional, compressible, thin-layer Navier–Stokes flow-solver is coupled with a two-degree-of-freedom structural model. Fully turbulent flows are computed with algebraic or one-equation turbulence models. Furthermore, natural transition is modeled with a transition model. Computations of the steady transonic aerodynamic characteristics show good agreement with Schewe's experiment after a simplified accounting for wind-tunnel interference effects is used. The aeroelastic computations predict limit-cycle flutter in agreement with the experiment. The computed flutter frequency agrees closely with the experiment but the computed flutter amplitudes are an order of magnitude larger than the measured ones. This discrepancy is likely due to the omission of the full wind-tunnel interference effects in the computations.