航空发动机双转子系统的拍振分析

 在双转子航空发动机中,由于转子系统不可避免地存在不平衡量,当两个转子的转速比较接近时,发动机会出现拍振现象,拍振将引起振动强度过大问题。对双转子系统的拍振进行了研究,分析了拍振的周期性、信号强度及其反向转子特性,阐明了拍振产生的机理和特征,并采用数值仿真和试验对拍振进行了定量分析和验证。研究表明,拍振与双转子转速差和不平衡量的相位因素有关,当转速差小于工作转速的20%时,双转子系统拍振信号的强度较大。     

基于磁路法与等效热网络法的航天 永磁同步电机设计与仿真

针对航天永磁同步电机方案初步设计耗时长、过度依赖商业软件的问题,基于磁路法和热网络法,提出了一套方案设计阶段航天永磁同步电机磁热性能快速预估与仿真方法。给出了定子内径、定子外径、铁芯长度、匝数等关键参数的取值准则,建立了包含36个节点集总参数热网络模型,并以端部绕组为例给出了热平衡方程的详细推导过程。通过与成熟商业软件对比,其电磁计算最大误差出现在电流有效值上,偏差值为607%;与样机实测值对比,绕组温升最大误差为73%,满足方案设计阶段预示精度要求,为方案设计阶段航天永磁同步电机快速性能预估提供有力支撑。     

存在干扰下的无人机中继站波束成形算法

无人机(UAV)通信具有部署快、使用灵活、通信质量好等优点,在无线通信领域具有广阔的应用前景。采用UAV作为中继站构成的增强型卫星通信网络经常受到各种干扰的影响,导致其性能急剧下降。以信干噪比(SINR)最大化为准则,UAV中继站发射功率满足要求为约束条件的优化问题的基础上,提出了一种基于最大瑞利熵的波束成形(BF)算法,得出最优权矢量。为了降低BF算法的实现复杂度,进一步提出了一种基于迫零(ZF)的次优BF算法。计算机仿真验证了这2种BF算法的有效性。     

Eliminating negative VTEC in global ionosphere maps using inequality-constrained least squares

Currently, ground-based Global Navigation Satellite System (GNSS) stations of the International GNSS Service (IGS) are distributed unevenly around the world. Most of them are located on the mainland, while only a small part of them are scattered on some islands in the oceans. As a consequence, many unreasonable zero values (in fact negative values) appear in Vertical Total Electron Content (VTEC) of European Space Agency (ESA) and Center for Orbit Determination in Europe (CODE) IONEX products, especially in 2008 and 2009 when the solar activities were rather quiet. To improve this situation, we directly implement non-negative physical constraints of ionosphere for global ionosphere maps (GIM) with spherical harmonic functions. Mathematically, we propose an inequality-constrained least squares method by imposing non-negative inequality constraints in the areas where negative VTEC values may occur to reconstruct GIM models. We then apply the new method to process the IGS data in 2008. The results have shown that the new algorithm efficiently eliminates the unwanted behavior of negative VTEC values, which could otherwise often be seen in the current CODE and ESA GIM products in both middle and high latitude areas of the Southern Hemisphere (45°S∼90°S) and the Northern Hemisphere (50°N∼90°N). About 64% of GPS receivers’ DCBs have been significantly improved. Finally, we compare the GIM results between with and without the inequality constraints, which has clearly shown that the GIM result with inequality constraints is significantly better than that without the inequality constraints. The inequality-constrained GIM result is also highly consistent with the final IGS products in terms of root mean squared (RMS) and mean VTEC.     

酚醛树脂基纳米多孔材料的制备及结构调控

酚醛树脂基纳米多孔材料（Phenolic Resin-based Nanoporous Materials,PNM）是满足新一代航天飞行器轻质、高效隔热需求的新型热防护材料,传统制备方法中需使用超临界干燥技术,制备周期长、成本高。本研究通过两步法,即先合成线性酚醛树脂,再进行溶胶-凝胶的方法,实现了常压干燥PNM的制备。系统研究了固化剂含量、固化温度和固化时间对材料结构的影响和调控作用,分析了影响材料收缩率和热稳定性的因素。结果表明,PNM的微观纳米结构的变化会影响材料干燥后的收缩率,制备大颗粒、大孔径的微观结构更有利于降低材料的收缩率。而PNM的热稳定性主要受交联反应过程形成的化学结构的影响,通过优化固化剂的含量可提高PNM的热稳定性。当固化剂含量为10%,固化温度提高至150℃,固化时间延长至48 h的条件下,获得的PNM有最高的热稳定性（900℃下的残碳率为54.2%）、最发达的孔结构（比表面积为264.0 m²/g、孔容为2.67 cm³/g、平均孔径为40.0 nm）和最小的收缩率（0%）。此PNM制备方法简单、性能优异,在未来航天飞行器上有广阔的应用前景。     

PIP工艺制备SiC晶须增强SiCf/SiC复合材料的性能

以不同界面层厚度的SiC纤维为增强相,采用先驱体浸渍裂解工艺(PIP)制备SiC_f(PyC)/SiC复合材料,并在复合材料基体中引入SiC晶须,对其性能进行研究。结果表明:热解碳(PyC)界面层厚度约为230 nm时,SiC纤维拔出明显,SiC_f/SiC复合材料拉伸强度、弯曲强度和断裂韧度分别达到192.3 MPa、446.9 MPa和11.4 MPa?m^1/2;在SiC_f/SiC复合材料基体中引入SiC晶须后,晶须的拔出、桥连及裂纹偏转等增韧机制增加了裂纹在基体中传递时的能量消耗,使复合材料的断裂韧度和弯曲强度分别提高了22.9%和9.1%。     

Focus Reflective Shock Wave Interaction with Flame

An experiment on deformation of flame under the effect of focusing shock wave reflection is performed with the help of multiple-spark camera to understand the flame instability of the deformation process. Methane and oxygen are mixed stoichiometrically to be used in the experiment. Based on Navier-Strokes equations, two-dimen- sional axisymmetric elementary reactions are numerically simulated. And the simulation results are solved by opti- cal calculation. Shaded pictures by simulation fit well with experimental photos. Focusing reflecton shock waves can affect the flame, which accelerates the deformation of flame and renders violent burning in high-energy flam- mable gases behind waves. Therefore anticlockwise whirlpool appears. It clusters around the external surface of flame and has a tendency to develop toward the right. Finally, the whirlpool focuses on the right side of the flame, which involves the fresh unfired gases into the whirlpool circle, and consequently the head of mushroom cloud is formed. Meanwhile, when shock wave passes through the flame, the intensity of the shock waves on the axis is strengthened.