机翼热气防冰系统设计

利用热流体系统仿真分析平台Flowmaster和计算流体力学软件Fluent进行联合仿真,对机翼热气防冰系统进行了设计和性能分析.设计参数包括防冰系统笛形管热气喷口孔径、孔数及孔间距等参数.基于Flowmaster对所设计的供气管路进行供气流量分配计算.基于Fluent模拟防冰腔内流动与换热,计算了防冰腔的热效率.根据防冰热载荷及热效率结果预测每段缝翼防冰所需热气流量,引入参数供气余度来分析防冰系统热性能.所提出的热气防冰系统设计方法可为热气防冰系统的工程设计与优化提供重要的帮助.     

激光位移传感器高速数据采集与处理系统设计

介绍了基于FPGA和单片机的激光位移传感器高速数据采集与处理系统的工作原理与软硬件设计,该系统采用FPGA作为核心控制器,主要完成A/D转换时钟控制、CCD像点位置提取、数据缓冲异步FIFO三部分功能。单片机负责键控、显示以及系统协调。这种基于FPGA和单片机的同步采集、实时读取采集数据的方案,可以提高系统采集和传输的速度。该硬件电路结构简单、成本低廉、可靠性高、功耗较低,满足了实际应用中的要求。     

DORIS processing at the European Space Operations Centre

This paper gives an overview of the DORIS related activities at the Navigation Support Office of the European Space Operations Centre. The DORIS activities were started in 2002 because of the launch of the Envisat satellite where ESOC is responsible for the validation of the Envisat Precise Orbits and a brief overview of the key Envisat activities at ESOC is given. Typical orbit comparison RMS values between the CNES POE (GDR-C) and the ESOC POD solution is 6.5, 18.8 and 23.1 mm in radial-, along- and cross-track direction. In the framework of the generation of the ITRF2008 ESOC participated in the reprocessing of all three space geodetic techniques; DORIS, SLR, and GPS. Here the main results of our DORIS reprocessing, in the framework of the International DORIS Service (IDS), are given. The WRMS of the weekly ESOC solution (esawd03) for the 2004–2009 period compared to the IDS-1 combined solution is of the order of 12 mm. Based on the long time series of homogeneously processed data a closer look is taken at the estimated solar radiation pressure parameters of the different satellites used in this DORIS analysis. The main aim being the stabilization of the Z-component of the geocentre estimates. We conclude that the ESOC participation to the IDS ITRF2008 contribution has been beneficial for both ESOC and the IDS. ESOC has profited significantly from the very open and direct communications and comparisons that took place within the IDS during the reprocessing campaign.     

The characteristics of sharp (small-scale) boundaries of solar wind plasma and magnetic field structures

We investigate properties of large (>20%) and sharp (<10 min) solar wind ion flux changes using INTERBALL-1 and WIND plasma and magnetic field measurements from 1996 to 1999. These ion flux changes are the boundaries of small-scale and middle-scale solar wind structures. We describe the behavior of the solar wind velocity, temperature and interplanetary magnetic field (IMF) during these sudden flux changes. Many of the largest ion flux changes occur during periods when the solar wind velocity is nearly constant, so these are mainly plasma density changes. The IMF magnitude and direction changes at these events can be either large or small. For about 55% of the ion flux changes, the sum of the thermal and magnetic pressure are in balance across the boundary. In many of the other cases, the thermal pressure change is significantly more than the magnetic pressure change. We also attempted to classify the types of discontinuities observed.     

Acceleration of interplanetary pick-up ions and anomalous cosmic rays

It may not be doubted anymore that anomalous cosmic rays (ACRs) are produced in the heliosphere from interplanetary pick-up ions through their acceleration at the solar wind termination shock. However, there is no general agreement in the community of heliospheric researchers concerning the mechanism of injection of the pick-up ions into the shock acceleration. We discuss here three possible ways for pick-up ions to be involved into the acceleration process at the termination shock: (1) preacceleration of pick-up ions in the whole region from the Sun up to the termination shock by solar wind turbulences and interplanetary shock waves, (2) local preacceleration of pick-up ions in a vicinity of the termination shock by shock surfing, and (3) formation of high-velocity tails in pick-up ion spectra consisting of secondary pick-up ions which are produced in the supersonic solar wind due to ionization of energetic neutral atoms entering from the inner heliosheath.     

后掠翼对细长体中段大迎角绕流的影响

采用在细长体顶点处添加扰动块的方式使细长体的绕流具有确定性.研究了在大迎角下,后 掠翼对细长体绕流结构和气动力特性的影响.实验结果表明,在30°迎角时,细长体中段背 风侧的流动和压力分布受到后掠翼与头部背涡的双重控制.在迎角α=40°~60°范围内 , 后掠翼对细长体中段绕流起主控作用,使细长体中段背风侧流动呈现完全分离流状态,使得 中段背风侧的压力分布保持为均值.      

飞机侧向波束导引控制系统结构方案及仿真

侧向波束导引控制系统是飞机在自动着陆时所采用的一种重要无线电波束导引系统。分析了侧向波束导引控制系统原理,基于飞机协调控制,构建一种侧向波束导引控制系统结构方案,在 MATLAB平台下,对所设计的侧向波束导引控制系统进行大量仿真研究。仿真结果显示,所设计的侧向波束导引控制系统结构是合理的,当其侧向耦合器结构参数设置准确时,可很好地改善导引控制系统的稳定性及动态品质。     

尾缘锯齿结构的降噪物理机制实验

对比分析了常规尾缘翼型与锯齿尾缘翼型尾缘湍流流场的基本特征,并通过线阵列的方法测量了两种尾缘结构的噪声.结果表明:锯齿尾缘翼型尾缘湍流流场的湍流强度以及3个方向上的湍流强度都相比于常规尾缘翼型有显著减少,声场结果显示锯齿尾缘翼型对尾缘噪声有显著减小,对前缘噪声影响很小.锯齿结构加宽了尾迹区域并加快了大涡的破碎,产生了额外的马蹄涡,湍流脉动衰减率沿着流动方向变大.      

有翼高超声速再入飞行器气动设计难点问题

有翼高超声速再入飞行器是近年来的研究热点,气动设计是飞行器设计的关键。为了更清楚地认识有翼高超声速再入飞行器气动设计的难点问题,对有翼高超声速再入飞行器的发展、优势及总体任务剖面进行了介绍,从5个方面详细介绍了该类飞行器气动设计的难点问题,包括多约束复杂面对称气动布局设计、高温真实气体效应对气动特性影响、天地差异与天地换算方法、反作用控制系统(RCS)喷流干扰对气动特性的影响以及气动数据不确定度等,简要阐明了这些难点问题对总体设计的重要性以及初步的解决思路,为有翼高超声速再入飞行器气动设计提供了一些参考。     

航天器贮箱变质量流固耦合系统的动力学响应

研究了航天器贮箱变质量流固耦合系统的动力学特性.根据虚拟质量法(VMM),结合边界元法和有限元法构建了系统的动力学模型,建模过程中着重考虑了质量变化对系统的动态影响.通过Newmark直接积分法计算出贮箱变质量系统的振动响应.结果表明:由于系统质量减少,引起了系统振动频率的增大,并产生一个附加负阻尼.系统的振动频率的范围可以通过系统质量的范围确定.变质量引起的附加负阻尼的大小与系统的质量变化率成正比.对于系统的横向振动,质量减少引起的附加负阻尼在整个过程对系统振动的影响比较稳定,对于系统的纵向振动,质量减少引起的附加负阻尼对系统振动的影响随时间的增加而增大.