基于神经网络的翼型积冰预测

采用神经网络方法对翼型表面的积冰进行了预测研究.建立了一种型面曲线坐标系,通过坐标变换将积冰外形转化为几何曲线.利用傅立叶级数对此曲线进行拟合,实现积冰外形的参数化.以结冰条件作为输人,冰形参数作为输出构建神经网络,对NACA 0012翼型表面的积冰进行预测.通过将预测结果与实验结果以及数值模拟结果进行对比,说明所提出...     

积冰对飞机纵向操稳特性的量化影响

提出了一种根据气象条件、飞机特征、飞行条件预测积冰对飞机飞行动力学特性影响的估算方法.采用热力学平衡分析方法完成了积冰增长过程的数学描述,利用逐步线性回归方法建立了结冰飞机的气动模型,计算得到了结冰飞机的气动参数,计算结果与试验结果吻合较好,表明这种方法具有一定的工程实用性.并在此基础上研究了不同部位积冰对飞机纵向操稳特性的影响,通过数值仿真计算得出,结冰飞机气动特性的急剧恶化会导致其纵向操稳特性显著降低,严重时会危及其飞行安全.      

民用飞机临界冰型确定策略浅析

分析了适航规章第25部121修正案中关于民机临界冰型的修订内容,提出大型客机结冰适航验证所用临界冰型的确定策略。针对飞机不同飞行阶段分析飞机结冰特征,对飞机不同部件开展结冰参数临界性分析,确定临界结冰条件,结合结冰数值预测和冰风洞试验手段提出相应的临界冰型确定方法;同时提出适航验证所需失效冰型、延迟冰型等特殊冰型的确定方法。根据性能、操稳和动力专业对于结冰临界性的不同要求,对比评估各种冰型对飞机影响的严重程度,最终确定飞机用于适航验证的临界冰型。本文可为大型客机的结冰适航验证工作提供参考。     

The infra-red background generated by pregalactic stars and their remnants

We examine whether the IR background reported by Matsumoto (1983) could have been generated by stars or black holes in the pregalactic era, z=10100.     

Infrared radiation from compact X-ray sources

Observations of the X-ray binaries 4U 0115+634 and A 0535+262 performed in 1981 – 1982 revealed significant IR variabilities of these sources. 4U 0115+634 was observed twice, in the state close to X-ray activity, and in the state of low activity, thus changing from K = 7^m.75 to K > 9^m. A 0535+262 shows the temporal variations ranged from tens minutes to some days. The regular variations of IR brightness are suspected with teh period close to 104 s that corresponds to the period of axial rotation of neutron star in A 0535+262. The results obtained present arguments in favour of hypothesis that IR radiation is generated near the accreting neutron star and is possibly of maser nature.     

First millimetric detections of AE Aquarii

We report the first millimetric detections of the magnetic cataclysmic variable AE Aquarii, accompanied by contemporaneous microwave observations. These data show that the time-averaged spectrum is well fit by a power-law which extends to mm wavelengths. We suggest that the spectrum is consistent with that expected from a superposition of flare-like events.     

飞机积冰后若干飞行力学问题综述

回顾飞机积冰后若干飞行力学问题研究的历史与现状,着重介绍了积冰飞机气动数据的获取途径、积冰飞机飞行力学建模与飞行仿真、积冰对飞机稳定性和操纵性的影响以及积冰对飞机飞行性能的影响.在已有飞机积冰后飞行力学问题研究的基础上,提出了飞机积冰后飞行力学问题研究领域需要解决和关注的若干问题,包括通过数值模拟方法获取积冰飞机的气动数据、完善积冰对飞机气动导数影响的计算模型以及加强平尾失速方面的研究.今后需要进一步对模拟冰风洞、数值模拟方法和平尾失速进行研究,并获取更多实验数据.     

尾部可调的发动机进口支板结冰数值模拟研究

基于模块化思想,在FLUENT软件基础之上开发了发动机进口支板的结冰计算程序,针对尾部可调支板的结冰问题进行了计算研究。通过分析发动机进口支板结冰的物理过程,将支板结冰计算分成四个模块,分别为两相流流场计算、水滴收集计算、热力学分析和表面结冰量计算、动网格计算。首先将各模块单独进行研究,通过FLUENT提供的UDF函数及宏函数逐一实现各模块功能,最后将各模块整合,实现了发动机进口支板的结冰计算。通过计算获得了调整角度为30°时,支板的液态水含量分布、不同时间下支板结冰的区域以及不同温度下支板结冰的特点,给出了可调支板应重点防冰区域。数值模拟方法为工程应用提供了一条可选的途径。     

Alfvén waves in the context of solar-like star formation: accretion columns and disks

In this work we examine the damping of Alfvén waves as a source of plasma heating in disks and magnetic funnels of young solar like stars, the T Tauri stars. We apply four different damping mechanisms in this study: viscous-resistive, collisional, nonlinear and turbulent, exploring a wide range of wave frequencies, from 10⁻⁵Ω_i to 10⁻¹Ω_i (where Ω_i is the ion-cyclotron frequency). The results show that Alfvénic heating can increase the ionization rate of accretion disks and elevate the temperature of magnetic funnels of T Tauri stars opening possibilities to explain some observational features of these objects. This revised version was published online in August 2006 with corrections to the Cover Date.     

Black-hole transients: From QPOs to relativistic jets

Due to the impressive amount of new data provided by the RXTE satellite in the past decade, our knowledge of the phenomenology of accretion onto black holes has increased considerably. In particular, it has been possible to schematize the outburst evolution of transient systems on the basis of their spectral and timing properties, and link them to the ejection of relativistic jets as observed in the radio. Here, I present this scheme, concentrating on the properties of the quasi-periodic oscillations observed in the light curves and on the link with jet ejection.