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...     

翼型表面结冰准定常数值模拟

对翼型表面的结冰过程进行了准定常数值模拟。在每个时间步长内完成网格随着壁面边界的移动而更新、周围流场和水滴撞击特性重新计算、冰形计算及壁面边界的重构工作,如此循环直至所需的结冰计算时间。采用拉格朗日轨迹追踪法获得水滴撞击特性,应用考虑壁面粗糙度影响的边界层积分法计算壁面的对流换热系数,在此基础上求解Messinger结冰热力学模型,冰层始终沿壁面外法线方向生长。对NACA0012翼型在不同环境下生成的三种典型冰形进行了预测,并与实验结果进行了比较,表明本文所述方法的有效性。     

风力机叶片翼型的结冰数值模拟研究

研究了风力机叶片翼型的结冰数值模拟方法,及翼型结冰后对其气动性能的影响。求解雷诺平均N-S方程,引入k-ωSST湍流模型封闭方程,获得风力机叶片流场;采用拉格朗日法计算风力机叶片翼型周围的水滴运动轨迹,同时考虑了多尺寸水滴分布的影响,获得翼型表面的局部水收集系数分布;根据质量守恒和能量守恒原理,计算翼型表面的各项热流,获得翼型表面的结冰速率和结冰冰形;考虑到翼型结冰是时间的动态函数,采用多时间步长法完成结冰数值模拟。计算了风力机叶片翼型在不同环境条件和气象条件下的结冰冰形,同时模拟了风力机翼型结冰后周围流场的变化,并与干净翼型的气动特性进行了对比。结果表明,环境温度较高时形成的明冰对翼型气动性能的影响较大,结冰导致翼型升力下降,升阻比减小,最大减小幅度达到61%,同时结冰后的翼型会提前进入失速区,导致桨叶气动性能恶化。     

Indicators of black-hole mass and Eddington accretion ratio from QSO X-ray and UV spectra

The evolution of luminous QSOs is linked to the evolution of massive galaxies. We know this because the relic black-holes found locally have masses dependent on the properties of the host galaxy’s bulge. An important way to explore this evolution would be to measure dependences of black-hole masses and Eddington accretion ratios over a range of redshifts, i.e., with cosmological age. For low redshift QSOs (and their lower luminosity Seyfert galaxy counterparts) it has been possible to infer black-hole masses from the luminosities and velocity dispersions of their host-galaxy bulges. These masses agree with those virial black-hole masses calculated from the Doppler widths of the broad Hβ emission lines. The latter method can then be extended to more distant and luminous QSOs, up to redshifts of 0.6 with ground-based optical observations. We discuss ways to extend these explorations to higher redshifts – up to 3 using the widths of QSOs’ broad UV emission lines, and in principle, and to redshifts near 4 from ground-based infrared observations of rest-frame Hβ at 2.5 μm. We discuss the possibility of investigating the accretion history of the higher redshift QSOs using measures of Eddington accretion ratio – the soft X-ray spectral index and the eigenvectors of Principal Components Analyses of QSOs’ UV emission-line spectra.     

Evolution of the periodicities in 2S 0114+650

We have analysed 9 years of data from the All Sky Monitor on the Rossi X-ray Timing Explorer for 2S 0114+650 to study the evolution of its spin, binary, and super-orbital periods. The spin history of the neutron star in this system exhibits torque reversals lasting 1 year. The newly discovered super-orbital period has remained stable over the 9-year span, making 2S 0114+650 the fourth known system to exhibit stable super-orbital modulation. We compare its super-orbital period evolution with those of the other three such systems.     

动力对全机水滴收集率的影响计算

针对飞机在飞行中遭遇过冷水滴撞击并结冰现象,建立了适合于发动机带动力情况下结冰过程水滴收集率计算的三维数值方法和计算程序.其基本思路为:采用多块技术与SIMPLE方法计算空气流场,以流场分布的计算结果为基础,求解水滴相的控制方程,进而获得物体表面的水滴收集率.空气相控制方程和水滴相控制方程均写成典型输运方程的形式,采用一致的有限体积法离散求解,方便了计算程序的编制.对某型运输机巡航构型有/无动力条件的水滴收集率进行了比较计算,获得了不同直径水滴在飞机表面的撞击特征以及水滴收集率在飞机机翼、平尾、垂尾和发动机进气道唇口上的分布规律.研究表明:(1)发动机是否带动力对机翼、平尾、垂尾的水滴收集率基本无影响;(2)飞机带动力主要影响发动机进气道唇口处的水滴收集率,带动力后唇口的收集率比无动力情况高,水滴撞击范围增大,在进行防除冰研究和设计时需引起重视.     

Appearance of neutron stars in the state of subsonic propeller

The state of subsonic propeller is intermediate between the states of supersonic propeller and accretor in the evolutionary tracks of magnetized compact stars. The rotational rate of a star at this stage decelerates due to the interaction between its magnetosphere and the surrounding hot, quasi-static plasma envelope. The magnetospheric radius is smaller than the corotation radius and the boundary of the magnetosphere is stable with respect to interchange instabilities. The rate of the mass flux from the inner radius of the envelope to the stellar surface is limited by the rate of plasma diffusion into the magnetic field of the star. As a result, the subsonic propeller would appear as a low-luminosity accretion-powered pulsar with a soft X-ray spectrum.     

旋转整流罩积冰过程中水膜流动和脱离的数值研究

为了更准确地模拟旋转整流罩积冰过程,在现有三维积冰与冰层表面薄水膜流动耦合模型基础上,基于功平衡分析的方法引入了旋转部件表面水膜脱离模型,并发展了相应的计算方法,给出了水膜脱离的判定依据:当气流曳力做的功和由于离心力使水膜增加的潜能之和大于黏附功时整流罩表面的水膜会发生脱离。对旋转整流罩积冰进行数值模拟,计算结果与实验结果吻合得较好,验证了该模型的合理性和计算方法的可行性。之后分析了转速和来流速度对整流罩表面水膜脱离和积冰的影响,结果表明:转速和来流速度越大,水膜发生脱离的比例越大。在研究范围内,转速为3000r/min和6000r/min时,因水膜脱离导致积冰总量分别减少13.4%和15.8%;来流速度为40、50m/s和60m/s时,因水膜脱离导致积冰总量分别减少为12.2%、13.4%、14.2%。      

飞机机翼积冰研究方法和进展分析

通过对目前国内外研究飞机机翼积冰三种方法的分析,指出了它们各自优缺点,重点介绍了现行国内外研究的进展和新趋势,提出了研究方法的改进方案和进一步研究的建议。     

风洞侧壁干扰对机翼表面霜冰的影响

采用数值模拟的方法研究了不同阻塞度下侧壁干扰对NACA0012翼型表面霜冰生长的影响。通过对流场和水滴撞击特性的研究发现:侧壁干扰会压缩来流空气,致使更多水滴跟随气流向机翼前缘汇集,增大了翼面水滴收集系数,且翼面水滴总收集量与阻塞度成正比、与液滴雷诺数成反比;同时会改变水滴的撞击方向,使水滴撞击极限和最大水收集系数的位置发生偏移。采用多步法对结冰特性的研究发现:在基准计算工况下,当阻塞度为20%时,侧壁干扰效应带来结冰量的相对附加增量约为16%;在同一阻塞度下,各时间步长内的结冰相对附加增量基本相等。提出了一种表征侧壁干扰对水滴收集影响强弱的因子,该影响因子与水滴收集相对附加增量具有较高的线性关系。