三角翼机翼摇滚主动控制多学科耦合数值模拟

细长机身和大后掠机翼气动构型的飞行器大攻角飞行时,由于缺少横向阻尼,易发生以绕体轴滚转振动为主的摇滚运动,飞行安全受到严重威胁。针对三角翼摇滚问题,采用动网格技术,建立了气动、运动和控制多学科耦合的数值模拟方法。通过耦合非定常Navier-Stokes方程、刚体运动方程和经典控制律,采用控制面差动偏转的方式对三角翼摇滚主动控制过程进行了数值模拟,并分析了不同控制状态下三角翼受控滚转的运动特性。在来流马赫数为0.3的条件下,实现了80°后掠三角翼摇滚现象的有效控制。     

翼间干涉效应对蜻蜓悬停气动性能的影响

蜻蜓在悬停飞行过程中,通过控制翅膀的运动规律,进行前后翅相位差为180°的扑翼运动。为了分析两对翅膀之间的干涉效应对悬停气动性能的影响,利用计算流体力学手段对蜻蜓悬停状态的串列扑翼和单对翅扑翼进行模拟。通过对两种模式下的流场进行分析,并计算对比了悬停效率、气动力及气动功率的数据,发现了悬停状态下翼间干涉的气动效应：尾迹集中效应和来流偏折效应。尾迹集中效应可以减少翅膀附近的涡耗散和尾迹耗散,提高悬停效率;来流偏折效应可以通过减小后翅在下拍过程中的来流攻角,从而降低前缘涡的尺寸和强度,降低悬停功率。数值结果表明：在运动规律相同的情况下,与单独拍动的前翅和后翅进行的悬停相比,串列双翅悬停的效率分别提高了18.6%和25.5%,功率分别降低了4.8%和14.0%。     

“人字形小肋”对激波/边界层干扰的影响研究

在曼彻斯特大学跨声速风洞开展激波/边界层干扰及“人字形小肋”对其影响的实验研究。在马赫数1.85流场条件下,应用高速纹影、油流、皮托压力测量和基于压敏漆的壁面压力测量技术,研究“人字形小肋”流动控制方法对激波/边界层干扰的流动分离结构与尺寸、压力分布特性与波系特征等影响。结果显示激波/边界层干扰诱发流动分离,分离区呈现三维特征,在“人字形小肋”的作用下,分离线呈现“波浪”形且整体向上游移动,干扰区流向尺寸增大,分离区高度减小且长度略增大,再附区的压力极值降低,这些特征与叶片、尖楔等微涡发生器的影响趋势相反。下一步工作中,拟针对“人字形小肋”开展参数优化研究,“人字形小肋”可能成为降低激波/边界层干扰诱发的高热流载荷的有效方法。     

Catching spiral – S0 transition in groups. Insights from SPH simulations with chemo-photometric implementation

We are investigating the co-evolution of galaxies within groups combining multi-wavelength photometric and 2D kinematical observations. Here we focus on S0s showing star formation in ring/arm-like structures. We use smooth particle hydrodynamical simulations (SPH) with chemo-photometric implementation which provide dynamical and morphological information together with the spectral energy distribution (SED) at each evolutionary stage. As test cases, we simulate the evolution of two such S0s: NGC 1533 and NGC 3626.     

斜下降旋翼桨涡干扰声源定位及表面压力

旋翼桨-涡干扰（BVI）是直升机在进场和离场等近地飞行时后行桨叶切割前行桨叶脱落桨尖涡产生的气动扰动，该扰动不仅对桨叶表面压力载荷产生激励作用，同时也会引起旋翼噪声出现激增，旋翼噪声激增的主要成分为桨-涡干扰噪声。本文首先对斜下降桨-涡干扰状态桨叶表面载荷进行数值计算；然后分别阐述了基于改进整周期同步平均旋翼噪声去噪方法、基于多层小波包分解的桨-涡干扰声源识别和分离方法以及基于bartlett时延计算和球面插值的声源定位方法，设计并开展了风洞斜下降状态桨-涡干扰桨叶表面压力和声源定位试验，给出了开发的声源定位软件界面、声源定位图像畸变校准方法及声阵列现场校准方法；最后对比分析了不同试验状态的桨-涡干扰噪声声源特性以及和桨叶表面压力之间的关联性，并给出了声源定位及表面压力试验数据分析结果。结果表明典型斜下降状态后行侧桨-涡干扰主要出现在方位角310°~330°、径向位置1.6~1.8 m桨盘平面区域。     

Correlations between neutral and ionized solar wind

We report results of a statistical study correlating ionized solar wind (ISW) fluxes observed by ACE during late 2000 and throughout 2001 with neutral solar wind (NSW) fluxes observed by IMAGE/LENA over the same period. The average correlation coefficient between the neutral and ionized solar wind is 0.66 with correlations greater than 0.80 occurring about 29% of the time. Correlations appear to be driven by high solar wind flux variability, similar to results obtained by in situ multi-spacecraft correlation studies. In this study, however, IMAGE remains inside the magnetosphere on over 95% of its orbits. As a function of day of year, or equivalently ecliptic longitude, the slope of the relationship between the neutral solar wind flux and the ionized solar wind flux shows an enhancement near the upstream direction, but the symmetry point appears shifted toward higher ecliptic longitudes than the interstellar neutral (ISN) flow direction by about 20°. The estimated peak interstellar neutral upstream density inside of 1 AU is about 7 × 10⁻³ cm⁻³.     

螺旋桨安装效应对无人机气动特性影响

为解决某型飞翼布局无人机(UAV)带动力构型风洞试验最大升阻比相对无动力状态大幅下降的问题,采用计算流体动力学(CFD)方法对无人机无动力与带动力构型进行了数值模拟,数值模拟结果分别与无动力以及带动力风洞试验数据吻合良好,在此基础上深入研究了螺旋桨安装效应对无人机气动特性的影响。结果表明:推力螺旋桨与机身之间气动干扰产生的低压区致使阻力增加,从而导致飞机最大升阻比相比无动力状态下降了30.7%。针对无人机在推力螺旋桨影响下出现的最大升阻比下降问题,采用增大螺旋桨与机身之间距离的方法可以有效地消除机身后部出现的低压区,减小了阻力,提升了无人机最大升阻比。桨毂拉长方案在8°和9°迎角下最大升阻比分别提升了17.3%和15.4%。     

Azimuthal propagation of Pc5 geomagnetic field pulsations in the southern polar cap

A statistical analysis of low frequency geomagnetic fluctuations at the two Antarctic stations Mario Zucchelli Station (geographic coordinates: 74.7°S, 164.1°E; corrected geomagnetic coordinates: 80.0°S, 306.8°E) and Dumont D’Urville (geographic coordinates: 66.7°S, 140.0°E; corrected geomagnetic coordinates: 80.4°S, 236.0°E) is shown. The analysis focuses on power spectra, coherence and phase difference between the stations, which are both located in the polar cap, with a 5-h magnetic local time displacement along a geomagnetic parallel; in this situation, the phase difference between geomagnetic fluctuations indicates the direction of their azimuthal propagation. Coherent fluctuations have been found to occur preferably when both stations are on the same side (dawnward or duskward) with respect to the polar cusp; moreover, around local magnetic midnight, they occur essentially during open magnetospheric conditions. The phase difference for coherent fluctuations indicates a propagation direction away from local geomagnetic noon and midnight. Also the analysis of three individual pulsation events, occurring at different times during the day, is shown; they are characterized at the two stations by simultaneous, coherent fluctuations, whose phase difference finds correspondence with the statistical behaviour.     

The LAGEOS satellites orbit and Yukawa-like interactions

LAGEOS II general relativity pericenter precession has been analysed in terms of the errors produced by the mismodelling of both the gravitational and non-gravitational perturbations acting on the satellite orbit. The accuracy in the pericenter determination may be considered as an upper-bound value for the estimate of the strength α of a possible new-long-range-interaction described by a Yukawa-like potential. In the present work we have focused on the constraints in α that can be obtained with the current best multi-satellites gravity field model EGM96 (α < 2.6 × 10⁻¹⁰) and also with the first promising models from the CHAMP (α < 1.8 × 10⁻¹⁰) and GRACE (α < 1.2 × 10⁻¹⁰) gravimetric missions. These results represent, potentially, an improvement of two or three orders-of-magnitude with respect to the best constraints obtained in the past with Earth–LAGEOS and Lunar–LAGEOS data (|α| < 10⁻⁵–10⁻⁸). The impact of the non-gravitational perturbations mismodelling in the final error budget has been determined together with the improvements obtainable in the constraint of the strength α with the proposed LARES satellite.     

叶轮机转静干涉计算建模方法比较

通过对尾迹-叶片干涉和激波-叶片干涉这两类典型转静干涉流动的模拟,对3种基于傅里叶分析的时域非定常计算建模方法,即形修正相延迟法、空间-时间梯度法和谐波平衡法进行对比分析;详细考察它们的区别与联系,不同方法的计算准确度和计算速度.计算表明:3种建模方法都可以很好地捕捉到非定常流动细节;与传统的时间推进法相比,计算速度提高了几倍到几十倍,可用于工程设计之中.