飞机支柱式起落架落震仿真及缓冲器优化分析

主要介绍支柱式起落架缓冲器的各个参数,包括缓冲支柱的初压力、初容积、油孔面积、活塞面积、缓冲支柱行程等。介绍起落架落震时缓冲器轴向载荷的计算公式。结合具体飞机型号利用初始参数通过AD-AMS软件建立数值模型并进行仿真分析,计算结果与试验结果比较,发现两者具有较好的一致性。最后以起落架缓冲器的油孔面积作为设计参数进行优化分析,给出最优值。     

钝锥有攻角分离流动的数值模拟及其分析

本文定性分析了开式分离的性状,并对钝锥有攻角超声速绕流的开式分离作了数值模拟。分析指出,开式分离可能存在两种形态,第一种分离线的起点为正常点,第二种分离线的起始为鞍、结点(包括螺旋点)的组合。对于第一种形态,分离线的起点是横向分离的起始点,除分离线外,分离面上的流线不是从分离线的起点发出的。对文中计算的情况,流动属第一种开式分离。计算证实了定性分析的结论。计算和分析均指出,对第一种开式分离,在分离的起始区域,分离流面尚未卷曲,但在下游,则变成卷曲面。文中还研究了围绕物体的流管在分离诱导下的变形情况。     

一种模拟喷管二维流场的新方法

采用ＳＩＭＰＬＥ方法对固体火箭发动机喷管进行了纯气相流场的数值模拟。推导了建立在同位网格之上利用协变物理速度分量为计算变量的离散方程，采用协变物理速度分量推导压力修正方程，对密度采用一阶迎风格式插值，将ＳＩＭＰＬＥ方法扩大到计算可压流动。计算结果表明：本方法计算精度高，收敛速度快，程序编写简单。     

基于FW-H方程的旋翼气动声学计算研究

由流体力学N S方程导出的非齐次波动方程———FfowcsWilliams Hawkings方程(简称FW H方程),可以精确地描述在静止流体中运动的物体与流体相互作用的发声问题。以FW H方程为理论模型,将旋翼桨叶运动发声问题等效为包含桨叶的任意运动控制面(声源面)的声辐射问题,并在旋翼绕流Euler方程数值模拟的基础上,在时域内计算了悬停旋翼和前飞旋翼的声场。应用于UH 1H和AH 1/OLS两种旋翼模型的气动声学计算表明:计算结果与噪声实验值符合良好;所研制的程序不仅能够较准确地计算单极子噪声和偶极子噪声,而且具有较强的跨音速四极子噪声预测能力。     

激光微推进器用于微小卫星的姿轨控仿真

为研究激光微推进器用于微小卫星在轨空间飞行任务的可行性,利用已建立的激光推进微小卫星仿真平台,对微小卫星在轨姿态调整、轨道维持和轨道转移等飞行任务进行了仿真和分析。仿真结果表明,星载激光微推进器可满足在轨微小卫星的高控制精度姿态调整、近地观测轨道维持以及较长时间要求的轨道转移等空间任务对推进系统的要求。     

Deep Impact: Working Properties for the Target Nucleus – Comet 9P/Tempel 1

In 1998, Comet 9P/Tempel 1 was chosen as the target of the Deep Impact mission (A’Hearn, M. F., Belton, M. J. S., and Delamere, A., Space Sci. Rev., 2005) even though very little was known about its physical properties. Efforts were immediately begun to improve this situation by the Deep Impact Science Team leading to the founding of a worldwide observing campaign (Meech et al., Space Sci. Rev., 2005a). This campaign has already produced a great deal of information on the global properties of the comet’s nucleus (summarized in Table I) that is vital to the planning and the assessment of the chances of success at the impact and encounter. Since the mission was begun the successful encounters of the Deep Space 1 spacecraft at Comet 19P/Borrelly and the Stardust spacecraft at Comet 81P/Wild 2 have occurred yielding new information on the state of the nuclei of these two comets. This information, together with earlier results on the nucleus of comet 1P/Halley from the European Space Agency’s Giotto, the Soviet Vega mission, and various ground-based observational and theoretical studies, is used as a basis for conjectures on the morphological, geological, mechanical, and compositional properties of the surface and subsurface that Deep Impact may find at 9P/Tempel 1. We adopt the following working values (circa December 2004) for the nucleus parameters of prime importance to Deep Impact as follows: mean effective radius = 3.25± 0.2 km, shape – irregular triaxial ellipsoid with a/b = 3.2± 0.4 and overall dimensions of ∼14.4 × 4.4 × 4.4 km, principal axis rotation with period = 41.85± 0.1 hr, pole directions (RA, Dec, J2000) = 46± 10, 73± 10 deg (Pole 1) or 287± 14, 16.5± 10 deg (Pole 2) (the two poles are photometrically, but not geometrically, equivalent), Kron-Cousins (V-R) color = 0.56± 0.02, V-band geometric albedo = 0.04± 0.01, R-band geometric albedo = 0.05± 0.01, R-band H(1,1,0) = 14.441± 0.067, and mass ∼7×10¹³ kg assuming a bulk density of 500 kg m⁻³. As these are working values, {i.e.}, based on preliminary analyses, it is expected that adjustments to their values may be made before encounter as improved estimates become available through further analysis of the large database being made available by the Deep Impact observing campaign. Given the parameters listed above the impact will occur in an environment where the local gravity is estimated at 0.027–0.04 cm s⁻² and the escape velocity between 1.4 and 2 m s⁻¹. For both of the rotation poles found here, the Deep Impact spacecraft on approach to encounter will find the rotation axis close to the plane of the sky (aspect angles 82.2 and 69.7 deg. for pole 1 and 2, respectively). However, until the rotation period estimate is substantially improved, it will remain uncertain whether the impactor will collide with the broadside or the ends of the nucleus.     

直升机燃油系统地面模拟试验中试验台转角与油面角的关系

为了在直升机燃油系统地面模拟试验中准确地模拟油面角，本文介绍了试验台转角与油面角的关系，并给出了转换结果，同时，提出了一种用油箱内增压来模拟过载的设想，使在模拟试验时，油泵供油更趋真实，通过简化计算，给出了确定气压力的方法和判断依据。     

求解可压缩N－S方程的无粘－粘性分数步法

用按物理过程作时间分裂的无粘－粘性分数步法求解可压缩Ｎ－Ｓ方程，无粘步用高效欧拉算法解欧拉方程，粘性步用全隐格式解抛物方程；并采取了有效措施消除由分步法产生的时间和空间不相容性，文中给出了轴对称喷管内外流场的数值模拟结果。     

MATLAB电力系统模块中频谱分析的实现

给出了利用电力系统模块(PSB)工具箱对仿真波形进行频谱分析的一种新方法.该方法以MATLAB提供的PSBFFT_SCOPE函数为基础,对其输入变量加以改造,克服了其不能应用于变步长算法模型频谱分析的缺陷,拓宽了在PSB工具箱中进行频谱分析的范围.实际仿真结果表明,该方法分析正确,使用简捷,在实际仿真过程中是切实可行的.     

芳纶纤维／环氧复合材料界面超声连续改性处理

运用超声技术在芳纶/环氧复合材料制备过程中对其界面进行改性处理,分析了超声处理过程中纤维与树脂之间浸润性的变化趋势以及超声作用对复合材料界面性能和力学性能的影响。结果表明:超声是通过改善纤维与树脂之间的浸润性,提高复合材料的界面性能及力学性能。