用粘性涡方法计算伞状物绕流

文章用粘性涡方法计算了二维伞状物绕流问题。首先阐述了涡方法的基本理论 ,包括涡元的对流、粘性扩散、物面涡元的脱落、物体所受气动力计算等 ,然后介绍了使用涡方法的一般步骤。最后将完全充满的伞衣简化为二维圆弧壳 ,计算了伞衣内外压力分布、阻力系数及升力系数     

临近空间环境下封闭方腔内耦合换热特性

以临近空间浮空器载荷舱为应用背景,对复杂热边界条件下含热源的三维封闭方腔内自然对流、表面辐射和导热的耦合问题进行了数值模拟。综合考虑对流换热、长波辐射、太阳辐射等因素的影响,建立了临近空间热环境模型。通过Fluent软件用户自定义函数（UDF）引入外部非定常的辐射-对流耦合热边界条件,对腔内换热特性的昼夜变化进行研究,并分析了腔壁厚度、发射率和导热系数对其的影响。数值结果表明,腔内平均温度昼夜变化很小,约为12.9 K,但温度场分布随太阳方位变化而变化;腔内对流换热较弱,同一时刻最大温差约为71.3 K;腔壁热阻和发射率增加会削弱自然对流的强度。      

Design of nanofluid-cooled heat sink using topology optimization

The paper presented topology optimization of 2D and 3D Nanofluid-Cooled Heat Sink (NCHS). The flow and heat transfer problem in the NCHS was treated as a single-phase nanofluid based convective heat transfer model. The temperature-dependent fluid properties were taken into account in the model due to the strong temperature-dependent features of nanofluids. An average temperature minimum problem was studied subject to the fluid area and energy dissipation constraints by using the density method. In the method, the design variable is updated according to the gradient information obtained by an adjoint based sensitivity analysis process. The effects of the energy dissipation constraint, temperature-dependent fluid properties and nanofluid characteristics on optimal configurations of NCHS were numerically investigated with following conclusions. Firstly, branched flow channels in the optimal configuration increased with the rise of the allowed energy dissipation. Secondly, temperature-dependent fluid properties were significant for obtaining the appropriate optimal results with best cooling performance. Thirdly, heat transfer performances of optimal configurations were enhanced by reducing the nanoparticle diameter or increasing the nanoparticle volume fraction. Fourthly, the optimal configuration for nanofluid had better cooling performance than that for its base fluid.     

某支线飞机概念设计阶段机翼气动弹性设计

在飞机的总体方案概念设计阶段,需要对飞机机翼进行气动弹性设计,以避免在后期设计中,因气动弹性问题而对设计方案进行较大更改.以某支线飞机的总体方案论证为背景,研究并归纳该飞机概念设计阶段气动弹性设计与分析的理论基础和计算方法,建立机翼的梁架式模型,初步设计模型刚度与质量分布,并进行机翼的静气动弹性响应与载荷分析、振动特性及颤振特性分析.结果表明:该支线飞机机翼的气动弹性特性合理,符合设计要求.     

气膜约束对轴系固有频率影响的试验

对10kg转子进行自由状态和有气膜约束两种状态下的试验模态分析,试验结果给出了转子平动、锥动和一阶弯曲时的固有频率及其振型等模态参数,分析了轴承供气压力变化对轴系固有频率的影响.进行了轴系升降速试验,结果表明:气膜约束下的模态分析结果比自由状态下的更接近于升降速试验的结果.试验结果为气体轴系固有频率的确定以及控制参数的选取提供了依据,也为下一步轴系振动控制奠定了基础.      

Magnetospheric disturbances associated with the 13 December 2006 solar flare and their ionospheric effects over North-East Asia

We present an observational study of magnetospheric and ionospheric disturbances during the December 2006 intense magnetic storm associated with the 4В/Х3.4 class solar flare. To perform the study we utilize the ground data from North–East Asian ionospheric and magnetic observatories (60–72°N, 88–152°E) and in situ measurements from LANL, GOES, Geotail and ACE satellites. The comparative analysis of ionospheric, magnetospheric and heliospheric disturbances shows that the interaction of the magnetosphere with heavily compressed solar wind and interplanetary magnetic field caused the initial phase of the magnetic storm. It was accompanied by the intense sporadic E and F2 layers and the total black-out in the nocturnal subauroral ionosphere. During the storm main phase, LANL-97A, LANL 1994_084, LANL 1989-046 and GOES_11 satellites registered a compression of the dayside magnetosphere up to their orbits. In the morning–noon sector the compression was accompanied by an absence of reflections from ionosphere over subauroral ionospheric station Zhigansk (66.8°N, 123.3°E), and a drastic decrease in the F2 layer critical frequency (foF2) up to 54% of the quite one over subauroral Yakutsk station (62°N, 129.7°E). At the end of the main phase, these stations registered a sharp foF2 increase in the afternoon sector. At Yakutsk the peak foF2 was 1.9 time higher than the undisturbed one. The mentioned ionospheric disturbances occurred simultaneously with changes in the temperature, density and temperature anisotropy of particles at geosynchronous orbit, registered by the LANL-97A satellite nearby the meridian of ionospheric and magnetic measurements. The whole complex of disturbances may be caused by radial displacement of the main magnetospheric domains (magnetopause, cusp/cleft, plasma sheet) with respect to the observation points, caused by changes in the solar wind dynamic pressure, the field of magnetospheric convection, and rotation of the Earth.     

关于电磁场的自然单元法

有限元法和无网格法在电磁场数值计算中已经得到了广泛的应用,然而有限元法存在前处理网格剖分问题,无网格法存在计算时间长、边界条件和不连续面难处理等问题。针对以上问题,本文提出了利用自然单元法求解电磁场的方法,该方法根据场域中的离散点的信息构造自然邻点插值函数,最后算出场值。通过算例证明了该方法在电磁场计算中的可行性。     

复合热条件下椭球形封闭腔内低压气体的自然对流

以填充氦气的平流层浮空器为应用背景,对非均匀复杂热边界条件下大尺寸椭球形封闭腔内低压气体的自然对流热特性与动力学特性进行了数值模拟。以Fluent软件为基础,采用用户自定义函数(UDF)自编程技术引入外部非均匀的对流-辐射耦合热边界条件,考虑了低压气体密度对压力、温度的依赖关系。分析了不同条件下腔壁与内部气体温度、对流换热特性以及流场、压力、质心变化等动力学特性,通过数据分析,获得了腔内自然对流的局部对流换热系数关联式。研究结果表明,在平流层环境下,外部非均匀热边界条件及其变化对封闭腔内低压气体的自然对流热特性与动力学特性影响很大。     

Numerical study of forced convective heat transfer around a spherical aerostat

Forced convective heat transfer is one of the major factors that dominate the thermal behaviors of aerostats. Due to the large physical size, the convection around an aerostat has high Reynolds numbers. The existing forced convective heat transfer correlations are limited to the Reynolds number lower than 10⁵, which are not appropriate for aerostat applications. Therefore, it is necessary to obtain a convective heat transfer correlation applicable to spherical aerostats at high Reynolds numbers. In this paper, steady convective heat transfer from an isothermal spherical aerostat is numerically investigated. The numerical simulation is carried out by commercial computational fluid dynamic software with the Reynolds number from 20 to 10⁸. The average Nusselt numbers are obtained and compared with those of available in literature. Based on regression and optimization with software, a new piecewise correlation of Nusselt number is proposed. The verification shows that the new correlation is reliable.     

基于线性稳定性理论的转捩控制试验

 使用线化稳定性理论研究了某后掠机翼试验模型在风洞试验条件下可能的试验结果。在当前试验条件下,三维边界层中横流驻波的不同波长扰动发展趋势不同,根据理论分析和数值计算给出了最大放大率波长为4.0 mm。通过升华法试验验证了理论分析与数值计算结果。在试验中使用丝网印刷技术在后掠机翼前缘添加粗糙带,成功地引入了理论计算的最大放大率波长。根据预期影响了三维边界层的转捩。