飞机整体油箱三维瞬态温度场分析

介绍了飞机整体油箱三维瞬态温度场分析方法。利用MSC.Patran/Nastran thermal 2001软件,建立了飞机整体油箱三维瞬态温度场分析有限元模型。模拟了发动机表面与油箱底部的面—面辐射,油箱顶部对外部空间的热辐射,以及进气道冷空气与油箱底部之间对流换热等多种复杂边界条件。在软件不具备单元死活功能的条件下,成功模拟了飞行过程中燃油的消耗。本文的研究结果对飞行器油箱部件的热分析具有一定借鉴意义。     

用湍流传热模型模拟室内空气流动和换热

利用低雷诺数NH模型、NK传热模型及模型系数改进后的NK传热模型,分别对室内空气流动和换热的速度场、温度场、湍动能场进行了模拟,并将计算结果与实验结果进行了对比分析.研究表明,低雷诺数NH模型、NK传热模型及模型系数改进后的NK传热模型均能对室内空气流动及换热的速度场、温度场、湍动能场进行较好的数值模拟,其中模型系数改进后的NK传热模型模拟的准确性最高.     

冲击＋同向对流＋气膜冷却的三维壁温计算与分析

采用Fluent 6.3软件对冲击＋同向对流＋气膜冷却结构的壁温进行了流固耦合传热计算,获得了该复合冷却结构的壁温和冷却效果分布规律,并将计算结果与试验结果进行了对比.结果表明：冲击＋同向对流＋气膜冷却具有壁温分布均匀、冷却效果好等优点.计算结果与试验结果的分布趋势一致,最大相对误差为3.6%.     

高空飞行环境中液体运载火箭底部热环境研究

采用数值模拟和飞行测试验证相结合的方法对液体运载火箭高空对流/辐射耦合换热问题开展系统深入研究。基于燃气多组分输运Navier-Stokes方程、热辐射方程、Realizable k-ε两方程湍流模型,建立了高空含自由流的运载火箭燃气喷流流动模型。辐射模型采用离散坐标法(DOM),空间离散采用二阶迎风TVD格式,对多个典型飞行高度火箭底部热流进行大型并行计算,将数值结果与试验数据进行广泛对比,验证了计算模型的精度和有效性。数值研究表明,火箭底部辐射热流在刚起飞阶段达到最大值,随着飞行高度上升,辐射热流逐渐降低,火箭底部对流热流表现为先升高后降低的趋势,并在20 km高空达到峰值。本文的预测分析方法对液体运载火箭底部热防护设计具有重要的理论意义和工程应用价值。     

横越两圆柱体的传热特性

用数值方法求解绕过两圆柱的对流传热问题。贝克列数在０－５０的范围内，了四种不同间距时的传热情况。从中发现两圆柱的传热特性相互有影响，这种影响随意距变化很敏感，两圆柱中任一个的平均谢尔特数总是小于单个圆柱的。并给出了简化计算的条件与公式。     

Atmospheric response to a Hot SST Event in November 2006 as observed by the AIRS instrument

Using Atmospheric Infrared Sounder (AIRS) products of atmospheric temperature and geopotential height, we investigate the atmospheric response to HE0611, which was found and investigated by [Qin, H., Kawamura, H., Sakaida, F., Ando, K. A case study of the tropical Hot Event in November 2006 (HE0611) using a geostationary meteorological satellite and the TAO/TRITON mooring array. J. Geophys. Res. 113, C08045, doi: 10.1029/2007JC004640, 2008]. HE0611 was formed by connecting two very high SST areas, HE0611-East and HE0611-West. The period-mean atmosphere temperatures at levels of 925 and 850 hPa in HE0611-West are higher, by about 0.5 K, than those in WE0611-East while the atmospheric temperatures at middle to high levels (700–300 hPa) are higher in HE0611-East. The period-mean geopotential heights HE0611-East are much lower than those in HE0611-West for the levels from the surface to 400 hPa. The mean geopotential heights from 400 hPa to 200 hPa are higher in HE0611-East. In the middle and high layers over HE0611-West, the atmosphere temperatures gradually decrease from 7th to 17th, and then increase significantly. The increase in HE0611-East starts from 15th November, which is earlier than that of HE0611-West. The geopotential heights in the high layer of both the areas also show corresponding behaviors. The lagged atmospheric response in the western part is confirmed by the correlation analysis. It emerges that the atmospheric response to HE0611 is well organized and associated with deep convention in HE0611-East and subsidence in HE0611-West. These are also consistent with the HE0611 features and evolution revealed by earlier HE studies.     

重力仪散热装置的热仿真分析

随着移动平台重力测量精度的不断提高,对重力仪的温度控制提出了更高的要求。为了实现在不同温度环境下的高精度重力测量,本文设计了一种保温散热装置,为重力仪提供第一级温控。利用Fluent软件分别模拟了0℃,22℃和40℃环境温度下此装置内重力仪系统的温度场,并在此基础上,利用高低温箱完成该装置的温度性能实验,验证了此温控方案的可行性。     

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。      

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.