共查询到20条相似文献,搜索用时 93 毫秒
1.
氦加热器是预冷组合发动机中重要的换热器之一,其原理是利用燃气燃烧的热量提高氦气做功能力,进而提升整个循环系统运行效率。研究中首先设计了蛇形管式、瓦片式、辐射式三种微细通道氦加热器。其次,基于FLUENT15.0软件对微细通道氦加热器管内外的对流换热系数和流动阻力进行了研究。对比模拟结果和经典关联式的计算结果,确定了适用于微细通道氦加热器管内外换热和流阻的关联式。结果表明:对于管内流动换热,经典关联式预测准确,平均误差小于8%。对于管外流动换热,经典关联式对流阻的预测依然准确,但是对换热系数的预测有较大偏差,最大偏差接近50%。基于数值模拟结果拟合了新的微细通道氦加热器管外对流换热关联式,平均误差小于5%。此外,对比分析发现蛇形管式微细通道氦加热器对流换热系数最大,综合性能最优。 相似文献
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I. A. Babushkin G. P. Bogatyrev A. F. Glukhov G. F. Putin S. V. Avdeev A. I. Ivanov M. M. Maksimova 《Cosmic Research》2001,39(2):150-158
The DACON instrument for studying the convection caused by low frequency microaccelerations aboard spacecraft is described. The convection sensor serves as a measuring element of this instrument. This is a cylindrical cavity filled with air, where two crossed differential thermocouples are located. The thermocouple junctions lay on two mutually perpendicular lines parallel to the bases of the cylinder and crossing at its axis. The distances from the junctions to this axis are equal. The lateral surface of the cylinder is thermally insulated, the difference of temperatures on its bases being kept constant. One of the tasks for the sensor is to prepare the data for checking the adequacy of mathematical models of fluid convection under weightlessness conditions and for obtaining quantitative characteristics of the microgravitational medium. The results of ground-based tests of the DACON instrument and the results of experiments with it aboard the Mirstation are presented. 相似文献
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Weak concentration convection which arises in the process of diffusion of impurities into the solvent filling a gap between two coaxial cylinders is studied experimentally. It is found that convective motion in the range of Grashof numbers 103–5 × 104 has a clear boundary-layer character. Near the inner porous cylinder, which is a source of impurity, a diffusion boundary layer passing into a two-dimensional convective plume is formed. The data on the structure and thickness of this layer are presented depending on the integral flux of impurity. The prospects of making an experiment in order to discover concentration convection onboard an orbital station are discussed. 相似文献
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综合考虑太阳辐射、长波辐射、对流换热等热环境因素对临近空间飞艇热特性的影响,建立飞艇热特性的数学模型,编写程序并计算得到蒙皮表面温度分布。以此作为热边界条件,采用Fluent软件模拟其内部自然对流的流动状态和温度分布,对不同季节不同时刻飞艇内部自然对流换热系数进行了计算分析,并对四个自然对流经验公式进行了评价分析。结果表明,Eckert-Jackson和Bayley公式更适用于计算浮空器内部自然对流换热,与数值模拟结果相比,平均绝对误差(MAD)分别为22.6%和24.1%。 相似文献
5.
V型皱褶芯材夹层结构与强迫对流冷却相结合,可应用于高超声速飞行器或大功率电子器件承载和散热的多功能设计。文章采用数值仿真方法对强迫对流条件下V型皱褶芯材夹层结构的换热及其产生的热应力进行研究,获得了相应的速度场、温度场及结构热应力分布。结果表明:强迫对流条件下,V型皱褶芯材夹层结构的换热性能明显提高,同时导致较大的压力损失。流体速度场随着几何构型的改变而发生周期性的变化,在结构偏折处波峰一侧流速达到最大,对流换热得到增强;沿着冷却液流动方向,结构与冷却液的温度逐渐升高,并伴随着周期性的波动;皱褶芯材夹层结构的整体换热能力随着入口流速的增大而增强。热流输入侧的面板热应力和变形均较大,结构皱褶部位存在应力集中。 相似文献
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Heat transfer of thermocapillary convection in a two-layered fluid system under the influence of magnetic field 总被引:1,自引:0,他引:1
Daniele Ludovisi Soyoung S. Cha Narayanan Ramachandran William M. Worek 《Acta Astronautica》2009,64(11-12):1066-1079
Heat transfer of a two-layer fluid system has been of great importance in a variety of industrial applications. For example, the phenomena of immiscible fluids can be found in materials processing and heat exchangers. Typically in solidification from a melt, the convective motion is the dominant factor that affects the uniformity of material properties. In the layered flow, thermocapillary forces can come into an important play, which was first emphasized by a previous investigator in 1958. Under extraterrestrial environments without gravity, thermocapillary effects can be a more dominant factor, which alters material properties in processing. Control and optimization of heat transfer in an immiscible fluid system need complete understanding of the flow phenomena that can be induced by surface tension at a fluid interface. The present work is focused on understanding of the magnetic field effects on thermocapillary convection, in order to optimize material processing. That is, it involves the study of the complicated phenomena to alter the flow motion in crystal growth. In this effort, the Marangoni convection in a cavity with differentially heated sidewalls is investigated with and without the influence of a magnetic field. As a first step, numerical analyzes are performed, by thoroughly investigating influences of all pertinent physical parameters. Experiments are then conducted, with preliminary results, for comparison with the numerical analyzes. 相似文献
7.
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。 相似文献
8.
诱导轮是现代液体火箭发动机中提高涡轮泵性能的关键部件,它可以在局部发生汽蚀的情况下工作,但是汽蚀所诱发的各种非定常不稳定现象会影响火箭发动机涡轮泵的性能、稳定性和寿命.本文利用基于Rayleigh-Plesset方程的混合流体模型,对诱导轮二维叶栅中的汽蚀不稳定现象进行了数值分析.结果表明,在一定汽蚀数范围内诱导轮容易... 相似文献
9.
The problem of stabilization of a rotating spacecraft with a flexible spike antenna located along the axis of spacecraft rotation is considered. A magnetohydrodynamic element is used as a final-control element in the control loop of spacecraft attitude, and the solar direction sensor serves as a measuring device. At the first stage of investigation, the problem of stability is considered for stationary and non-stationary modes of rotation of the spacecraft with a flexible antenna and with a cavity partially filled with a low-viscosity liquid. 相似文献
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M.N. Smirnova A.V. Zvyaguin I.V. Shugan Ray-Yeng Yang Hwung-Hweng Hwung 《Acta Astronautica》2011,68(1-2):46-51
The two-dimensional problem of high velocity moving slender body interaction with fluid free surface was regarded. Gravity was neglected as compared with fluid inertia. The problem is relevant to underwater motion of a bullet or shell, which could take place in orbital collisions of particles with fluid-filled containments. The problem is also relevant to evaluating wave-breakers effect on the streaming flow. The solution was obtained for the case of final length cavity formation behind the body. The solution allows determining free surface shape, drag and lift forces. In the limiting cases of relatively small depth or high compressibility, the obtained solution permitted analytical approximation. 相似文献
12.
L. V. Dokuchaev 《Cosmic Research》2002,40(1):37-47
The influence of dissipative forces in a viscous liquid that completely fills the cavities of a space object executing a rotational motion is analyzed. The Navier–Stokes equations are solved by expanding them into a series in terms of eigenfunctions of the boundary value problem on involving the resting liquid in rotation around the longitudinal axis of a cavity. The analytical solutions for coaxial cylindrical and concentric spherical cavities are obtained, in particular, for a straight circular cylinder and a sphere. The stability of the single-axis orientation of a space object filled with a viscous liquid is investigated. The dependences of rotation decay processes and drifts of the space object's longitudinal axis from a given direction are shown on the plane of constructive parameters. 相似文献
13.
L.M.B.C. Campos 《Acta Astronautica》2009,64(9-10):969-978
An analytical model of the aerothermodynamics of fluid–structure interaction through an ablative wall is developed, involving: (i) the solution to the Navier–Stokes equations in the fluid; (ii) the solution to the equations of thermoelasticity in the solid wall; (iii) the matching of the two solutions across the fluid–wall interface by continuity of normal and tangential stresses and jump of the heat flux equal to the heat of ablation. These three matching conditions determine the three constants of integration, besides the boundary conditions: (i) in the free stream far above the wall, the fluid velocity and temperature are given; (ii) in the backing material below the wall the temperature is given and displacement is assumed to be zero. In order to arrive at a simple analytical solution the simplest geometry is chosen: two-dimensional, with a flat fluid–wall interface, and all quantities in the fluid and structure depending only on distance from the wall. Extensions to unsteady and three-dimensional cases would be more complex. The present theory specifies: (i) the velocity, pressure and density in the fluid; (ii) the displacement vector, and strain and stress tensors in the structure; (iii) the temperature and heat flux in the fluid and structure, including discontinuities across the fluid–wall interface. The model is applied to examples of (a) hypersonic flight and (b) atmospheric re-entry. 相似文献
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航天器密封舱在地面模拟试验中常通过降压法抑制自然对流的影响,但降压比的选择 往往缺乏定量准则,这使得自然对流的抑制效果得不到保证。使用数值模拟方法确定临 界压力比,以几种典型航天器密封舱内的流动换热情况为例,分析了不同Gr/Re 2 数和压力比下密封舱内的流动换热情况。得到了舱内气体温度分布和对流换热系数。通 过比较空间情况和地面情况的计算结果,分析了自然对流给流动换热带来的影响,给出了判 断临界压力的准则式,并给出了临界Gr/Re 2数。结果表明:临界压力 的准则关系和密封舱的形状和内部结构无关。
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17.
We have reconstructed the uncontrolled rotational motion of the Progress M-29M transport cargo spacecraft in the single-axis solar orientation mode (the so-called sunward spin) and in the mode of the gravitational orientation of a rotating satellite. The modes were implemented on April 3–7, 2016 as a part of preparation for experiments with the DAKON convection sensor onboard the Progress spacecraft. The reconstruction was performed by integral statistical techniques using the measurements of the spacecraft’s angular velocity and electric current from its solar arrays. The measurement data obtained in a certain time interval have been jointly processed using the least-squares method by integrating the equations of the spacecraft’s motion relative to the center of mass. As a result of processing, the initial conditions of motion and parameters of the mathematical model have been estimated. The motion in the sunward spin mode is the rotation of the spacecraft with an angular velocity of 2.2 deg/s about the normal to the plane of solar arrays; the normal is oriented toward the Sun or forms a small angle with this direction. The duration of the mode is several orbit passes. The reconstruction has been performed over time intervals of up to 1 h. As a result, the actual rotational motion of the spacecraft relative to the Earth–Sun direction was obtained. In the gravitational orientation mode, the spacecraft was rotated about its longitudinal axis with an angular velocity of 0.1–0.2 deg/s; the longitudinal axis executed small oscillated relative to the local vertical. The reconstruction of motion relative to the orbital coordinate system was performed in time intervals of up to 7 h using only the angularvelocity measurements. The measurements of the electric current from solar arrays were used for verification. 相似文献
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In oceanographics situations where salt fingers may be an important mechanism for the transport of heat and salt in the vertical direction, velocity shears may also be present. Salt finger convection is analogous to Bénard convection in that the kinetic energy of the motions is obtained from the potential energy stored in the unstable distribution of a stratifying component. On the basis of the thermal analogy it is of interest to discover whether salt fingers are converted into two-dimensional sheets by wind shear, and how the vertical fluxes of heat and salt are changed by wind shear. Salt finger convection under the effect of steady wind shear is theoretically examined in this paper. The evolution of instability developing in the presence of a vertical density gradient disturbance and the horizontal Couette flow is considered near the onset of salt fingers under a moderate rate of shear. We use velocity as the basic variable and solve the pressure Poisson equation in terms of the associated Green function. Growth competition between the longitudinal rolls (LR) and the transverse rolls (TR), whose axes are, respectively, in the direction parallel to and perpendicular to the Couette flow, is investigated by the weakly nonlinear analysis of coupled-mode equations. The results show that the TR mode is stable under a small wind shear and the LR mode is stable for a higher wind shear. 相似文献
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局部多孔壁-内腔结构的气动加热瞬态特性 总被引:4,自引:0,他引:4
根据超声速飞行器外表面连接结构处密封结构几何特征,以局部多孔壁和内腔结构为研究对象,建立流/固/多孔区域流动和传热过程耦合计算模型,其中多孔区域中运用分布阻力法,流、固区域间换热过程采用准稳态耦合计算方法。经过与相关实验数据进行对比,验证了程序可靠性,并进一步分析在整个长时间瞬态过程中,该密封结构的流动和传热特征,阐明了在瞬态过程中多孔材料等效热流对缝隙壁面的加热作用。研究了有、无多孔材料填充两种情况下缝隙壁面热流分布形态的差异,探讨了缝隙中填充多孔材料对高速流场边界层热气流侵入内腔过程的影响。
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