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Regenerative Orr mechanism yielding large non-modal perturbation energy growth in a viscosity stratified plane shear flow 在粘度分层平面剪切流中产生大量非模态扰动能量增长的再生奥尔机制
IF 3.6 2区 工程技术 Q1 MECHANICS Pub Date : 2024-09-16 DOI: 10.1016/j.ijmultiphaseflow.2024.105001
Sharath Jose

Transiently growing non-modal perturbations can play a crucial role in the transition of plane shear flows in modally stable regimes. In terms of the extent of transient amplification, three-dimensional perturbations are typically more prominent due to the lift-up effect. In contrast, two-dimensional (2D) spanwise-independent perturbations are often considered less important as they typically undergo modest levels of transient growth and are short-lived. The Orr mechanism is key to the amplification of energy for 2D perturbations. In this work, we discuss 2D non-modal perturbations of three-layer viscosity stratified flows with the mean shear rates of the outer layers being equal. Strikingly, a novel regenerative Orr mechanism is found that allows for significant amount of energy amplification despite the 2D nature of the perturbations. Moreover, these perturbations survive for considerably long times. The perturbation structure shows symmetry about the middle layer and evolves such that the Orr mechanism can repeatedly occur in a regenerative manner resulting in the perturbation energy evolving in a markedly non-monotonic fashion. When these same perturbations are introduced in a uniform plane shear flow, the corresponding non-modal transient amplifications are shown to be much smaller.

瞬时增长的非模态扰动对平面剪切流向模态稳定区的过渡起着至关重要的作用。就瞬态放大的程度而言,由于抬升效应,三维扰动通常更为突出。相比之下,与跨度无关的二维(2D)扰动通常被认为不那么重要,因为它们的瞬态增长水平一般不高,而且持续时间很短。奥尔机制是二维扰动能量放大的关键。在这项工作中,我们讨论了外层平均剪切速率相等的三层粘性分层流的二维非模态扰动。令人震惊的是,我们发现了一种新颖的再生奥尔机制,尽管扰动具有二维性质,但仍能实现大量的能量放大。此外,这些扰动还能持续相当长的时间。扰动结构显示出关于中间层的对称性,并不断演化,从而使奥尔机制能够以再生方式反复发生,导致扰动能量以明显的非单调方式演化。当在均匀平面剪切流中引入这些相同的扰动时,相应的非模态瞬态放大效应要小得多。
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引用次数: 0
Molecular dynamics study of the mechanism of explosive boiling on hybrid wettability surfaces 混合润湿表面爆炸沸腾机理的分子动力学研究
IF 3.6 2区 工程技术 Q1 MECHANICS Pub Date : 2024-09-16 DOI: 10.1016/j.ijmultiphaseflow.2024.105002
Hongren Zhan, Dongling Liu, Baichen Ji, Debin Liu, Zhigang Zhang, Xianzhen Zhang

In this work, molecular dynamics (MD) simulation is applied to study the effect of heating surfaces with different hydrophobicity occupancy ratios (the ratio of the surface area of hydrophobic spots to the total area of the heating surface) on the boiling process of the liquid film explosion. At the same time, the mechanism is revealed from the trajectory of argon atoms. The simulation results showed that the onset of explosive boiling was later for purely hydrophilic surfaces than for hybrid wettability surfaces with a hydrophobicity percentage of <11%. The earliest onset of explosive boiling was observed for the heated surfaces with a hydrophobicity ratio of 6%. In addition, it was found that the superheat required for explosive boiling tended to decrease first and then increase with the gradual increase of the hydrophobicity ratio. Hydrophobic spots arranged on the surface provided bubble nucleation earlier for explosive boiling while enhancing convective heat transfer and thermal perturbation. The critical heat flux (CHF) of the heated surfaces with a hydrophobicity ratio of <11% were all greater than that of the purely hydrophilic surfaces, and all reached the CHF before the purely hydrophilic surfaces.

本研究应用分子动力学(MD)模拟研究了不同疏水占据比(疏水点表面积与加热表面总面积之比)的加热表面对液膜爆炸沸腾过程的影响。同时,从氩原子的运动轨迹揭示了其机理。模拟结果表明,纯亲水表面的爆炸沸腾开始时间晚于疏水性百分比为 11% 的混合润湿表面。疏水性比例为 6% 的受热表面最早出现爆沸现象。此外,研究还发现,随着疏水性比率的逐渐增加,爆炸沸腾所需的过热度呈先降低后升高的趋势。表面上的疏水点为爆炸沸腾提供了更早的气泡成核,同时增强了对流传热和热扰动。疏水比为 11% 的受热表面的临界热通量 (CHF) 均大于纯亲水表面,且均先于纯亲水表面达到临界热通量。
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引用次数: 0
Experimental investigation on pressure drop characteristics of adiabatic two-phase flow in a Gyroid-structured channel 陀螺结构通道中绝热两相流压降特性的实验研究
IF 3.6 2区 工程技术 Q1 MECHANICS Pub Date : 2024-09-13 DOI: 10.1016/j.ijmultiphaseflow.2024.104982
Tomoki Hirokawa, Hajime Miyata
Recent advancements in additive manufacturing techniques have enabled the fabrication of intricate structures. Among these structures, triply periodic minimal surfaces (TPMSs) such as the gyroid, are particularly promising for heat and mass transfer applications owing to their higher surface area to volume ratios compared to conventional structures such as heat exchangers. This study experimentally investigates the pressure drop characteristics of single- and two-phase flows in a gyroid-structured channel under adiabatic conditions. In particular, using an additively manufactured test section with a gyroid-structured channel, the pressure drop characteristics of both single- and two-phase flows are analyzed. The results ofsingle-phase flow experiments reveal that the friction factor depends on the hydraulic diameter, which is defined by the internal volume and surface area of the channel. This suggests that in addition to the hydraulic diameter, other parameters such as porosity and wall thickness must also be considered. Subsequently, the two-phase pressure drop predictions of homogeneous and separated models are compared with the pressure drop data obtained from two-phase flow experiments. The results reveal that gas–liquid separation must be considered to accurately predict the pressure drop in regions influenced by gravitational effects. Furthermore, correlations for predicting the pressure drops both single- and two-phase flows within the operating constraints are proposed.
增材制造技术的最新进展使得复杂结构的制造成为可能。与热交换器等传统结构相比,三周期极小表面(TPMS)具有更高的表面积与体积比,因此在传热和传质应用中特别有前景。本研究通过实验研究了绝热条件下陀螺结构通道中单相流和两相流的压降特性。特别是,利用带有陀螺结构通道的快速成型试验段,分析了单相流和两相流的压降特性。单相流实验结果表明,摩擦因数取决于水力直径,而水力直径是由通道的内部容积和表面积决定的。这表明,除了水力直径外,还必须考虑其他参数,如孔隙率和壁厚。随后,将均相模型和分离模型的两相压降预测结果与两相流实验获得的压降数据进行了比较。结果表明,要准确预测受重力影响区域的压降,必须考虑气液分离。此外,还提出了在运行限制条件下预测单相流和两相流压力降的相关性。
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引用次数: 0
Modelling aerodynamic forces and torques of spheroid particles in compressible flows 球形颗粒在可压缩气流中的空气动力和扭矩建模
IF 3.6 2区 工程技术 Q1 MECHANICS Pub Date : 2024-09-12 DOI: 10.1016/j.ijmultiphaseflow.2024.104996
Yibin Du , Ming Yu , Chongwen Jiang , Xianxu Yuan

In the present study, we conduct numerical simulations of compressible flows around spheroid particles, for the purpose of refining empirical formulas for drag force, lift force, and pitching torque acting on them. Through an analysis of approximately a thousand numerical simulation cases spanning a wide range of Mach numbers, Reynolds numbers and particle aspect ratios, we first identify the crucial parameters that are strongly correlated with the forces and torques via Spearman correlation analysis, based on which the empirical formulas for the drag force, lift force and pitching torque coefficients are refined. The novel formulas developed for compressible flows exhibit consistency with their incompressible counterparts at low Mach number limits and, moreover, yield accurate predictions with average relative errors of less than 5%. This underscores their robustness and reliability in predicting aerodynamic loads on spheroidal particles under various flow conditions.

在本研究中,我们对球形颗粒周围的可压缩流进行了数值模拟,目的是完善作用在颗粒上的阻力、升力和俯仰力矩的经验公式。通过对跨越各种马赫数、雷诺数和颗粒长宽比的近千个数值模拟案例进行分析,我们首先通过斯皮尔曼相关性分析确定了与力和力矩密切相关的关键参数,并在此基础上完善了阻力、升力和俯仰力矩系数的经验公式。为可压缩流开发的新公式在低马赫数限制条件下与不可压缩流的公式一致,而且预测准确,平均相对误差小于 5%。这突出表明,在预测球形颗粒在各种流动条件下的空气动力载荷时,这些公式非常稳健可靠。
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引用次数: 0
Understanding solid particle transport in a gas cyclone separator 了解气体旋风分离器中的固体颗粒传输
IF 3.6 2区 工程技术 Q1 MECHANICS Pub Date : 2024-09-12 DOI: 10.1016/j.ijmultiphaseflow.2024.104992
M. Sommerfeld, M.A. Taborda
A cyclone separator is a widespread device used in many industrial areas and daily life for removing fine particulate matter from a gas stream. This separator has been used for more than 100 years due to its simple and robust design, but was continuously further developed and adapted to specific applications. The mostly used configuration is the reverse flow type cyclone exhibiting however, a very complex vortex flow with high turbulence. In the past numerous experimental as well as numerical studies were conducted for optimising cyclone geometry with the goal of improving the separation efficiency. In most of the numerical studies done so far not all the relevant transport mechanisms affecting particle motion were considered. Therefore, a thorough numerical investigation is presented using an LES-point-particle-Euler/Lagrange approach with momentum 2-way coupling for analysing the effects of particle-scale transport processes on the performance of a 290 mm Stairmand type of cyclone. All simulations presented here were conducted for an inlet velocity of 10 m/s. The sub-grid-scale (SGS) turbulence was described by a dynamic Smagorinsky model. Particle transport was computed considering all relevant forces and modelling also SGS dispersion. For the first time, the influence of particle collisions with rough walls, modelled according to the stochastic approach presented by Sommerfeld and Huber (International Journal of Multiphase Flow, Vol. 25, 1457-1489, 1999), was analysed in detail with respect to the performance of a cyclone separator. Moreover, inter-particle collisions were described through the efficient stochastic model introduced by Sommerfeld (International Journal of Multiphase Flow, Vol. 27, 1828-1858, 2001). Specifically, the importance of the interplay between rough wall collisions and inter-particle collisions is highlighted in this contribution. Three different particle size spectra were considered with log-normal size distributions ranging up to 20 μm (mean diameter 5.21 μm), up to 60 μm (mean diameter 15.43 μm), and up to 100 μm (mean diameter 25.71 μm); each case with different mass loading. Naturally, due to their different inertia, the effects of wall collisions and inter-particle collisions are also different for these types of particles. After a thorough validation, the influences of two-way coupling, particle rough wall collisions (three surface roughness degrees) and inter-particle collisions are analysed and elucidated. It is shown that specifically surface roughness has a huge effect on the grade efficiency of a cyclone and cannot be neglected, as done in most numerical cyclone studies done so far. Inter-particle collisions may partly compensate the deterioration of separation by wall roughness.
旋风分离器是一种广泛应用于许多工业领域和日常生活中的设备,用于去除气流中的微粒物质。这种分离器因其设计简单、坚固耐用,已使用了 100 多年,但仍在不断改进,以适应特定的应用。最常用的配置是反向流型旋风分离器,但这种旋风分离器会产生非常复杂的高湍流涡流。过去,为了优化旋流器的几何形状,进行了大量的实验和数值研究,目的是提高分离效率。在迄今为止进行的大多数数值研究中,并没有考虑到影响颗粒运动的所有相关传输机制。因此,本文采用具有动量双向耦合的 LES-点-颗粒-Euler/Lagrange 方法进行了全面的数值研究,以分析颗粒尺度传输过程对 290 毫米 Stairmand 型旋风分离器性能的影响。本文介绍的所有模拟都是在入口速度为 10 米/秒的条件下进行的。亚网格尺度(SGS)湍流由动态 Smagorinsky 模型描述。计算粒子传输时考虑了所有相关的作用力,并对 SGS 扩散进行了建模。根据 Sommerfeld 和 Huber(《国际多相流杂志》,第 25 卷,1457-1489 年,1999 年)提出的随机方法建模,首次详细分析了颗粒与粗糙壁碰撞对旋风分离器性能的影响。此外,还通过 Sommerfeld(《国际多相流杂志》,第 27 卷,1828-1858 年,2001 年)引入的高效随机模型对粒子间碰撞进行了描述。具体而言,粗糙壁面碰撞和粒子间碰撞之间的相互作用在本文中得到了强调。我们考虑了三种不同的粒度谱,其对数正态粒度分布范围分别为 20 μm(平均直径 5.21 μm)、60 μm(平均直径 15.43 μm)和 100 μm(平均直径 25.71 μm);每种情况下的质量负荷都不同。当然,由于惯性不同,壁面碰撞和颗粒间碰撞对这些类型颗粒的影响也不同。经过全面验证后,分析并阐明了双向耦合、颗粒粗糙壁面碰撞(三种表面粗糙度)和颗粒间碰撞的影响。结果表明,具体来说,表面粗糙度对旋风分离器的分级效率有很大影响,不能像迄今为止的大多数旋风分离器数值研究那样被忽视。颗粒间的碰撞可以部分弥补壁面粗糙度对分离效果的影响。
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引用次数: 0
Trigger mechanism for a singing cavitating tip vortex 用于歌唱空化尖端涡流的触发机制
IF 3.6 2区 工程技术 Q1 MECHANICS Pub Date : 2024-09-11 DOI: 10.1016/j.ijmultiphaseflow.2024.104995
Zhaohui Qian , Yongshun Zeng , Xiaoxing Peng , Xianwu Luo

The discrete tone radiated from tip vortex cavitation (TVC), known as ‘vortex singing’, was recognized in 1989, but its triggering remains unclear for over thirty years. In this study, the desinent cavitation number and viscous correction are applied to describe the dynamics of cavitation bubbles and the dispersion relation of cavity interfacial waves. The wavenumber-frequency spectrum of the cavity radius from the experiment in CSSRC indicates that singing waves predominantly consist of the stationary double helical modes (kθ = 2- and -2+) and the breathing mode (kθ = 0-), rather than standing waves as assumed in previous literatures. Moreover, two trigger mechanisms, expressed by two triggering lines, are proposed: the twisted TVC, initially at rest, is driven into motion through the corrected natural frequency (fn) due to the step change of the far-field pressure. Subsequently, the frequency associated with the zero-group-velocity point (zgv) at kθ = 0- is excited through i, the frequency at the intersection of dispersion curves at kθ = 0- and -2+, or j, the frequency at the intersection of dispersion curves at kθ = 0- and 2-, corresponding to two types of the vortex singing triggering. These solutions, without empirical parameters, are validated using singing conditions provided by CSSRC and G.T.H., respectively. Furthermore, the coherence and the cross-power spectral density spectrum indicates a large-scale breathing wave propagating along the singing cavity surface and travelling from downstream to hydrofoil tip, providing us a comprehensive understanding for the triggering of vortex singing.

1989 年,人们认识到了由尖端涡旋空化(TVC)辐射出的离散音调,这种音调被称为 "涡旋歌唱",但三十多年来,其触发原因仍不清楚。在这项研究中,应用了 Desinent 空化数和粘性修正来描述空化气泡的动力学和空腔界面波的弥散关系。来自 CSSRC 实验的空腔半径的波数-频率谱表明,歌唱波主要由静止的双螺旋模式(kθ = 2- 和 -2+)和呼吸模式(kθ = 0-)组成,而不是之前文献中假设的驻波。此外,还提出了由两条触发线表示的两种触发机制:扭曲的 TVC 最初处于静止状态,由于远场压力的阶跃变化,通过校正固有频率(fn)被驱动运动。随后,与 kθ = 0- 处的零组速度点 (ῶzgv)相关的频率通过 kθ = 0- 和 -2+ 处频散曲线交点的频率ῶi 或 kθ = 0- 和 2- 处频散曲线交点的频率ῶj 被激发,对应于两种类型的涡唱触发。这些不含经验参数的解分别利用 CSSRC 和 G.T.H. 提供的歌唱条件进行了验证。此外,相干性和交叉功率谱密度频谱表明有一个大尺度呼吸波沿歌唱腔表面传播,并从下游向水翼顶端传播,这为我们全面理解涡旋歌唱的触发提供了依据。
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引用次数: 0
The GFMxP and the basic extrapolation of the ghost values to solve the Poisson equation for discontinuous functions 用 GFMxP 和鬼影值的基本外推法求解不连续函数的泊松方程
IF 3.6 2区 工程技术 Q1 MECHANICS Pub Date : 2024-09-10 DOI: 10.1016/j.ijmultiphaseflow.2024.104997
Sandro Ianniello

In a recent paper, a novel coding of the Ghost Fluid Method for the variable coefficient Poisson equation with discontinuous functions (named GFMxP) was proposed. A lot of numerical tests, with all the required quantities available in a analytic form, were used to demonstrate the ability of the new procedure in modeling a sharp interface and to check the accuracy order of the solutions. In practical applications, however, the real difficulty stands in the estimation of the so-called “ghost values”, that is the values at points where the function is not only unknown, but even not defined. These values allow to compute the corrective terms enabling the use of standard finite difference formulas in presence of a singularity and/or a discontinuity, and can be only determined through some extrapolation procedure, whose truthfulness is essential to achieve a reliable result. The paper deals with such a basic issue, by testing different numerical strategies and demonstrating the strict relationship between the order of the adopted fit-model, the order of the solving scheme for the Poisson equation and the accuracy of the final solution.

在最近的一篇论文中,针对具有不连续函数的变系数泊松方程,提出了一种新颖的幽灵流体法编码(名为 GFMxP)。通过大量的数值测试(所有需要的量都可以用解析形式表示),证明了新程序在模拟尖锐界面和检查解的精度阶次方面的能力。然而,在实际应用中,真正的困难在于估算所谓的 "幽灵值",即函数不仅未知,甚至没有定义的点上的值。这些值可以计算校正项,从而在出现奇异点和/或不连续性时使用标准有限差分公式,并且只能通过一些外推法程序来确定,而外推法程序的真实性对于获得可靠的结果至关重要。本文通过测试不同的数值策略来解决这一基本问题,并证明了所采用的拟合模型阶数、泊松方程求解方案阶数和最终求解精度之间的严格关系。
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引用次数: 0
Description of phase separation motion in gas‒liquid two-phase flow 气液两相流中的相分离运动描述
IF 3.6 2区 工程技术 Q1 MECHANICS Pub Date : 2024-09-10 DOI: 10.1016/j.ijmultiphaseflow.2024.104998
Xitong Wu, Chenhao Li, Xingqi Luo, Jianjun Feng, Like Wang

Understanding the physics of phase separation between gas and liquid phases as a mixture mass has long been a challenge. In this paper, a phase separation description criterion based on heterogeneous flow model is proposed. A mathematical method similar to Lagrangian coherent structure (LCS) is used to identify the two-phase separation process, which is called relative motion Lagrangian coherent structure (rLCS). The rLCS is able to describe the dynamic evolution of the phase separation process and flow pattern transition in multiphase flows, which is very common in gas‒liquid mixture transportation and industrial processes. The most striking finding of rLCS is that phase separation and phase distribution are not in the same spatial position, that is, the process and the result of separation may not be exactly corresponding as we thought. This new flow structure reflects the underlying dynamic behavior of the multiphase flow field. In addition, the phase separation process has obvious periodicity. This paper reveals the typical phase separation process in the simulation of gas‒liquid two-phase pipe flow and gas‒liquid multiphase pump. These are very important to improve the understanding of multiphase flow processes, and can also lay a solid foundation for future flow control based on multiphase flow characteristics, highlighting the application potential of the new method.

长期以来,理解作为混合物质的气相和液相之间的相分离物理学一直是一项挑战。本文提出了一种基于异相流模型的相分离描述标准。本文采用了一种类似于拉格朗日相干结构(LCS)的数学方法来识别两相分离过程,这种方法被称为相对运动拉格朗日相干结构(rLCS)。相对运动拉格朗日相干结构(rLCS)能够描述多相流中相分离过程的动态演化和流动模式的转变,这在气液混合物运输和工业过程中非常常见。rLCS 最引人注目的发现是,相分离和相分布并不在同一空间位置,也就是说,分离过程和分离结果可能并不像我们想象的那样完全对应。这种新的流动结构反映了多相流场的基本动态行为。此外,相分离过程具有明显的周期性。本文揭示了气液两相管道流动和气液多相泵模拟中典型的相分离过程。这些对于提高人们对多相流过程的认识非常重要,也能为未来基于多相流特性的流量控制打下坚实基础,凸显了新方法的应用潜力。
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引用次数: 0
Experimental investigation and modelling of hydrodynamics and heat transfer in flow boiling in normal and microgravity conditions 正常和微重力条件下流动沸腾的流体力学和传热的实验研究与建模
IF 3.6 2区 工程技术 Q1 MECHANICS Pub Date : 2024-09-07 DOI: 10.1016/j.ijmultiphaseflow.2024.104991
Paul Onubi Ayegba, Julien Sebilleau, Catherine Colin
<div><p>The development of long-term space thermal management systems has informed research into the influence of gravity on boiling. This work explored the influence of gravity on the hydrodynamics and heat transfer of boiling flow. Experiments were carried out using two test loops each consisting of a 6 mmID transparent cylindrical test section. Upward (<span><math><mrow><mo>+</mo><mn>1</mn><mi>░</mi><mi>g</mi></mrow></math></span>) and downward (<span><math><mrow><mo>−</mo><mn>1</mn><mi>░</mi><mi>g</mi></mrow></math></span>) flow boiling experiments were carried out in the laboratory while microgravity (<span><math><mrow><mi>μ</mi><mi>g</mi></mrow></math></span>) experiments were carried out during a parabolic flight campaign. The results of flow visualisation showed significant influence of gravity on the flow patterns and the influence of gravity was generally limited to mass flux, <span><math><mrow><mi>G</mi><mo>≤</mo><mn>400</mn><mspace></mspace><mi>k</mi><mi>g</mi><mo>/</mo><msup><mrow><mi>m</mi></mrow><mn>2</mn></msup><mi>s</mi></mrow></math></span> and/or vapor quality, <span><math><mrow><mi>x</mi><mo>≤</mo><mn>0.35</mn></mrow></math></span>. In all three gravity conditions, the measured heat transfer coefficient was influenced by heat flux, mass flux and/or vapor quality. For liquid Reynolds number, <span><math><mrow><mi>R</mi><msub><mi>e</mi><mrow><mi>l</mi><mi>o</mi></mrow></msub><mo>≤</mo><mn>2000</mn><mspace></mspace><mrow><mo>(</mo><mrow><mi>G</mi><mo>≤</mo><mn>150</mn><mspace></mspace><mi>k</mi><mi>g</mi><mo>/</mo><msup><mrow><mi>m</mi></mrow><mn>2</mn></msup><mi>s</mi></mrow><mo>)</mo></mrow></mrow></math></span> and boiling number <span><math><mrow><mi>B</mi><mi>o</mi><mo><</mo><mn>0.002</mn></mrow></math></span> the measured heat transfer coefficient was highest in <span><math><mrow><mo>−</mo><mn>1</mn><mi>g</mi></mrow></math></span> flow and lowest in <span><math><mrow><mi>μ</mi><mi>g</mi></mrow></math></span> flow but becomes comparable at <span><math><mrow><mi>B</mi><mi>o</mi><mo>></mo><mn>0.002</mn></mrow></math></span>. A correlation for predicting microgravity heat transfer coefficient was proposed in this work and the proposed correlation predicted 100 % of the <span><math><mrow><mi>μ</mi><mi>g</mi></mrow></math></span> data in the current work within <span><math><mrow><mo>±</mo><mn>20</mn><mo>%</mo></mrow></math></span>, predicted nearly 100 % of the <span><math><mrow><mi>μ</mi><mi>g</mi></mrow></math></span> data of <span><span>Ohta et al. (2013)</span></span> within <span><math><mrow><mo>±</mo><mn>30</mn><mo>%</mo></mrow></math></span> and around 85 % of the <span><math><mrow><mi>μ</mi><mi>g</mi></mrow></math></span> data of <span><span>Narcy (2014)</span></span> within -20 % to +50 %. A correlation for predicting the gravity dependent regime as it relates to heat transfer coefficient in <span><math><mrow><mo>+</mo><mn>1</mn><mi>g</mi></mrow></math></span> and <span><math><mrow><mi>μ</mi><mi>g</mi></mrow></math
长期太空热管理系统的开发为研究重力对沸腾的影响提供了依据。这项研究探讨了重力对沸腾流的流体力学和传热的影响。实验使用两个测试环进行,每个测试环由一个 6 mmID 的透明圆柱测试部分组成。向上(+1░g)和向下(-1░g)流动沸腾实验在实验室进行,而微重力(μg)实验则在抛物线飞行活动中进行。流动可视化结果表明,重力对流动模式有显著影响,而且重力的影响一般仅限于质量通量 G≤400kg/m2s 和/或蒸汽质量 x≤0.35。在所有三种重力条件下,测得的传热系数都受到热通量、质量通量和/或蒸汽质量的影响。对于液体雷诺数 Relo≤2000(G≤150kg/m2s)和沸腾数 Bo<0.002,测量到的传热系数在 -1g 流量下最高,在 μg 流量下最低,但在 Bo>0.002 时变得相当。在这项工作中提出了一种预测微重力传热系数的相关方法,所提出的相关方法对当前工作中的μg数据的预测在±20%以内,对Ohta等人(2013年)的μg数据的预测在±30%以内,对Narcy(2014年)的μg数据的预测在-20%至+50%以内,对Narcy(2014年)的μg数据的预测在-20%至+50%以内。在这项工作中,还提出了一种预测重力依赖机制的相关方法,因为它与 +1g 和 μg 流量中的传热系数有关。在目前的工作和 Lebon 等人(2019 年)、Narcy(2014 年)、Ohta 等人(2013 年)的工作中,所提出的标准正确预测了超过 85% 的重力相关传热系数。
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Upward (&lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mo&gt;+&lt;/mo&gt;&lt;mn&gt;1&lt;/mn&gt;&lt;mi&gt;░&lt;/mi&gt;&lt;mi&gt;g&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt;) and downward (&lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mo&gt;−&lt;/mo&gt;&lt;mn&gt;1&lt;/mn&gt;&lt;mi&gt;░&lt;/mi&gt;&lt;mi&gt;g&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt;) flow boiling experiments were carried out in the laboratory while microgravity (&lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;μ&lt;/mi&gt;&lt;mi&gt;g&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt;) experiments were carried out during a parabolic flight campaign. The results of flow visualisation showed significant influence of gravity on the flow patterns and the influence of gravity was generally limited to mass flux, &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;G&lt;/mi&gt;&lt;mo&gt;≤&lt;/mo&gt;&lt;mn&gt;400&lt;/mn&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mi&gt;k&lt;/mi&gt;&lt;mi&gt;g&lt;/mi&gt;&lt;mo&gt;/&lt;/mo&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mi&gt;m&lt;/mi&gt;&lt;/mrow&gt;&lt;mn&gt;2&lt;/mn&gt;&lt;/msup&gt;&lt;mi&gt;s&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; and/or vapor quality, &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;x&lt;/mi&gt;&lt;mo&gt;≤&lt;/mo&gt;&lt;mn&gt;0.35&lt;/mn&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt;. In all three gravity conditions, the measured heat transfer coefficient was influenced by heat flux, mass flux and/or vapor quality. For liquid Reynolds number, &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;R&lt;/mi&gt;&lt;msub&gt;&lt;mi&gt;e&lt;/mi&gt;&lt;mrow&gt;&lt;mi&gt;l&lt;/mi&gt;&lt;mi&gt;o&lt;/mi&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;mo&gt;≤&lt;/mo&gt;&lt;mn&gt;2000&lt;/mn&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mrow&gt;&lt;mo&gt;(&lt;/mo&gt;&lt;mrow&gt;&lt;mi&gt;G&lt;/mi&gt;&lt;mo&gt;≤&lt;/mo&gt;&lt;mn&gt;150&lt;/mn&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mi&gt;k&lt;/mi&gt;&lt;mi&gt;g&lt;/mi&gt;&lt;mo&gt;/&lt;/mo&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mi&gt;m&lt;/mi&gt;&lt;/mrow&gt;&lt;mn&gt;2&lt;/mn&gt;&lt;/msup&gt;&lt;mi&gt;s&lt;/mi&gt;&lt;/mrow&gt;&lt;mo&gt;)&lt;/mo&gt;&lt;/mrow&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; and boiling number &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;B&lt;/mi&gt;&lt;mi&gt;o&lt;/mi&gt;&lt;mo&gt;&lt;&lt;/mo&gt;&lt;mn&gt;0.002&lt;/mn&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; the measured heat transfer coefficient was highest in &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mo&gt;−&lt;/mo&gt;&lt;mn&gt;1&lt;/mn&gt;&lt;mi&gt;g&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; flow and lowest in &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;μ&lt;/mi&gt;&lt;mi&gt;g&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; flow but becomes comparable at &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;B&lt;/mi&gt;&lt;mi&gt;o&lt;/mi&gt;&lt;mo&gt;&gt;&lt;/mo&gt;&lt;mn&gt;0.002&lt;/mn&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt;. A correlation for predicting microgravity heat transfer coefficient was proposed in this work and the proposed correlation predicted 100 % of the &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;μ&lt;/mi&gt;&lt;mi&gt;g&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; data in the current work within &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mo&gt;±&lt;/mo&gt;&lt;mn&gt;20&lt;/mn&gt;&lt;mo&gt;%&lt;/mo&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt;, predicted nearly 100 % of the &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;μ&lt;/mi&gt;&lt;mi&gt;g&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; data of &lt;span&gt;&lt;span&gt;Ohta et al. (2013)&lt;/span&gt;&lt;/span&gt; within &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mo&gt;±&lt;/mo&gt;&lt;mn&gt;30&lt;/mn&gt;&lt;mo&gt;%&lt;/mo&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; and around 85 % of the &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;μ&lt;/mi&gt;&lt;mi&gt;g&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; data of &lt;span&gt;&lt;span&gt;Narcy (2014)&lt;/span&gt;&lt;/span&gt; within -20 % to +50 %. A correlation for predicting the gravity dependent regime as it relates to heat transfer coefficient in &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mo&gt;+&lt;/mo&gt;&lt;mn&gt;1&lt;/mn&gt;&lt;mi&gt;g&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; and &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;μ&lt;/mi&gt;&lt;mi&gt;g&lt;/mi&gt;&lt;/mrow&gt;&lt;/math","PeriodicalId":339,"journal":{"name":"International Journal of Multiphase Flow","volume":"181 ","pages":"Article 104991"},"PeriodicalIF":3.6,"publicationDate":"2024-09-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S0301932224002684/pdfft?md5=495272ac2b385d10ddf92c05eb0a8c29&pid=1-s2.0-S0301932224002684-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142168361","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"工程技术","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Universal law for identifying the singing vortex 识别歌唱旋涡的普遍规律
IF 3.6 2区 工程技术 Q1 MECHANICS Pub Date : 2024-09-06 DOI: 10.1016/j.ijmultiphaseflow.2024.104993
Zhaohui Qian , Huan Han , Yongshun Zeng , Xiaoxing Peng , Xianwu Luo

The discrete tone radiated from a cavitating tip vortex, named as ‘vortex singing’, has remained a mystery for over thirty years. In this study, based on the dispersion relation of cavity interfacial waves, the vortex singing is proved to be generated by breathing mode waves propagating from downstream to the hydrofoil tip, solely determined by the mean cavity radius (rc), the cavitation number (σ) and the desinent cavitation number (σd). Then we have identified three types of vortex singing, the universal law, such as the dimensionless singing frequency for each type ( = 2πfrc/U = 0.312, 0.037 and 0.926, f is frequency and U denotes the incoming velocity) and the wavenumber for one typical type (κ = 2πrc /λ = 0.361, λ represents the wavelength) have been first derived and validated. Furthermore, the minimum cavitation number and desinent cavitation number required for detecting each type of vortex singing are given theoretically. Importantly, we have illustrated a long-standing perplexity: why such a whistler can appear only within a narrow range of frequency, wavelength as well as the cavitation number.

空化尖端涡旋辐射出的离散音被命名为 "涡旋歌唱",三十多年来一直是个谜。在这项研究中,根据空腔界面波的频散关系,证明了涡唱是由从下游向水翼顶端传播的呼吸模态波产生的,完全由平均空腔半径(rc)、空化数(σ)和去空化数(σd)决定。然后,我们确定了三种类型的涡旋歌唱,首次推导并验证了普遍规律,如每种类型的无量纲歌唱频率(ῶ = 2πfrc/U∞ = 0.312、0.037 和 0.926,f 为频率,U∞ 表示传入速度)和一种典型类型的波长(κ = 2πrc /λ = 0.361,λ 表示波长)。此外,我们还从理论上给出了检测每种涡唱类型所需的最小空化数和大空化数。重要的是,我们说明了一个长期存在的困惑:为什么这种啸声只能出现在频率、波长和空化数的狭窄范围内。
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引用次数: 0
期刊
International Journal of Multiphase Flow
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