The effect of temperature-dependent viscosity and thermal conductivity on the onset of compressible convection

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2020-06-22 DOI:10.1080/03091929.2020.1777549
Abrar A. Ali, L. Silvers
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Abstract

The linear equations of thermal convection in a compressible fluid with non-constant transport coefficients are derived. The criterion for the onset of convection is established, based on linear stability analysis, for a range of different temperature-dependent profiles of thermal conductivity and viscosity. Temperature-dependent transport coefficients are shown to lead to a more complex behaviour than their constant counterparts, and modifies the stability condition of the fluid. When the Rayleigh number is defined in terms of the mid-layer physical properties and the temperature gradient at the top is held constant, increasing the temperature-dependence of thermal conductivity is found to raise the critical Rayleigh number dramatically, as the convective disturbance is then concentrated mainly at the top of the layer. In contrast, for viscosity a more subtle effect on stability is identified.
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随温度变化的粘度和热导率对可压缩对流发生的影响
导出了非恒定输运系数的可压缩流体中热对流的线性方程。在线性稳定性分析的基础上,建立了对流开始的准则,适用于一系列不同的温度依赖的导热系数和粘度剖面。温度相关的输运系数比恒定的输运系数导致更复杂的行为,并改变流体的稳定性条件。当用中间层物理性质来定义瑞利数,并保持顶部温度梯度不变时,增加导热系数的温度依赖性会显著提高临界瑞利数,因为此时对流扰动主要集中在顶层。相比之下,粘度对稳定性的影响更为微妙。
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来源期刊
Geophysical and Astrophysical Fluid Dynamics
Geophysical and Astrophysical Fluid Dynamics 地学天文-地球化学与地球物理
CiteScore
3.10
自引率
0.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: Geophysical and Astrophysical Fluid Dynamics exists for the publication of original research papers and short communications, occasional survey articles and conference reports on the fluid mechanics of the earth and planets, including oceans, atmospheres and interiors, and the fluid mechanics of the sun, stars and other astrophysical objects. In addition, their magnetohydrodynamic behaviours are investigated. Experimental, theoretical and numerical studies of rotating, stratified and convecting fluids of general interest to geophysicists and astrophysicists appear. Properly interpreted observational results are also published.
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