Chaotic convection in a rotating fluid layer

A study of thermal convection in a rotating fluid layer is investigated based on the dynamical systems approach. A system of differential equation like Lorenz model has been obtained by using Galerkin-truncated approximation. The chaotic convection is investigated in a rotating fluid layer. A low-di...

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Main Authors: Vinod K. Gupta, B.S. Bhadauria, I. Hasim, J. Jawdat, A.K. Singh
Format: Article
Language:English
Published: Elsevier 2015-12-01
Series:Alexandria Engineering Journal
Subjects:
Online Access:http://www.sciencedirect.com/science/article/pii/S1110016815001386
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spelling doaj-92a4bb3947d04182a194371d2fa64b3c2021-06-02T04:59:43ZengElsevierAlexandria Engineering Journal1110-01682015-12-0154498199210.1016/j.aej.2015.09.002Chaotic convection in a rotating fluid layerVinod K. Gupta0B.S. Bhadauria1I. Hasim2J. Jawdat3A.K. Singh4Department of Mathematics, Banaras Hindu University, Varanasi, IndiaDepartment of Mathematics, Banaras Hindu University, Varanasi, IndiaUniversiti of Kebansberg, MalaysiaUniversiti of Kebansberg, MalaysiaDepartment of Mathematics, Banaras Hindu University, Varanasi, IndiaA study of thermal convection in a rotating fluid layer is investigated based on the dynamical systems approach. A system of differential equation like Lorenz model has been obtained by using Galerkin-truncated approximation. The chaotic convection is investigated in a rotating fluid layer. A low-dimensional, Lorenz-like model was obtained using Galerkin truncated approximation. The fourth-order Runge–Kutta method is employed to obtain the numerical solution of Lorenz-like system of equations. We found that there is proportional relation between Taylor number and the scaled Rayleigh number R. This means that chaotic behavior can be delayed (for increasing value of R) when we increase the scaled Taylor number. We conclude that the transition from steady convection to chaos depends on the level of Taylor number.http://www.sciencedirect.com/science/article/pii/S1110016815001386Chaotic behaviorRotationLorenz-equationFluid layer
collection DOAJ
language English
format Article
sources DOAJ
author Vinod K. Gupta
B.S. Bhadauria
I. Hasim
J. Jawdat
A.K. Singh
spellingShingle Vinod K. Gupta
B.S. Bhadauria
I. Hasim
J. Jawdat
A.K. Singh
Chaotic convection in a rotating fluid layer
Alexandria Engineering Journal
Chaotic behavior
Rotation
Lorenz-equation
Fluid layer
author_facet Vinod K. Gupta
B.S. Bhadauria
I. Hasim
J. Jawdat
A.K. Singh
author_sort Vinod K. Gupta
title Chaotic convection in a rotating fluid layer
title_short Chaotic convection in a rotating fluid layer
title_full Chaotic convection in a rotating fluid layer
title_fullStr Chaotic convection in a rotating fluid layer
title_full_unstemmed Chaotic convection in a rotating fluid layer
title_sort chaotic convection in a rotating fluid layer
publisher Elsevier
series Alexandria Engineering Journal
issn 1110-0168
publishDate 2015-12-01
description A study of thermal convection in a rotating fluid layer is investigated based on the dynamical systems approach. A system of differential equation like Lorenz model has been obtained by using Galerkin-truncated approximation. The chaotic convection is investigated in a rotating fluid layer. A low-dimensional, Lorenz-like model was obtained using Galerkin truncated approximation. The fourth-order Runge–Kutta method is employed to obtain the numerical solution of Lorenz-like system of equations. We found that there is proportional relation between Taylor number and the scaled Rayleigh number R. This means that chaotic behavior can be delayed (for increasing value of R) when we increase the scaled Taylor number. We conclude that the transition from steady convection to chaos depends on the level of Taylor number.
topic Chaotic behavior
Rotation
Lorenz-equation
Fluid layer
url http://www.sciencedirect.com/science/article/pii/S1110016815001386
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