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...
Main Authors: | , , , , |
---|---|
Format: | Article |
Language: | English |
Published: |
Elsevier
2015-12-01
|
Series: | Alexandria Engineering Journal |
Subjects: | |
Online Access: | http://www.sciencedirect.com/science/article/pii/S1110016815001386 |
id |
doaj-92a4bb3947d04182a194371d2fa64b3c |
---|---|
record_format |
Article |
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 |
work_keys_str_mv |
AT vinodkgupta chaoticconvectioninarotatingfluidlayer AT bsbhadauria chaoticconvectioninarotatingfluidlayer AT ihasim chaoticconvectioninarotatingfluidlayer AT jjawdat chaoticconvectioninarotatingfluidlayer AT aksingh chaoticconvectioninarotatingfluidlayer |
_version_ |
1721408297571975168 |