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A Characterization of Thermosolutal Convection in Rivlin-Ericksen Fluid in the Presence of Magnetic Field in a Porous Medium


Affiliations
1 Department of Mathematics, Govt. College Nadaun (Hamirpur), (HP) 177033, India
     

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Thermosolutal instability of Veronis type in Rivlin-Ericksen viscoelastic fluid in the presence of uniform magnetic field in a porous medium is considered. Following the linearized stability theory and normal mode analysis, the paper mathematically established the condition for characterizing the oscillatory motions which may be neutral or unstable, for any arbitrary combination of free and rigid boundaries at the top and bottom of the fluid. It is established that all nondecaying slow motions starting from rest, magneto-thermosolutal instability of Veronis type in a Rivlin-Ericksen viscoelastic fluid of infinite horizontal extension and finite vertical depth in a porous medium, are necessarily nonoscillatory, in the regime.

Keywords

Thermosolutal Convection, Rivlin-Ericksen Fluid, Magnetic Field, PES, Rayleigh Number, Chandrasekhar Number.
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  • A Characterization of Thermosolutal Convection in Rivlin-Ericksen Fluid in the Presence of Magnetic Field in a Porous Medium

Abstract Views: 289  |  PDF Views: 1

Authors

Ajaib S. Banyal
Department of Mathematics, Govt. College Nadaun (Hamirpur), (HP) 177033, India

Abstract


Thermosolutal instability of Veronis type in Rivlin-Ericksen viscoelastic fluid in the presence of uniform magnetic field in a porous medium is considered. Following the linearized stability theory and normal mode analysis, the paper mathematically established the condition for characterizing the oscillatory motions which may be neutral or unstable, for any arbitrary combination of free and rigid boundaries at the top and bottom of the fluid. It is established that all nondecaying slow motions starting from rest, magneto-thermosolutal instability of Veronis type in a Rivlin-Ericksen viscoelastic fluid of infinite horizontal extension and finite vertical depth in a porous medium, are necessarily nonoscillatory, in the regime.

Keywords


Thermosolutal Convection, Rivlin-Ericksen Fluid, Magnetic Field, PES, Rayleigh Number, Chandrasekhar Number.