Hydromagnetic Stability of Two Rivlin-Ericksen Elastico-Viscous
Superposed Conducting Fluids
R. C. Sharma and P. Kumar
Department of Mathematics, Himachal Pradesh University, Summer Hill, Shimla-171 005, India
Z. Naturforsch. 52a, 528-532 (1997); received April 18, 1996
The stability of the plane interface separating two Rivlin-Ericksen elastico-viscous superposed
fluids of uniform densities when the whole system is immersed in a uniform horizontal magnetic field
has been studied. The stability analysis has been carried out, for mathematical simplicity, for two
highly viscous fluids of equal kinematic viscosities and equal kinematic viscoelasticities. It is found
that the stability criterion is independent of the effects of viscosity and viscoelasticity and is
dependent on the orientation and magnitude of the magnetic field. The magnetic field is found to
stabilize a certain wave-number range of the unstable configuration. The behaviour of growth rates
with respect to kinematic viscosity and kinematic viscoelasticity parameters are examined numeri-
cally.
1. Introduction
The instability of the plane interface separating two
Newtonian fluids when one is accelerated towards the
other or when one is superposed over the other has
been studied by several authors, and Chandrasekhar
[1] has given a detailed account of these investigations.
Roberts [2] has extended the analysis to the case of two
fluids of equal kinematic viscosities in presence of a
vertical magnetic field, while Gerwin [3] has studied
the case of compressible streaming fluids. The influ-
ence of viscosity on the stability of the plane interface
separating two incompressible superposed fluids of
uniform densities, when the whole system is immersed
in a uniform horizontal magnetic field has been stud-
ied by Bhatia [4]. He has carried out the stability
analysis for two fluids of equal kinematic viscosities
and different uniform densities. A good account of
hydrodynamic stability problems has also been given
by Drazin and Reid [5] and Joseph [6].
The fluids have been considered to be Newtonian in
all the above studies. The stability of a layer of vis-
coelastic (Oldroyd) fluid heated from below and sub-
ject to a magnetic field has been studied by Sharma [7],
In another study Sharma and Sharma [8] have studied
the stability of the plane interface separating two vis-
coelastic (Oldroyd) superposed fluids of uniform den-
sities. Fredricksen [9] has given a good review of non-
Newtonian fluids whereas Joseph [6] has also
considered the stability of viscoelastic fluids. Molten
Reprint requests to Prof. R. C. Sharma.
plastics, petroleum oil additives and whipped cream
are examples of incompressible viscoelastic fluids.
There are many non-Newtonian fluids that cannot be
characterized by Oldroyd's [10] constitutive relations.
The Rivlin-Ericksen elastico-viscous fluid is one such
fluid. It is this class of elastico-viscous fluids we are
interested in particularly to study the stability of the
plane interface separating two incrompressible super-
posed Rivlin-Ericksen fluids of uniform densities per-
vaded by a uniform horizontal magnetic field in addi-
tion to a constant gravity field. This aspect forms the
subject of the present paper where we have carried out
the stability analysis for two fluids of equal kinematic
viscosities, equal kinematic viscoelasticities and differ-
ent densities.
2. Perturbation Equations
Consider a static state, in which an incompressible,
infinitely conducting, Rivlin-Ericksen elastico-viscous
fluid of variable density pervaded by a uniform mag-
netic field H(H
X
,H
Y
, 0) is arranged in horizontal
strata and the pressure p and density q are functions
of the vertical coordinate z only. The character of the
equilibrium of this initial static state is determined, as
usual, by supposing that the system is slightly dis-
turbed and then by following its further evolution.
Let q(u, v, w), öq, öp and h(h
x
,h
y
,h
:
) denote the
perturbations in velocity (0, 0, 0), density g, pressure p
and magnetic field H, respectively. Then the linearized
hydromagnetic perturbation equations relevant to the
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