The mechanism of the instability is kinematic: pressure gradient variations, leading to velocity variations, develop along the interface as a result of the perturbation to the interface.
We consider flow through a porous medium and choose a co-ordinate system in which x is directed vertically upwards in the direction of the base state fluid flow at velocity V, and y and z lie in a horizontal plane.
On length scales larger than the pores of the medium, flow through a porous medium is described by Darcy's law:
(where
is velocity, k is permeability of the porous
medium,
is dynamic viscosity, p is pressure,
is density, g is gravitational constant, and
is the velocity
potential). Hence the pressure
p is harmonic.
Laplace's equation must be solved for the pressure p in two media, each with different permeability, viscosity and density, subject to two boundary conditions:
To examine stability, the interface in the base state is taken to be
x=0 (note that this is in a co-ordinate frame moving upwards at
velocity V) and a small time-dependent perturbation
is added, where
is an arbitrary small
constant, n is an arbitrary integer and the sign of
denotes
stability (if negative) or instability (if positive).
The velocity potential gradients on x=0 equal the velocity of the interface and are given by
The velocity potential functions are harmonic functions subject to the
above boundary condition (
) at the interface and such the
the effects of the interface perturbation decay at large distances
from the interface.
Neglecting surface tension effects, Saffman and Taylor found the
solutions
(
) and equating the pressures on the interface
showed that the stability condition is as follows: when fluid 2 is
forced upwards towards fluid 1 such that the undisturbed interface
at x = 0 is traveling at velocity V, the interface is stable if
and unstable if the reverse inequality holds (for all wavelengths n). Hence the effect of the more viscous fluid lying above the less viscous fluid when the lower fluid is forced upwards is destabilizing and vice versa; similarly, the effect of the more dense fluid lying above the less dense fluid is destabilizing and vice versa (as in the Rayleigh-Taylor instability). Note that when the fluid is forced at a large velocity V, gravitational effects are negligible.