164 CHAPT ER 3. THEORY OF MAGNETIC SEPARATION
flocculation of weakly magnetic particles and wet high-gradient magnetic sep-
aration have received considerable theoretical attention. A notable number of
papers dealing with the problem of particle capture in HGMS led to an under-
standing of the interaction between a particle and a matrix element. However,
completely general treatment of the magnetostatic and hydrodynamic behav-
iour of an assembly of the ore particles in a system of matrix elements, in the
presence of a strong magnetic field, is a theoretical problem of considerable
complexity.
A brief survey of the current theoretical descriptions of separation of ma-
terials in various types of magnetic separation equipment will be given in the
following sections.
3.1 The forces and the equations of particle mo-
tion
The equations of particle motion are relations between accelerations, velocities
and coordinates of the particles. They are second-order dierential equations
for the function u(w)> where u is the radius vector and w is the time. Their
integration makes possible, in principle, the determination of this function and
so of the path of the particles.
The equation of particle motion in a magnetic separator can be written in a
vector form as
p
s
d
s
=
l
I
l
(3.1)
where p
s
d
s
is the inertial force, p
s
is the mass of the particle and d
s
its
acceleration. I
l
are all the forces that may be present in a magnetic separator,
such as the magnetic force, force of gravity, hydrodynamic drag, centrifugal
force, the friction force, surface forces, magnetic dipolar forces and electrostatic
forces among the particles and others. In order to be able to solve eq. (3.1), it
is necessary to evaluate the components of all its terms in suitable coordinates.
To obtain the components of the inertial force in polar coordinates that are
convenient for most types of magnetic separators, let us consider two mutually
perpendicular unit vectors ˆu and
ˆ
= We shall assume that these vectors have
directions of increasing u and and their directions change with time. Since
the derivative of a unit vector is perpendicular to the vector, the time rates of
ˆu and
ˆ
can be expressed as [G1]
gˆu
gw
=
g
gw
ˆ
(3.2)
g
ˆ
gw
=
g
gw
ˆu (3.3)
Now, the position of the particle, in polar coordinates, is given by u = uˆu.
Dierentiating this equation and using eqs. (3.2) and (3.3), the components of