Next we consider the radial component of the momentum equation. Taking scalar
product of the momentum equation with
, we obtain
 |
(106) |
After some algebra (the details are given in Sec. (9.5)), Eq.
(106) is written
where
 |
(108) |
and
is the
magnetic field curvature with
the unit vector
along equilibrium magnetic field. Equation (107) agrees with Eq.
(17) in Cheng's paper[3]. In passing, let us examine the
physical meaning of
defined by (108). In linear approximation,
we have
This indicates the perturbation in the square of the magnetic strength is
. Therefore, the perturbation in magnetic
pressure is written
 |
(110) |
which indicate
defined by Eq. (108) is the total perturbation
in the thermal and magnetic pressure.
yj
2015-09-04