Reusing the analysis of Sections 5.7–5.9, let us again suppose that there are two layers in
space (i.e., Fourier space). The
small-
layer turns out to be of width
, where
 |
(6.4) |
Here,
is the hydromagnetic timescale defined in Equation (5.43). Given that we are effectively assuming that
, the condition for the separation of the layer solution into two layers (i.e., that the width of the small-
layer is less than that of the large-
layer) is always satisfied. The large-
layer is governed by the equation
 |
(6.5) |
where
Here,
is the normalized diamagnetic frequency [see Equation (5.65)],
and
are magnetic Prandtl numbers [see Equations (5.53) and (5.54)], and
is the ratio of the electron
to the ion pressure gradient at the rational surface [see Equation (4.5)].
The boundary conditions on Equation (6.5) are
that
is bounded as
, and
![$\displaystyle Y_e(p)= Y_0\left[1-\frac{\skew{6}\hat{\mit\Delta}\,p}{\pi\,\hat{\gamma}} + {\cal O}(p^2)\right]$](img2373.png) |
(6.8) |
as
. Here,
is an arbitrary constant.
In the various constant-
linear growth-rate regimes considered in the next section, Equation (6.5) reduces to an equation of the form
 |
(6.9) |
where
is real and non-negative, and
is a complex constant. As described in Section 5.8, the solution of this
equation that is bounded as
can be matched to the small-
asymptotic form (6.8) to give
 |
(6.10) |
where
. The width of the large-
layer in
space is
.