The function
and
in the GS equation are free functions
which must be specified by users before solving the GS equation. Next, we
discuss one way to specify the free functions. Following Ref.
[9], we take
and
to be of the forms
 |
(441) |
 |
(442) |
with
and
chosen to be of polynomial form:
 |
(443) |
 |
(444) |
where
 |
(445) |
with
the value of
on the boundary,
the value of
on the magnetic axis,
,
,
,
,
, and
are free parameters. Using the profiles of
and
given by Eqs.
(441) and (442), we obtain
 |
(446) |
where
, and
 |
(447) |
Then the term on the r.h.s (nonlinear source term) of the GS equation is
written
 |
(448) |
The value of parameters
,
, and
in Eqs. (441) and
(442), and the value of
and
in Eqs. (443)
and (444) can be chosen arbitrarily. The parameter
is used to
set the value of the total toroidal current. The toroidal current density is
given by Eq. (62), i.e.,
 |
(449) |
which can be integrated over the poloidal cross section within the boundary
magnetic surface to give the total toroidal current,
Using
 |
(451) |
Eq. (450) is written as
![$\displaystyle I_{\phi} = \int \left[ \left( - \frac{1}{\Delta} \right) (P_0 - P...
...\frac{1}{\Delta} \hat{g}' (\overline{\Psi}) \right] \mathcal{J}d \psi d \theta,$](img1358.png) |
(452) |
from which we solve for
, giving
![$\displaystyle \gamma = \frac{- \Delta I_{\phi} - (P_0 - P_b) \int [\hat{p}' (\o...
... \frac{1}{R^2} \hat{g}' (\overline{\Psi}) \right] \mathcal{J}d \psi d \theta} .$](img1359.png) |
(453) |
If the total toroidal current
is given, Eq. (453) can be
used to determine the value of
.
yj
2018-03-09