Glasser-Greene-Johnson Parameters
It is convenient to add to this appendix a generalized calculation of the magnetic curvature length,
, that appears in the Rutherford island width evolution
equation, (12.15).
Let
,
, and
.
Furthermore, let
 |
 |
(A.89) |
 |
 |
(A.90) |
 |
 |
(A.91) |
 |
 |
(A.92) |
 |
 |
(A.93) |
 |
 |
(A.94) |
It follows that [6]
where
, and
is the equilibrium plasma pressure.
Finally,
 |
(A.98) |
The value of the dimensionless parameter
at a given rational magnetic flux-surface is related to the magnetic curvature length,
, introduced in Section 11.4, according to
 |
(A.99) |
Here,
is a dimensionless measure of the plasma pressure at the rational surface [see Equations (4.65) and (4.66)],
the magnetic shear-length at the rational surface [see Equation (5.27)], and
the effective pressure gradient scale-length at the rational surface [see Equation (8.35)]. The previous equation is a generalization of Equation (11.57).
The latter equation only holds in a large-aspect ratio, low-
, tokamak plasma with magnetic flux-surfaces of circular cross-section.