Determination of Electron Flows
Making use of Equations (2.169), (2.177), (2.196), and (2.203), we obtain
|
(2.233) |
It follows from Equations (2.183) and (2.233) that
However,
because
, for , and
. Hence, we
get
|
|
(2.235) |
where use has been made of Equation (2.214). It follows that
|
(2.236) |
where
Making use of Equations (2.197), (2.198), and (2.216), and only retaining terms up to first order in the
small parameter , we get
where
Here use has been made of Equations (2.209)–(2.211), (2.217), and (2.218).
It follows from Equations (2.165), (2.166), (2.170), (2.181)–(2.185), (2.236), and (2.240)–(2.242) that
and
Here, we have made use of the fact that
.
In the circular magnetic flux-surface limit, Equations (2.255) and (2.256) reduce
to
whereas
Equations (2.257)–(2.258) yield
Expressions (2.259)–(2.262) have many features in common with the corresponding expressions, (2.226)–(2.229), for the ions, despite being much more complicated in nature. In particular, the
E-cross-B velocity makes no contribution to the poloidal component of the electron fluid velocity. Moreover, the
poloidal component of the electron fluid velocity is similar in magnitude to a diamagnetic velocity, whereas the
parallel component is larger by a factor
.