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Let
,
,
be standard spherical coordinates. Consider axisymmetric Stokes flow such that
 |
(10.84) |
According to Equations (A.175) and (A.176), we can automatically satisfy the incompressibility constraint (10.80) by writing (see Section 7.4)
 |
(10.85) |
where
is the Stokes stream function (i.e.,
). It follows that
Moreover, according to Section C.4,
, and
 |
(10.88) |
where (see Section 7.4)
 |
(10.89) |
Hence, given that
, we can write
  |
(10.90) |
It follows from Equations (A.176) and (A.178) that
Thus, by analogy with Equations (10.85) and (10.90), and making use of Equations (A.173) and (A.177),
we obtain
Equation (10.83) implies that
 |
(10.93) |
which is the governing equation for axisymmetric Stokes flow.
In addition, Equations (10.82) and (10.91) yield
![$\displaystyle \nabla P = \mu\,\nabla\varphi\times \nabla[{\cal L}(\psi)].$](img3745.png) |
(10.94) |
Next: Axisymmetric Stokes Flow Around
Up: Incompressible Viscous Flow
Previous: Stokes Flow
Richard Fitzpatrick
2016-03-31