Astron. Astrophys. 356, 301-307 (2000)
Appendix A: components of b and j with respect to B0
Let us prove that there is generally no simple relation between the
components of and
along
and perpendicular to it. In the
following calculations for the vector
![[EQUATION]](img185.gif)
![[EQUATION]](img186.gif)
![[EQUATION]](img187.gif)
![[EQUATION]](img188.gif)
the terms ,
,
and vanish because of the
collinearity of and
for a potential or force-free field
, and the properties (34a,b). This
yields the expressions
![[EQUATION]](img192.gif)
![[EQUATION]](img193.gif)
![[EQUATION]](img194.gif)
![[EQUATION]](img195.gif)
which do not vanish in general. Nevertheless,
vanishes in the particular case of
a potential field , so that relation
(A.7) becomes
![[EQUATION]](img197.gif)
This proves that and
are both perpendicular to
(or
), but we cannot conclude they are
collinear. Similar relations to (A5)-(A8) hold for
instead of
.
Let us notice that Eqs. (17c,d) expressing
and
are solenoidal
![[EQUATION]](img200.gif)
imply after decomposition the relations
![[EQUATION]](img201.gif)
which actually do not inter-link the components of
and
.
In conclusion, and
should be decomposed
geometrically as follows
![[EQUATION]](img202.gif)
and
![[EQUATION]](img203.gif)
![[EQUATION]](img204.gif)
wherever .
© European Southern Observatory (ESO) 2000
Online publication: March 28, 2000
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