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Astron. Astrophys. 356, 301-307 (2000)

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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 [FORMULA] and [FORMULA] along [FORMULA] and perpendicular to it. In the following calculations for the vector [FORMULA]

[EQUATION]

[EQUATION]

[EQUATION]

[EQUATION]

the terms [FORMULA], [FORMULA], [FORMULA] and [FORMULA] vanish because of the collinearity of [FORMULA] and [FORMULA] for a potential or force-free field [FORMULA], and the properties (34a,b). This yields the expressions

[EQUATION]

[EQUATION]

[EQUATION]

[EQUATION]

which do not vanish in general. Nevertheless, [FORMULA] vanishes in the particular case of a potential field [FORMULA], so that relation (A.7) becomes

[EQUATION]

This proves that [FORMULA] and [FORMULA] are both perpendicular to [FORMULA] (or [FORMULA]), but we cannot conclude they are collinear. Similar relations to (A5)-(A8) hold for [FORMULA] instead of [FORMULA].

Let us notice that Eqs. (17c,d) expressing [FORMULA] and [FORMULA] are solenoidal

[EQUATION]

imply after decomposition the relations

[EQUATION]

which actually do not inter-link the components of [FORMULA] and [FORMULA].

In conclusion, [FORMULA] and [FORMULA] should be decomposed geometrically as follows

[EQUATION]

and

[EQUATION]

[EQUATION]

wherever [FORMULA].

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© European Southern Observatory (ESO) 2000

Online publication: March 28, 2000
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