Very little polarized flux is either predicted or observed to come from the inner region, and no polarized emission is detected from the inner counter-jet. For this reason, the field ratios are essentially unconstrained there (Table 7).
The toroidal field component is the largest over most of the flaring and
outer regions, increasing from 0.6 to
0.9 of the total
between the inner boundary and the end of the modelled region
(Fig. 21). The longitudinal component, conversely, decreases
from
0.7 to
0.4 over the same distance. We found no
evidence for any variation of the longitudinal/toroidal field ratio across
the shear layer. The component ratios for the spine are not well
determined (Table 7) and could quite plausibly be identical to
those for the shear layer.
![]() |
Close to the edge of the jet in the flaring region, the radial component
becomes appreciable, reaching a maximum of 0.6 at the edge on the
outer boundary (marked by the arrows in Fig. 21).
Thereafter, it decreases rapidly with distance along the jet, becoming
negligible by 9.5 kpc from the nucleus in the SSL model. The radial
component, unlike the other two, increases with radius
(Fig. 21). As mentioned earlier, this variation is required
in order to achieve even a qualitative fit to the observed polarization in
the flaring region.