After some marginal fine-tuning of the given
ranges, a workable
definition of the Mk IV auto-folder can be given as follows:
![]() |
Figure 6: Left: PS solution; Right: Mk IV Auto-folder applied to PS sample. The vertical lines indicate the positions of the A, B, C, D and E peaks in the PS solution |
The Mk IV auto-folder strategy was based on the working hypothesis
(cf. Sect. 11.1), that significant
changes in
correlations through the hole-cutting
process are indicative of rotation curves with intrinsically noisy transition
regions.
This strategy has been manifestly so successful that its success
must be considered as very strong circumstantial evidence supporting
the view that the working hypothesis on which it is based is correct.
Thus, cross-referencing Table 1 with Fig. 6 (right),
we see that strong circumstantial evidence exists to suggest that the rotation
curves associated with the peaks C and E have intrinsically noisier
transition regions on their interiors than do those associated with the
peaks B and D.
Finally, we note from Table 1 that
the transition region behaviours of the two "quiet transition region''
peaks, B and D, are mutually distinct: specifically, for the B peak,
the coefficient of determination
changes from 20.7% to 26.3% through hole-cutting - and each of these
values signifies a very strong
correlation;
by contrast, for the D peak, the coefficient of determination changes
from 1.9% to 8.4% - the first value signifies a very weak
correlation
whilst the second signifies a moderately weak
correlation.
As we have already noted, the sample sizes are sufficiently great that
we can discount random statistical fluctuations as the source of these
differences between the B and D peak rotation curves, and so the
question arises of why strong
correlations are
present for B peak rotation curves, but are more-or-less absent
for D peak rotation curves?
Since the existence of strong correlations implies the existence of
some coherent physical process, the question becomes, why are the
correlating effects of this physical process not present for the
D peak rotation curves?
These considerations all point to the need of further research.
Copyright The European Southern Observatory (ESO)