It is clear from the PCA of all the available magnetic measurements in
figure 3.10 that much of the variance is explained by
just the first two PCs. The eigenvector weightings in
figure 3.11 indicate that the first PC is a measure
of the plasma energy content (or equivalently
, the dipole
moment of the Pfirsch-Schlüter currents) and the second is
determined by the
signal ratio. We redo the
earlier regressions using just these predictors in order to demonstrate
that comparitively little information is lost.
In order to confirm that our choice of signals is favourable, we also
tabulate recovery results for a model with the largest practical
number of PCs of the individual poloidal field coil signals; it turns
out that 3 PCs can be retained. As before, we include 5%
pseudo-random measurement noise throughout.
Table 3.9 shows that despite the extra
fitted parameter of the 3 PC model over the
and
model, the results are on average slightly
inferior to the latter case. This is particularly noticeable for the
flux surface Fourier coefficients. We remark that it is more
straightforward in practice to measure the cosine moments in hardware,
since constructing them by software post-processing places higher
demands on the accuracy of the individual signal measurements. It
also requires the digitizing and storage of fewer signals and thus a
more compact diagnostic setup.
This is a good indicator that for equilibrium reconstructions based on magnetic measurements, the diagnostic setup of choice would be an array of local probe measurements, possibly with an additional diamagnetic coil to provide an independent check of the plasma energy.