Consider the case of an intensity calibrator and perfect feeds represented by known
unitary Jones matrices
.
(This assumption is justified in
Appendix B.3.
The argument becomes slightly more complicated for
imperfect feeds, but leads to the same conclusion.) After intensity self-alignment
and imposition of our prior knowledge about the feeds, the only error remaining is
the receiver phase-difference term of Eq. (18), so the interferometer
equation becomes
The latter solution is new: in a heterogeneous array with perfectly known feeds, this knowledge alone suffices to calibrate all receiver phases without an additional measurement. In reality we may at best assume our feed descriptions to be correct on the average, just as for the homogeneous array. The solutions that we find for the individual feed characteristics as well as for the receiver phases will then be imperfect, and perhaps more sensitive to errors in our a priori assumptions and to system noise than in the homogeneous case; this is a matter that needs further study.
The possibility of a priori phase alignment is surprising at first sight. Yet there are several good intuitive reasons to accept it:
Most fundamentally, the nominal receptor characteristics in the heterogeneous case
are arbitrarily distributed. There is no natural way to split them into two disjoint
groups between which an asymmetry such as the phase difference might arise. The only
way out is for the difference not to exist.
Another viewpoint is that the homogeneous case is, in physical terms, a
degenerate one. The degeneracy results in a decoupling of the feed and phase
characteristics which are normally coupled. Mathematically, this decoupling is
represented by the product
reducing to the value
I.
A third viewpoint is that a set of identical feeds defines a preferred direction in
polvector space, viz. that of the polvectors to which the two receptors are
matched (e.g. the V axis for circular feeds). This results in an asymmetry in the
characteristics of the instrument that is directly related to the phase-difference
problem. "Randomised'' feed characteristics destroy this preferential direction: the
phase difference evaporates and all polarizations can be measured equally well, --
or equally poorly.
An array having altaz mounts is heterogeneous in a sense, since in the course of an observation its feed orientations relative to the source assume a range of values. Yet at any instant it is homogeneous and consequently its long-term heterogeneity does not help in removing the phase error and associated polrotation. As we have seen, it may help in controlling the polconversion (Sect. 7.2) when we have no intensity calibrators.
The only historical example of a truly heterogeneous array is that of the Westerbork Synthesis Radio Telescope (WSRT) in its "crossed-dipole'' configuration. Weiler (1973) analysed this system to show that, in the quasi-scalar approximation, it can be fully calibrated through observations of only one intensity calibrator. His system is too different from modern ones to relate his analysis directly to ours. Yet his work pointed to the potential of heterogeneous arrays as long as a quarter century ago and provided a major motivation for carrying the present investigation to completion.
The method of Sect. 6.3 for dealing with imperfect feeds is to assume that they are correct on the average. For a heterogeneous array, we may use the equivalent requirement that the sum of the receptor errors squared be minimised.
Following Paper I, we model the antenna Jones matrix in terms of the nominal feed
(
in Paper I), a feed error
and the receiver-gain
(a
diagonal matrix). After intensity self-alignment we then have
It may not be obvious that this condition leads to a unique solution. Simulations (Appendix D) using the MATLAB (1997) programming environment show that this is indeed the case. Moreover, the system of equations becomes singular for a homogeneous array; something of this sort was to be expected because of the degeneracy discussed in Sect. 8.1.
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