For sources with circular symmetry it may be necessary to obtain the
variation of amplitude with antenna spacing, in order to compare the
amplitude data with models. For this purpose, with task UV_CIRCLE one takes the mean of all the visibilities in
concentric rings in the uv plane. The output has the format of a
uv table (except that all v's are zero), and may be plotted with
UVALL (fig. 12.5).
Use this sort of averaging with caution: the phase center must accurately coincide with the source position or the amplitude of the visibility average will decrease on long spacings (use UV_FIT and UV_SHIFT. One may also do this kind of averaging in separate sectors in the uv plane, to check for asymmetries, provided the uv plane is well sampled (task UV_CUTS).