The resulting normalized aperture field distributions from the recorded primary radiation patterns of various feed horns are examined and simulated by equivalent mathematical functions such as

and

, where

and

are constants. Convenient methods are worked out for the computation of the different secondary far field radiation pattern parameters for circularly symmetric equiphase distributions in terms of

or

. Computed and experimental data for beamwidth, efficiency, first and second side lobes, and aperture blocking effects are plotted and compared as a function of p. The resulting secondary patterns due to aperture field distribution

are computed and presented in graph form for comparison.