Few projections astrotomography: radio astronomical approach to 3D reconstruction

摘要

We develop a radio astronomical approach to 3D-reconstruction in few projections tomography. It is based on the 2-CLEAN DSA method which consists of two clean algorithms by using a synthesized beam. In complex cases two extreme solutions are used for the analysis of the image structure. These solutions determine the limits of permissible energy redistribution on the image among the components of small and large scales. Two variants of 3D-reconstruction proceeding from a set of two-dimensional projections (3D_(2D)) and from a set of one-dimensional ones (3D_(1D)) are considered. It is shown that the quality of 3D_(2D)-reconstruction should be similar to the quality of 2D_(1D)-reconstruction if the same number of equally spaced scans is used. But a doubled number of projections is required for 3D_(1D)-reconstruction. We have simulated 3D-reconstruction of an optically thin emitting object. The present technique is a component of astrotomography and it has good prospects for a wide range of remote sensing.