Laboratory measurements of super-resolving Toraldo pupils for radio astronomical applications

TL;DR

This paper reports laboratory microwave measurements of Toraldo Pupils, demonstrating their potential for super-resolution in radio astronomy and validating previous experimental results through extensive testing and simulations.

Contribution

It provides a comprehensive analysis of Toraldo Pupils for radio astronomical super-resolution, including experimental validation and electromagnetic simulations.

Findings

Microwave measurements confirm super-resolution capabilities of TPs.

Different geometrical shapes of TPs were tested successfully.

Simulations and near-field scans support experimental results.

Abstract

The concept of super-resolution refers to various methods for improving the angular resolution of an optical imaging system beyond the classical diffraction limit. Although several techniques to narrow the central lobe of the illumination Point Spread Function have been developed in optical microscopy, most of these methods cannot be implemented on astronomical telescopes. A possible exception is represented by the variable transmittance filters, also known as "Toraldo Pupils" (TPs) since they were introduced for the first time by G. Toraldo di Francia in 1952. In the microwave range, the first successful laboratory test of TPs was performed in 2003. These first results suggested that TPs could represent a viable approach to achieve super-resolution in Radio Astronomy. We have therefore started a project devoted to a more exhaustive analysis of TPs and how they could be implemented on a radio telescope. In the present work we report on the results of extensive microwave measurements, using TPs with different geometrical shapes, which confirm the correctness of the first experiments in 2003. We have also extended the original investigation to carry out full-wave electromagnetic numerical simulations and also to perform planar scanning of the near-field and transform the results into the far-field.