Visibility Interpolation in Solar Hard X-ray Imaging: Application to RHESSI and STIX

TL;DR

This paper introduces a novel visibility interpolation method using Variably Scaled Kernels for improved solar hard X-ray image reconstruction from Fourier domain data, demonstrating superior performance on RHESSI and STIX observations.

Contribution

The study presents the first application of Variably Scaled Kernels for visibility interpolation in solar X-ray imaging, enhancing image reconstruction accuracy especially with sparse Fourier data.

Findings

VSK-based interpolation outperforms previous methods for RHESSI data.

Significant improvements in STIX imaging due to sparse Fourier sampling.

Reliable reconstruction of narrow, ribbon-like flaring sources.

Abstract

Space telescopes for solar hard X-ray imaging provide observations made of sampled Fourier components of the incoming photon flux. The aim of this study is to design an image reconstruction method relying on enhanced visibility interpolation in the Fourier domain. % methods heading (mandatory) The interpolation-based method is applied on synthetic visibilities generated by means of the simulation software implemented within the framework of the Spectrometer/Telescope for Imaging X-rays (STIX) mission on board Solar Orbiter. An application to experimental visibilities observed by the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) is also considered. In order to interpolate these visibility data we have utilized an approach based on Variably Scaled Kernels (VSKs), which are able to realize feature augmentation by exploiting prior information on the flaring source and which are used here, for the first time, for image reconstruction purposes.} % results heading (mandatory) When compared to an interpolation-based reconstruction algorithm previously introduced for RHESSI, VSKs offer significantly better performances, particularly in the case of STIX imaging, which is characterized by a notably sparse sampling of the Fourier domain. In the case of RHESSI data, this novel approach is particularly reliable when either the flaring sources are characterized by narrow, ribbon-like shapes or high-resolution detectors are utilized for observations. % conclusions heading (optional), leave it empty if necessary The use of VSKs for interpolating hard X-ray visibilities allows a notable image reconstruction accuracy when the information on the flaring source is encoded by a small set of scattered Fourier data and when the visibility surface is affected by significant oscillations in the frequency domain.