Aims. To provide a schematic mathematical description of the imaging concept of the Spectrometer/Telescope for Imaging X-rays (STIX) on board Solar Orbiter. The derived model is the fundamental starting point for both the interpretation of STIX data and the description of the data calibration process. Methods. We describe the STIX indirect imaging technique which is based on spatial modulation of the X-ray photon flux by means of tungsten grids. We show that each of 30 STIX imaging sub-collimators measures a complex Fourier component of the flaring X-ray source corresponding to a specific angular frequency. We also provide details about the count distribution model, which describes the relationship between the photon flux and the measured pixel counts. Results. We define the image reconstruction problem for STIX from both visibilities and photon counts. We provide an overview of the algorithms implemented for the solution of the imaging problem, and a comparison of the results obtained with these different methods in the case of the SOL2022-03-31T18 flaring event.
@article{arxiv.2303.02485,
title = {STIX imaging I -- Concept},
author = {Paolo Massa and Gordon. J. Hurford and Anna Volpara and Matej Kuhar and Andrea Francesco Battaglia and Hualin Xiao and Diego Casadei and Emma Perracchione and Sara Garbarino and Sabrina Guastavino and Hannah Collier and Ewan C. M. Dickson and Daniel F. Ryan and Shane A. Maloney and Frederic Schuller and Alexander Warmuth and Anna Maria Massone and Federico Benvenuto and Michele Piana and Säm Krucker},
journal= {arXiv preprint arXiv:2303.02485},
year = {2023}
}