http://arxiv.org/abs/1812.08413
We describe two inversion methods for the reconstruction of hard X-ray solar images. The methods are tested against experimental visibilities recorded by the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) and synthetic visibilities based on the design of the Spectrometer/Telescope for Imaging X-rays (STIX).
A. Massone, F. Sciacchitano, M. Piana, et. al.
Fri, 21 Dec 18
45/72
Comments: submitted to ‘Nuovo Cimento’ as proceeding SOHE3