Compressed sensing and Sequential Monte Carlo for solar hard X-ray imaging
classification
🌌 astro-ph.SR
math.NAstat.CO
keywords
solarhardimagingmethodsvisibilitiesx-raycarlocompressed
read the original abstract
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).
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.