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Compressed sensing and Sequential Monte Carlo for solar hard X-ray imaging. (arXiv:1812.08413v1 [astro-ph.SR])
来源于:arXiv
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). 查看全文>>