We describe two inversion methods for the reconstruction of hard Xray 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).
Compressed sensing and Sequential Monte Carlo for solar hard X-ray imaging
Massone A. M.;Sciacchitano F.;Piana M.;Sorrentino A.
2019-01-01
Abstract
We describe two inversion methods for the reconstruction of hard Xray 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).
File in questo prodotto:
| File | Dimensione | Formato | |
|---|---|---|---|
|
ncc11770.pdf
accesso aperto
Descrizione: Articolo principale
Tipologia:
Documento in versione editoriale
Dimensione
274.29 kB
Formato
Adobe PDF
|
274.29 kB | Adobe PDF | Visualizza/Apri |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
