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)
Visibilities are calibrated measurements of sampled Fourier components of a source distribution. In ...
Context. This paper is concerned with the image reconstruction problem when the measured data are so...
The Ramaty High Energy Solar Spectroscopic Imager (RHESSI) mission provides information on high reso...
We describe two inversion methods for the reconstruction of hard Xray solar images. The methods are ...
Aims. Compressed sensing realized by means of regularized deconvolution and the finite isotropic wav...
The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) produces solar flare images with t...
Space telescopes for solar hard X-ray imaging provide observations made of sampled Fourier component...
The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) produces solar flare images with t...
The Spectrometer/Telescope for Imaging X-rays (STIX) is one of six remote sensing instruments on-boa...
Aims. We seek to determine to what extent the problem of forward fitting visibilities measured by th...
STIX is a X-ray imaging spectroscopy device to be mounted as part of the Solar Orbiter cluster. Its ...
The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) uses rotational modulation synthes...
Context. The Spectrometer/Telescope for Imaging X-rays (STIX) is one of 6 remote sensing instruments...
In this paper we present new optimization strategies for the reconstruction of X-ray images of solar...
The Spectrometer/Telescope for Imaging X-rays (STIX) will study solar flares across the hard X-ray w...
Visibilities are calibrated measurements of sampled Fourier components of a source distribution. In ...
Context. This paper is concerned with the image reconstruction problem when the measured data are so...
The Ramaty High Energy Solar Spectroscopic Imager (RHESSI) mission provides information on high reso...
We describe two inversion methods for the reconstruction of hard Xray solar images. The methods are ...
Aims. Compressed sensing realized by means of regularized deconvolution and the finite isotropic wav...
The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) produces solar flare images with t...
Space telescopes for solar hard X-ray imaging provide observations made of sampled Fourier component...
The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) produces solar flare images with t...
The Spectrometer/Telescope for Imaging X-rays (STIX) is one of six remote sensing instruments on-boa...
Aims. We seek to determine to what extent the problem of forward fitting visibilities measured by th...
STIX is a X-ray imaging spectroscopy device to be mounted as part of the Solar Orbiter cluster. Its ...
The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) uses rotational modulation synthes...
Context. The Spectrometer/Telescope for Imaging X-rays (STIX) is one of 6 remote sensing instruments...
In this paper we present new optimization strategies for the reconstruction of X-ray images of solar...
The Spectrometer/Telescope for Imaging X-rays (STIX) will study solar flares across the hard X-ray w...
Visibilities are calibrated measurements of sampled Fourier components of a source distribution. In ...
Context. This paper is concerned with the image reconstruction problem when the measured data are so...
The Ramaty High Energy Solar Spectroscopic Imager (RHESSI) mission provides information on high reso...
DOI
Add to ORKG