Non-parametric PSF estimation from celestial transit solar images using blind deconvolution

Context: Characterization of instrumental effects in astronomical imaging is important in order to extract accurate physical information from the observations. The measured image in a real optical instrument is usually represented by the convolution of an ideal image with a Point Spread Function (PS...

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Bibliographic Details
Main Authors: González Adriana, Delouille Véronique, Jacques Laurent
Format: Article
Language:English
Published: EDP Sciences 2016-01-01
Series:Journal of Space Weather and Space Climate
Subjects:
Online Access:http://dx.doi.org/10.1051/swsc/2015040

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