2008/05/28 by M. J. van Noort, L. Rouppe van der Voort, L. H. M. Rouppe van der Voort
Computer Science · Physics and Astronomy · #Adaptive optics and wavefront sensing #Artificial intelligence #Calibration #Computer science #Deconvolution #Geology #Image (mathematics) #Image resolution #Noise (video) #Optics #Physics #Polarimetry #Remote sensing #Scattering #Solar Radiation and Photovoltaics #Solar and Space Plasma Dynamics #Solar telescope #Telescope #astro-ph
paper · pdf · doi:10.1051/0004-6361:200809959
Accepted for publication in Astronomy & Astrophysics, 12 pages, 11 figures
arxiv created 2008/05/28 · openalex publication_date 2008/07/17 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Aims. We aim to achieve both high spatial resolution and high polarimetric sensitivity, using an earth-based 1m-class solar telescope, for the study of magnetic fine structure on the surface of the Sun.