Number of the records: 1  

Probabilistic suppression of astronomical degradations

  1. 1.
    SYSNO ASEP0080188
    Document TypeA - Abstract
    R&D Document TypeThe record was not marked in the RIV
    R&D Document TypeNení vybrán druh dokumentu
    TitleProbabilistic suppression of astronomical degradations
    Author(s) Haindl, Michal (UTIA-B) RID, ORCID
    Šimberová, Stanislava (ASU-R) RID
    Source TitleProceedings of Abstracts of Modern Solar Facilities - Advanced Solar Science. - Göttingen : Universitätsverlag Göttingen, 2007
    s. 1-1
    Number of pages1 s.
    ActionModern solar facilities - advanced solar science
    Event date27.09.2006-29.09.2006
    VEvent locationGöttingen
    CountryDE - Germany
    Event typeWRD
    Languageeng - English
    CountryDE - Germany
    Keywordsimage restoration ; multichannel restoration
    Subject RIVBD - Theory of Information
    R&D Projects1ET400750407 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
    1M0572 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    GA102/04/0155 GA ČR - Czech Science Foundation (CSF)
    CEZAV0Z10750506 - UTIA-B (2005-2011)
    AnnotationA multichannel fast adaptive recursive restoration method based on the underlying spatial probabilistic image model is presented. The method assumes linear degradation model with the unknown possibly non-homogeneous point-spread function and additive noise for each of mutually registered degraded observations. Pixels in the vicinity of image steep discontinuities are left unrestored to minimize restoration blurring effect. The method is completely autonomous and doesn't assume any knowledge of the underlying degradation process. The algorithm is verified on the artificial data with known ideal image. In the multichannel input are blurred channels created from the ideal image using various degradation functions. Then the method is applied to the real optical solar data. The experiments are carried on the synthetic data set and on a sequence of the short-exposure solar photosphere images. The multichannel input is presented by the temporal plains of a data cube. The results are compared under the most frequented criterions of image quality. The method can be also easily and naturally generalized for multispectral (e.g. colour, multispectral satellite images) or registered images which is seldom the case for alternative methods.
    WorkplaceInstitute of Information Theory and Automation
    ContactMarkéta Votavová, votavova@utia.cas.cz, Tel.: 266 052 201.
    Year of Publishing2007
Number of the records: 1  

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