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Optical Image of Stars in the Camera Field
Author(s) -
Tschobanoff P. D.,
Nikolov N. S.
Publication year - 1979
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.19793000506
Subject(s) - collimator , stars , atmosphere (unit) , physics , optical image , turbulence , field (mathematics) , optics , astronomy , remote sensing , image (mathematics) , computer science , computer vision , meteorology , geology , mathematics , pure mathematics
The possibility the turbulent atmosphere to act as a cause for an amplification of the optical star images is considered. This is made on introducing the turbulent atmosphere a an optical collimator set. Some considerations about the modelling and formalization of this effect are made. Finally some consequences relative to the optical record photometrical information extraction are mentioned.