How to determine the quality of solar granulation images: The optimal window method

Authors
Citation
C. Giammanco, How to determine the quality of solar granulation images: The optimal window method, ASTR AST SS, 147(1), 2000, pp. 1-4
Citations number
6
Categorie Soggetti
Space Sciences
Journal title
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES
ISSN journal
03650138 → ACNP
Volume
147
Issue
1
Year of publication
2000
Pages
1 - 4
Database
ISI
SICI code
0365-0138(200011)147:1<1:HTDTQO>2.0.ZU;2-A
Abstract
An optimal window for image analysis is determined by means of information theory. The size of the window is then used as a good estimator of image qu ality. The method is sensitive to the size of the structures present in the image (contrary to the contrast method, widely used to select the best ima ges of a series) and can provide a quality map, indicating the zones more o r less degraded in the image. In this letter I describe the optimal window method (OWM) and compare it with the contrast method, showing a first appli cation to a series of images taken at Themis IPM.