Astron. Astrophys. Suppl. Ser. 131, 371-375
E. Bratsolis1,2 - M. Sigelle3
Send offprint request: E. Bratsolis (ebrats@atlas.uoa.gr)
1 - Astronomical Institute, National Observatory of Athens,
P.O. Box 20048, GR-11810 Athens, Greece
2 -
Section of Astrophysics, Astronomy and Mechanics, Department of
Physics, University of Athens, GR-15784 Athens, Greece
3 -
École Nationale Supérieure des Télécommunications,
Département Images, 46 rue Barrault, F-75634 Paris Cedex 13, France
Received September 8, 1997; accepted February 23, 1998
We present a "continuous'' analysis of a solar image
in order to address the problem of image segmentation. Our approach
is based on combinatorial optimization methods and in particular on
Mean Field Fast Annealing (MFFA).
Mean-field theory gives a deterministic nature to our algorithm
while its efficiency is improved by a fast cooling schedule.
We show how this method can be used to separate efficiently the
regions of different solar activity giving a tool for a future
automated recognition and classification of sunspots.
Key words: sunspots -- methods: data analysis
Copyright The European Southern Observatory (ESO)