A PART OF THE STARRY SKY DESCRITION FORMIG WHEN TV OBSERVATION

P. P. Sukhov; N. Z. Strygin

doi:10.18524/1810-4215.1996.9.87289

A PART OF THE STARRY SKY DESCRITION FORMIG WHEN TV OBSERVATION

Автор(и)

P. P. Sukhov Astronomical observatory, Odessa State University, Україна
N. Z. Strygin Astronomical observatory, Odessa State University, Україна

DOI:

https://doi.org/10.18524/1810-4215.1996.9.87289

Ключові слова:

Picels', pixels, measured, images, algoritm.

Анотація

The observing part of the starring sky is represented by two-dimentional pulse parametric field M, M = [(S,B,(X₀,Y₀)_i], i = 1,n. Where(X₀,Y₀) - optical radiation centroid's coordinates, B - Summary radiation (brightness), S - the object's area Compact object's isolation and their parameters S, B, (X₀, Y₀) determination real time algoritm is developed. The method may be realised by a middle class computer vision system (CVS). The CVS computing system may be realised by convejor inhomogeneous structure "base computer + functional oriented processor" (BC + FOP). Some FOp's units are developed. The method's efficiency was carried out when imitation testing of binary image models.