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.

Посилання

Val'teris S.E.: 1983, Trudy AN Litov. SSR, 3, 105.

Strygin N.Z.: 1985, Author. Svidet. USSR N1487069 G06 F15/66.

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Опубліковано

2017-11-04

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