About using wide lens field optics for observations artificial satellites and space surveillance (O primenenii shirokopol'nykh linzovykh ob"yektivov dlya zadach kontrolya kosmicheskogo prostranstva, on Russian)
Sukhov, P. P.; Volkov, S. K.; Karpenko, G. F.; Gubin, E. G.; Titenko, V. V.; Yamnitsky, V. A.; Tkachenko, A. A.
On base results of the observations in Odessa astronomical observatory (Ukraine), is shown. The possibility of the using domestic wide field lens optics for monitoring high orbital objects. With wide field lens optics "Tair-19 5003", limited mag = 15m.5 per 10 seconds of the accumulation, average square-error (ASE) of the measurements of the coordinates slowly moving GSS not more than 2 arcsec. About 90% measurements has ASE less 1 arcsec. At surveillance of the area of the equator by width 5° areas 500 square deg. are discovered 46 active GSS, 12 passive GSS and 2 high elliptical orbital satellites (HEO). Is shown perspective possibility of the use WFO for monitoring LEO height before of 2 000 km. 90% of 39 objects LEO fixed in mode "beam-park" in current 1 hour, surely are identified using catalog NORAD.
Some modern astronomical problem of creating television-measuring systems (ATVMS) for observations artificial earth satellites (Nekotoryye sovremennyye problemy sozdaniya astronomicheskikh televizionno-izmeritel'nykh sistem (ATVIS) dlya nablyudeniy za iskusstvennymi sputnikami Zemli, on Russian))
Prokof'yeva-Mikhaylovskaya, V. V.; Strígin, N. Z.; Sukhov, P. P.; Karpenko, G. F.
History of the artificial satellite observations is briefly described. On objective reasons there is no enough perfected methodses of the creation astronomical television-measuring systems (ATVMS) on today. There are shown some problems methdological, technological, algorithmic and etc nature, which necessary to solve for development of this methods. Possible ways of the decision is specified for some problems.