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- W2009481142 abstract "The method of constructing error model of pointing the telescope to the target is present in the article. It bases on using the angular encoders data (azimuth and elevation). This angles are fixed in time in the satellite laser ranging. The data is presented in the codes of angles (in inside frame) and the moments of time, in which they are fixed. The consistence of procedures and result of received model are presented in article. Also advantages and disadvantages of the new model are considered in comparison with the method of stars observers. The method tested on the 40 passes of the satellites. The model constructing in station “Kyiv-Golosiiv” in 2003 year is used for the comparison.[1]. The accuracy of this model is on the level 15 arcsec. TARGET SETTING For successful observation of any object it is necessary to point at it instrument, with a help of which we will do observation and track it with necessary accuracy during all necessary time. Accuracy of pointing and tracking depends on type of observations and can be changed from dozens of angular minutes to fractions of angular seconds. So, the higher accuracy of pointing and tracking we need the more careful we will study and take into account reasons, which lead to inaccuracy. It was always paid much attention to the questions of construction of telescope inaccuracy model. It is necessary to pay attention to some of the following works [1]-[4]. For example, for radio-telescopes which function in VLBI network, created standard complex of software for observation of radio sources with aim of defining more precisely of telescope model parameters, because these radio-telescopes function under total control of computer, that is in automatic regime. Tendency of development of SLR technique directed to creation of automatized systems that can do observation of satellites in semiautomatic and automatic regimes. For this purpose it is necessary to provide accuracy of pointing by laser beam at observed object and make it’s tracking with accuracy that does not exceed a half of beam width. Reasons of not accurate laser beam pointing at satellite can be inaccuracy in telescope assembling and searching ephemeris. Inaccuracy in searching ephemeris can be compensated by moving calculated position of satellite along orbit. This correction can be done automatically during observation session changing “ephemeris” time of observations since we get reflected from satellite signals. More than that, at regular observations we can determine corrections to searching ephemeris ARTIFICIAL SATELLITES, Vol. 41, No. 3 2006 DOI: 10.2478/v10018-007-0010-8 Unauthenticated Download Date | 6/20/16 7:16 AM" @default.
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- W2009481142 date "2006-01-01" @default.
- W2009481142 modified "2023-09-25" @default.
- W2009481142 title "Construction of Telescope Inaccuracy Model According to Data of Satellites Laser Ranging" @default.
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