Telescope inaccuracy model based upon satellite laser ranging data

dc.contributor.authorZhaborovskyy, V.P.
dc.contributor.authorPap, V.O.
dc.contributor.authorMedvedsky, M.M.
dc.contributor.authorCholiy, V.Ya.
dc.date.accessioned2017-06-07T18:08:39Z
dc.date.available2017-06-07T18:08:39Z
dc.date.issued2013
dc.description.abstractIn this paper, a new approach to constructing a telescope pointing model is described. Procedures of data collection, data processing, and model construction are presented. Telescope encoder countings, obtained during satellite laser ranging, are used as input data for the construction of the model. The model is presented as a harmonical series with frequencies obtained by the maximum entropy spectral analysis method.uk_UA
dc.identifier.citationTelescope inaccuracy model based upon satellite laser ranging data / V.P. Zhaborovskyy, V.O. Pap, M.M. Medvedsky, V.Ya. Choliy // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 1. — С. 63-65. — Бібліогр.: 5 назв. — англ.uk_UA
dc.identifier.issn2227-1481
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/119612
dc.language.isoenuk_UA
dc.publisherГоловна астрономічна обсерваторія НАН Україниuk_UA
dc.relation.ispartofAdvances in Astronomy and Space Physics
dc.statuspublished earlieruk_UA
dc.titleTelescope inaccuracy model based upon satellite laser ranging datauk_UA
dc.typeArticleuk_UA

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