An instability of the trigonometric solution for the periodical components of the polar motion

dc.contributor.authorChapanov, Ya.
dc.date.accessioned2015-04-03T18:29:31Z
dc.date.available2015-04-03T18:29:31Z
dc.date.issued2005
dc.description.abstractEstimation of the real errors of the polar motion approximation with trigonometric functions is made by a model of simulated polar motion with variable amplitudes of the Chandler and seasonal components. It is shown that the real errors of the trigonometric coefficients are much more than the formal estimation errors, obtained by the least-squares method (LSM).uk_UA
dc.description.sponsorshipThe work was supported by the National Council for Scientific Research at Ministry of Education and Science of Republic Bulgaria with the grant NZ-1213/02, also by the Organizing Committee of the MAO-2004 Conference “Astronomy in Ukraine – Past, Present and Future”, Kiev, Ukraine, July 15–17, 2004.uk_UA
dc.identifier.citationAn instability of the trigonometric solution for the periodical components of the polar motion / Ya. Chapanov // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 351-354. — Бібліогр.: 3 назв. — англ.uk_UA
dc.identifier.issn0233-7665
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/79673
dc.language.isoenuk_UA
dc.publisherГоловна астрономічна обсерваторія НАН Україниuk_UA
dc.relation.ispartofКинематика и физика небесных тел
dc.statuspublished earlieruk_UA
dc.subjectMS4: Positional Astronomy and Global Geodynamicsuk_UA
dc.titleAn instability of the trigonometric solution for the periodical components of the polar motionuk_UA
dc.typeArticleuk_UA

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