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<article article-type="research-article" dtd-version="1.3" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xml:lang="ru"><front><journal-meta><journal-id journal-id-type="publisher-id">izmertech</journal-id><journal-title-group><journal-title xml:lang="ru">Измерительная техника</journal-title><trans-title-group xml:lang="en"><trans-title>Izmeritel`naya Tekhnika</trans-title></trans-title-group></journal-title-group><issn pub-type="ppub">0368-1025</issn><issn pub-type="epub">2949-5237</issn><publisher><publisher-name>ФГУП "ВНИИФТРИ"</publisher-name></publisher></journal-meta><article-meta><article-id custom-type="elpub" pub-id-type="custom">izmertech-525</article-id><article-categories><subj-group subj-group-type="heading"><subject>Research Article</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="ru"><subject>ФУНДАМЕНТАЛЬНЫЕ ПРОБЛЕМЫ МЕТРОЛОГИИ</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>FUNDAMENTAL PROBLEMS OF METROLOGY</subject></subj-group></article-categories><title-group><article-title>Расщепление частоты свободной нутации ядра в магнитном поле Земли</article-title><trans-title-group xml:lang="en"><trans-title></trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Кузнецова</surname><given-names>Л. А.</given-names></name></name-alternatives><email xlink:type="simple">leila@lnfm1.sai.msu.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Пасынок</surname><given-names>С. Л.</given-names></name></name-alternatives><email xlink:type="simple">pasynok@vniiftri.ru</email><xref ref-type="aff" rid="aff-2"/></contrib></contrib-group><aff xml:lang="ru" id="aff-1"><institution>Государственный астрономический институт им. П.К. Штернберга МГУ им. М.В. Ломоносова</institution><country>Russian Federation</country></aff><aff xml:lang="ru" id="aff-2"><institution>Всероссийский научно-исследовательский институт физико-технических и радиотехнических измерений</institution><country>Russian Federation</country></aff><pub-date pub-type="collection"><year>2014</year></pub-date><pub-date pub-type="epub"><day>07</day><month>02</month><year>2023</year></pub-date><volume>0</volume><issue>6</issue><fpage>8</fpage><lpage>10</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; ФГУП "ВНИИФТРИ", 2023</copyright-statement><copyright-year>2023</copyright-year><copyright-holder xml:lang="ru">ФГУП "ВНИИФТРИ"</copyright-holder><copyright-holder xml:lang="en">ФГУП "ВНИИФТРИ"</copyright-holder><license xlink:href="https://www.izmt.ru/jour/about/submissions#copyrightNotice" xlink:type="simple"><license-p>https://www.izmt.ru/jour/about/submissions#copyrightNotice</license-p></license></permissions><self-uri xlink:href="https://www.izmt.ru/jour/article/view/525">https://www.izmt.ru/jour/article/view/525</self-uri><abstract><p>Анализ остаточных расхождений принятой теории МАС2000 и измерений последних лет показал, что структура этих расхождений не соответствует предсказанной. Согласно указанной теории детерминированная часть расхождений должна представлять собственные колебания на частоте свободной нутации ядра, однако корреляционный анализ выявляет большее число гармоник. Предложена модель, позволяющая полностью объяснить две главные составляющие в остаточных расхождениях теории и измерений. Полученные периоды совпадают с периодами, выделенными из расхождений модели МАС2000 и результатов измерений.</p></abstract><trans-abstract xml:lang="en"><p>The analysis of last years measurements has shown that the accepted IAU2000 theory has the best characteristics in comparison with other nutation models. However the analysis of residual divergences of the theory and measurement has shown that the structure of these divergences does not correspond to predictions of IAU2000 nutation theory. According tothis predictions the quasi-systematic part of these divergences should represent its own fluctuations on frequency of the core free nutation. However, the correlation analysis reveals the greater number of harmonics. A model allowing to explain completely the presence of two main components in residual divergences of IAU2000 nutation theory and measurements is suggested. The received periods coincide with periodsalloted from residual divergences of IAU2000 model and the results of measurements.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>вращение Земли</kwd><kwd>магнитное поле</kwd><kwd>глобальная геодинамика</kwd><kwd>свободная нутация ядра</kwd><kwd>Earth rotation</kwd><kwd>magnetic field</kwd><kwd>geodynamics</kwd><kwd>core free nutation</kwd></kwd-group></article-meta></front><back><ref-list><title>References</title><ref id="cit1"><label>1</label><citation-alternatives><mixed-citation xml:lang="ru">Vondrak J., Ron C. Resonant period of free core nutation - its observed changes and excitations // Acta Geodyn. Geomater. 2006. N.3.(143). P. 53-60.</mixed-citation><mixed-citation xml:lang="en">Vondrak J., Ron C. 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