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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-1171</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>Статьи</subject></subj-group></article-categories><title-group><article-title>Расчет фазы при повороте изображения 
в неплоском поляризационном нуль-интерферометре</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>Тавров</surname><given-names>А. В.</given-names></name></name-alternatives><email xlink:type="simple">tavrov@iki.rssi.ru &lt;mailto:tavrov@iki.rssi.ru&gt;, tavrov@gmx.net &lt;mailto:tavrov@gmx.net&gt;</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>Орлов</surname><given-names>Д. А.</given-names></name></name-alternatives><email xlink:type="simple">noemail@neicon.ru</email><xref ref-type="aff" rid="aff-2"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Виноградов</surname><given-names>И. И.</given-names></name></name-alternatives><email xlink:type="simple">noemail@neicon.ru</email><xref ref-type="aff" rid="aff-1"/></contrib></contrib-group><aff xml:lang="ru" id="aff-1"><institution>Институт космических исследований РАН, Москва</institution><country>Russian Federation</country></aff><aff xml:lang="ru" id="aff-2"><institution>Московский энергетический институт (технический университет), Москва</institution><country>Russian Federation</country></aff><pub-date pub-type="collection"><year>2010</year></pub-date><pub-date pub-type="epub"><day>07</day><month>02</month><year>2023</year></pub-date><volume>0</volume><issue>9</issue><fpage>31</fpage><lpage>37</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/1171">https://www.izmt.ru/jour/article/view/1171</self-uri><abstract><p>Предложен новый матричный метод расчета геометрического поворота изображения, учитывающий эффекты геометрической и динамической  фаз в неплоской оптической схеме. Для описания распространения света в этой системе алгебра поляризационных двумерных векторов и матриц Джонса двумерного пространства продолжена в трехмерное пространство. Приведены практические примеры неплоских схем поляризационных нуль-интерферометров для применений в астрономии и для прецизионного анализа волнового фронта.</p></abstract><trans-abstract xml:lang="en"><p>To evaluate the image rotation and to separate the effects of the geometric phase from the dynamic phase, a new matrix method is proposed for a non-planar optical schematic. Conventional 2×2 Jones matrix calculation is generalized and a new scheme of 3×3 matrix calculation is proposed. Several practical examples of non-planar interferometer schematics are discussed to be applied as an astronomical nulling interferometer and as an accurate wavefront metrological tool.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>интерферометр</kwd><kwd>поляризация</kwd><kwd>геометрическая фаза</kwd></kwd-group><kwd-group xml:lang="en"><kwd>interferometer</kwd><kwd>polarization</kwd><kwd>geometric phase</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">Тавров А. В. Физические основы ахроматической ноль интерферометрии для звездной коронографии // ЖЭТФ. 2008. Т. 134. Вып. 6(12). С. 1103-1114.</mixed-citation><mixed-citation xml:lang="en">Тавров А. В. Физические основы ахроматической ноль интерферометрии для звездной коронографии // ЖЭТФ. 2008. Т. 134. Вып. 6(12). 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