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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">gtcrust</journal-id><journal-title-group><journal-title xml:lang="ru">Геодинамика и тектонофизика</journal-title><trans-title-group xml:lang="en"><trans-title>Geodynamics &amp; Tectonophysics</trans-title></trans-title-group></journal-title-group><issn pub-type="epub">2078-502X</issn><publisher><publisher-name>Institute of the Earth's crust of the Russian Academy of Sciences, Siberian Branch</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.5800/GT-2019-10-2-0424</article-id><article-id custom-type="elpub" pub-id-type="custom">gtcrust-851</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>СОВРЕМЕННАЯ ГЕОДИНАМИКА</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>RECENT GEODYNAMICS</subject></subj-group></article-categories><title-group><article-title>ГЕНЕРАЛЬНАЯ Pb‐ИЗОТОПНАЯ СИСТЕМАТИКА ИСТОЧНИКОВ ВУЛКАНИЧЕСКИХ ПОРОД НОВЕЙШЕГО ГЕОДИНАМИЧЕСКОГО ЭТАПА АЗИИ</article-title><trans-title-group xml:lang="en"><trans-title>GENERAL PB‐ISOTOPE SYSTEMATICS OF SOURCES FOR VOLCANIC ROCKS OF THE LATEST GEODYNAMIC STAGE IN ASIA</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0001-9084-1652</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Рассказов</surname><given-names>С. В.</given-names></name><name name-style="western" xml:lang="en"><surname>Rasskazov</surname><given-names>S. V.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Сергей Васильевич Рассказов - доктор геолого–минералогических наук, профессор, заведующий лабораторией</p><p>664033, Иркутск, ул. Лермонтова, 128, </p><p>664003, Иркутск, ул. Ленина, 3</p></bio><bio xml:lang="en"><p>Sergei V. Rasskazov - Doctor of Geology and Mineralogy, Professor, Head of Laboratory</p><p>128 Lermontov street, Irkutsk 664033, </p><p>3 Lenin street, Irkutsk 664003</p></bio><email xlink:type="simple">rassk@crust.irk.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-1582-4753</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Чувашова</surname><given-names>И. С.</given-names></name><name name-style="western" xml:lang="en"><surname>Chuvashova</surname><given-names>I. S.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Ирина Сергеевна Чувашова - кандидат геолого-минералогических наук, старший научный сотрудник</p><p>664033, Иркутск, ул. Лермонтова, 128, </p><p>664003, Иркутск, ул. Ленина, 3</p></bio><bio xml:lang="en"><p>Irina S. Chuvashova - Candidate of Geology and Mineralogy, Senior Researcher</p><p>128 Lermontov street, Irkutsk 664033, </p><p>3 Lenin street, Irkutsk 664003</p></bio><email xlink:type="simple">chuvashova@crust.irk.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>Ясныгина</surname><given-names>Т. А.</given-names></name><name name-style="western" xml:lang="en"><surname>Yasnygina</surname><given-names>Т. A.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Татьяна Александровна Ясныгина - кандидат геолого-минералогических наук, старший научный сотрудник</p><p>664033, Иркутск, ул. Лермонтова, 128</p></bio><bio xml:lang="en"><p>Tatiana A. Yasnygina - Candidate of Geology and Mineralogy, Senior Researcher</p><p>128 Lermontov street, Irkutsk 664033</p></bio><email xlink:type="simple">ty@crust.irk.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>Сунь</surname><given-names>Йи‐минь</given-names></name><name name-style="western" xml:lang="en"><surname>Sun</surname><given-names>Yi‐min</given-names></name></name-alternatives><bio xml:lang="ru"><p>Сунь Йи-минь - научный сотрудник</p><p>164155, Удаляньчи, Хэйлунцзян</p></bio><bio xml:lang="en"><p>Wudalianchi 164155, Heilongjiang</p></bio><email xlink:type="simple">894817259@qq.com</email><xref ref-type="aff" rid="aff-3"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Саранина</surname><given-names>Е. В.</given-names></name><name name-style="western" xml:lang="en"><surname>Saranina</surname><given-names>Е. V.</given-names></name></name-alternatives><bio xml:lang="ru"><p>664033, Иркутск, ул. Лермонтова, 128</p></bio><bio xml:lang="en"><p>128 Lermontov street, Irkutsk 664033</p></bio><email xlink:type="simple">e_v_sar@mail.ru</email><xref ref-type="aff" rid="aff-2"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru"><institution>Институт земной коры СО РАН;&#13;
Иркутский государственный университет</institution><country>Россия</country></aff><aff xml:lang="en"><institution>Institute of the Earth's Crust, Siberian Branch of RAS;&#13;
Irkutsk State University</institution><country>Russian Federation</country></aff></aff-alternatives><aff-alternatives id="aff-2"><aff xml:lang="ru"><institution>Институт земной коры СО РАН</institution><country>Россия</country></aff><aff xml:lang="en"><institution>Institute of the Earth's Crust, Siberian Branch of RAS</institution><country>Russian Federation</country></aff></aff-alternatives><aff-alternatives id="aff-3"><aff xml:lang="ru"><institution>Институт вулканов и минеральных источников Хэйлунцзянской академии наук</institution><country>Китай</country></aff><aff xml:lang="en"><institution>Institute of Volcano and Mineral Spring, Heilongjiang Academy of Science</institution><country>China</country></aff></aff-alternatives><pub-date pub-type="collection"><year>2019</year></pub-date><pub-date pub-type="epub"><day>24</day><month>06</month><year>2019</year></pub-date><volume>10</volume><issue>2</issue><fpage>507</fpage><lpage>539</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Рассказов С.В., Чувашова И.С., Ясныгина Т.А., Сунь Й., Саранина Е.В., 2019</copyright-statement><copyright-year>2019</copyright-year><copyright-holder xml:lang="ru">Рассказов С.В., Чувашова И.С., Ясныгина Т.А., Сунь Й., Саранина Е.В.</copyright-holder><copyright-holder xml:lang="en">Rasskazov S.V., Chuvashova I.S., Yasnygina Т.A., Sun Y., Saranina Е.V.</copyright-holder><license xml:lang="ru" license-type="creative-commons-attribution" xlink:href="https://creativecommons.org/licenses/by/4.0/" xlink:type="simple"><license-p>Данная работа распространяется под лицензией Creative Commons Attribution 4.0.</license-p></license><license xml:lang="en" license-type="creative-commons-attribution" xlink:href="https://creativecommons.org/licenses/by/4.0/" xlink:type="simple"><license-p>This work is licensed under a Creative Commons Attribution 4.0 License.</license-p></license></permissions><self-uri xlink:href="https://www.gt-crust.ru/jour/article/view/851">https://www.gt-crust.ru/jour/article/view/851</self-uri><abstract><p>Современная теория эволюционирующей Земли основана на комплексных изотопных данных о доступной для опробования части планеты и космических телах, в которых ключевую роль играют построения в U‐Pb изотопной системе. Теория тестируется разработанной изотопной систематикой источников океанических базальтов. Происхождение вулканических пород континентов часто трактуется в терминах изотопной систематики океанических базальтов. Однако такие интерпретации, как правило, содержат противоречия, вытекающие из различий истории становления и ныне существующих различий в динамике мантии океанов и континентов. Под океанами мантийный материал давно утратил связь с поверхностными структурами Земли; под континентами такая связь нередко устанавливается. Характер эволюции глубинных процессов под континентами остается неопределенным и, по аналогии с океанами, требует расшифровки в терминах компонентов мантийных источников вулканических пород. В современных литосферных плитах Земли различаются области шириной от сотен до тысяч километров, характеризующиеся высокой скоростью деформаций и, следовательно, по меньшей мере, на один – два порядка пониженной вязкостью относительно внутренних стабильных частей плит, что придает им особый структурный статус «рассеянных плитных границ». Изотопно‐геохимические исследования вулканических пород регионов нестабильной Азии выявили различный характер компонентов источников, для которых были предложены частные интерпретации. В настоящей работе определяется генеральная систематика источников вулканических пород новейшего геодинамического этапа Азии по оценке времени инкубации их материала на диаграмме 207Pb/204Pb–206Pb/204Pb. Обозначаются два домена: один – с низким 238U/204Pb (LOMU), производный вязкой протомантии (VIPMA), другой – с повышенным 238U/204Pb (ELMU). Мантийные домены эволюционировали от первичного материала Земли во временных интервалах 4.51–4.36 млрд лет назад, 4.0–3.7 млрд лет назад, 2.9–2.6 млрд лет назад, 2.0–1.8 млрд лет назад, около 0.66 млрд лет назад и &lt;0.09 млрд лет назад. Расплавные аномалии источников ELMU характеризуют нестабильную мантию Южной Азии, расплавные аномалии источников LOMU – мантию Японско‐Байкальского геодинамического коридора области перехода от нестабильной мантии Азии к ее стабильному ядру. Позднекайнозойская эволюция Японско‐Байкальского геодинамического коридора привела к рассечению домена LOMU Чеджу‐Витимской линией источников ELMU.</p></abstract><trans-abstract xml:lang="en"><p>The modern theory of the evolving Earth is based on integrated isotopic data obtained for the accessible part of the planet and cosmic bodies, in which the U–Pb isotope system plays a key role. The theory is tested by the isotope systematics of oceanic basalt sources. The origin of continental volcanic rocks is often interpreted in terms of the isotopic systematics of oceanic basalts. However, such interpretations, as a rule, reveal contradictions arising from differences in the history and current mantle dynamics of oceans and continents. Under the oceans, a mantle material has long lost connection with the accessible Earth tectonic units; under the continents such a connection is often established. The nature of the evolution of deep‐seated processes under the continents remains uncertain and, by analogy with the oceans, requires deciphering in terms of the components of the mantle sources for volcanic rocks. In modern lithospheric plates of the Earth, there are regions ranging in width from hundreds to thousands of kilometers, which are characterized by high strain rates and, consequently, at least one to two orders of magnitude lower viscosity relative to that of the internal stable parts of the plates. This gives them a special structural status of “dispersed plate boundaries”. The isotope‐geochemical studies of volcanic rocks from regions of the unstable Asia revealed the different nature of components in sources, for which particular interpretations have been proposed. In this paper, a general systematics of sources is defined for volcanic rocks of the latest geodynamic stage in Asia through estimating the incubation time on the 207Pb/204Pb versus 206Pb/204Pb diagram. Two domains are designated: (1) low 238U/204Pb (LOMU) derived from the viscous protomantle (VIPMA), and (2) elevated 238U/204Pb (ELMU). The mantle domains evolved from the Earth's primary material between 4.51 and 4.36 Gyr ago, 4.0 and 3.7 Gyr ago, 2.9 and 2.6 Gyr ago, 2.0 and 1.8 Gyr ago, about 0.66 Gyr ago and &lt;0.09 Gyr ago. Melting anomalies of ELMU sources characterize the unstable mantle of Southern Asia, and those of LOMU sources belong to the Japan‐Baikal geodynamic corridor of the transitional region between the unstable mantle of Asia and its stable core. The Late Cenozoic evolution of the Japan‐Baikal geodynamic corridor resulted in cutting the LOMU domain by the Jeju‐Vitim ELMU source line.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>вулканические породы</kwd><kwd>изотопы Pb</kwd><kwd>новейший геодинамический этап</kwd><kwd>геодинамический коридор</kwd><kwd>Азия</kwd></kwd-group><kwd-group xml:lang="en"><kwd>volcanic rocks</kwd><kwd>Pb isotopes</kwd><kwd>latest geodynamic stage</kwd><kwd>geodynamic corridor</kwd><kwd>Asia</kwd></kwd-group><funding-group><funding-statement xml:lang="ru">Работа выполнена в Китайско-Российском исследовательском центре Удаляньчи–Байкал по новейшему вулканизму и окружающей среде при поддержке РНФ (проект 18-77-10027)</funding-statement></funding-group></article-meta></front><back><ref-list><title>References</title><ref id="cit1"><label>1</label><citation-alternatives><mixed-citation xml:lang="ru">Albarède F., 2009. Volatile accretion history of the terrestrial planets and dynamic implications. 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