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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">litosphere</journal-id><journal-title-group><journal-title xml:lang="ru">Литосфера</journal-title><trans-title-group xml:lang="en"><trans-title>LITHOSPHERE (Russia)</trans-title></trans-title-group></journal-title-group><issn pub-type="ppub">1681-9004</issn><issn pub-type="epub">2500-302X</issn><publisher><publisher-name>A.N. Zavaritsky Institute of Geology and Geochemistry</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.24930/1681-9004-2023-23-4-549-563</article-id><article-id custom-type="elpub" pub-id-type="custom">litosphere-1931</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><subj-group subj-group-type="section-heading" xml:lang="en"><subject>Articles</subject></subj-group></article-categories><title-group><article-title>Кристаллы алмаза кимберлитовой трубки им. В. Гриба: морфология и структурно-химические особенности</article-title><trans-title-group xml:lang="en"><trans-title>Diamonds from V. Grib kimberlite pipe: Morphology and spectroscopic features</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>Васильев</surname><given-names>Е. А.</given-names></name><name name-style="western" xml:lang="en"><surname>Vasilev</surname><given-names>E. A.</given-names></name></name-alternatives><bio xml:lang="ru"><p>199106, Санкт-Петербург, 21 линия, 2</p></bio><bio xml:lang="en"><p>Evgenii A. Vasilev.</p><p>2 21 line, St. Petersburg 199106</p></bio><email xlink:type="simple">vasilev_ea@pers.spmi.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>Устинов</surname><given-names>В. Н.</given-names></name><name name-style="western" xml:lang="en"><surname>Ustinov</surname><given-names>V. N.</given-names></name></name-alternatives><bio xml:lang="ru"><p>163001, Архангельск, Троицкий пр-т, 168</p></bio><bio xml:lang="en"><p>Viktor N. Ustinov.</p><p>168 Troitsky av., Arkhangelsk 163001</p></bio><email xlink:type="simple">ustinovVN@agddiamonds.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>Лешуков</surname><given-names>С. И.</given-names></name><name name-style="western" xml:lang="en"><surname>Leshukov</surname><given-names>S. I.</given-names></name></name-alternatives><bio xml:lang="ru"><p>163001, Архангельск, Троицкий пр-т, 168</p></bio><bio xml:lang="en"><p>Sergei I. Leshukov.</p><p>168 Troitsky av., Arkhangelsk 163001</p></bio><email xlink:type="simple">Sleshukov@agddiamonds.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>Пенделяк</surname><given-names>Р. Н.</given-names></name><name name-style="western" xml:lang="en"><surname>Pendeliak</surname><given-names>R. N.</given-names></name></name-alternatives><bio xml:lang="ru"><p>163001, Архангельск, Троицкий пр-т, 168</p></bio><bio xml:lang="en"><p>Roman N. Pendeliak.</p><p>168 Troitsky av., Arkhangelsk 163001</p></bio><email xlink:type="simple">RPendelyak@agddiamonds.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>Николаева</surname><given-names>Э. В.</given-names></name><name name-style="western" xml:lang="en"><surname>Nikolaeva</surname><given-names>E. V.</given-names></name></name-alternatives><bio xml:lang="ru"><p>163001, Архангельск, ул. Урицкого, 47</p></bio><bio xml:lang="en"><p>Evelina V. Nikolaeva.</p><p>47 Uritsky st., Arkhangelsk 163001</p></bio><email xlink:type="simple">ENikolaeva@Geolrazvedka.ru</email><xref ref-type="aff" rid="aff-3"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru"><institution>Горный университет</institution><country>Россия</country></aff><aff xml:lang="en"><institution>Mining University</institution><country>Russian Federation</country></aff></aff-alternatives><aff-alternatives id="aff-2"><aff xml:lang="ru"><institution>АО “АГД ДАЙМОНДС”</institution><country>Россия</country></aff><aff xml:lang="en"><institution>JSC “AGD DIAMONDS”</institution><country>Russian Federation</country></aff></aff-alternatives><aff-alternatives id="aff-3"><aff xml:lang="ru"><institution>ООО “Архангельскгеолразведка”</institution><country>Россия</country></aff><aff xml:lang="en"><institution>JSC “Arkhangelskgeolrazvedka”</institution><country>Russian Federation</country></aff></aff-alternatives><pub-date pub-type="collection"><year>2023</year></pub-date><pub-date pub-type="epub"><day>08</day><month>09</month><year>2023</year></pub-date><volume>23</volume><issue>4</issue><fpage>549</fpage><lpage>563</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Васильев Е.А., Устинов В.Н., Лешуков С.И., Пенделяк Р.Н., Николаева Э.В., 2023</copyright-statement><copyright-year>2023</copyright-year><copyright-holder xml:lang="ru">Васильев Е.А., Устинов В.Н., Лешуков С.И., Пенделяк Р.Н., Николаева Э.В.</copyright-holder><copyright-holder xml:lang="en">Vasilev E.A., Ustinov V.N., Leshukov S.I., Pendeliak R.N., Nikolaeva E.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.lithosphere.ru/jour/article/view/1931">https://www.lithosphere.ru/jour/article/view/1931</self-uri><abstract><p>Объект исследований. В статье приводятся результаты изучения 500 кристаллов алмаза из керна скважин эксплуатационной разведки, вскрывающих кратерную и жерловую фации верхней части кимберлитовой трубки им. В. Гриба. Отдельно проанализированы кристаллы из туфов и туффитов (кратерная часть), ксенотуфобрекчии, автолитовой кимберлитовой брекчии и порфирового кимберлита (жерловая часть). Методы. Основной задачей исследования было морфологическое и спектроскопическое изучение алмазов трубки им. В.П. Гриба. Спектры поглощения ИК-диапазона регистрировались на спектрометре VERTEX-70 с микроскопом Hyperion 1000 при разрешении 2 см-1. По ним определялись общая концентрация и доля азота в форме дефектов В (NBS), коэффициенты поглощения полос В', 3107 см-1. Для выявления неоднородностей и цвета фотолюминесценции (ФЛ) регистрировались изображения в ФЛ при возбуждении 360 нм на приборе ALROSA VIEW PRO. При комнатной температуре спектры ФЛ регистрировались на спектрометре Horiba FL-3 при возбуждении 350, 450 нм. С возбуждением лазерами 405, 488 и 787 нм спектры ФЛ регистрировались на спектрометре InVia Renishaw при 77 К. Результаты. Распределение по концентрации азота и NBS алмаза трубки им. В. Гриба специфическое: около 50% кристаллов располагаются вдоль одной изотермы, высока доля (5%) низкоазотных кристаллов. В спектрах ФЛ 25% кристаллов выявлены линии 883/885 нм элементарного Ni-содержащего дефекта. Большинство кристаллов с этим дефектом имеют менее 400 ppm азота, но по NBS занимают весь диапазон. Эта система встречается в спектрах 76% двойников и сростков; к ним относятся 36% кристаллов с ФЛ на 883/885 нм. Изученные кристаллы трубки им. В. Гриба отличаются от продукции месторождения им. М.В. Ломоносова намного меньшим содержанием индивидов кубического габитуса (2 и 15%), меньшей степенью их растворения (октаэдров 33 и 15% соответственно), низкой долей окрашенных камней, широким диапазоном концентрации азота и NBS. Выводы. Выявленные особенности указывают на специфические условия кристаллизации алмаза месторождения им. В. Гриба, отличающиеся от таковых в других кимберлитовых телах Восточно-Европейской, Сибирской платформ и россыпей Урала. Высокая доля низкоазотных кристаллов и индивидов с примесью Ni может быть индикатором наличия в трубке крупных кристаллов типа CLIPPIR.</p></abstract><trans-abstract xml:lang="en"><p>Research subject. The article presents the results of studying 500 diamond crystals from the core of exploration boreholes of crater and diatreme facies of the upper part of V. Grib kimberlite pipe. Crystals from tuffs and tuffites (crater), tufobreccia, autolith kimberlite breccia and porphyry kimberlite (diatreme) were analyzed separately. aim. To carry out a morphological and spectroscopic study of diamonds from V. Grib pipe. Materials and Methods. An VERTEX-70 spectrometer with a Hyperion 1000 microscope was used to determine the total nitrogen concentration and the share of nitrogen in the form of B defects (NBS), the absorption coefficients of the “platelet” bands B', 3107 cm-1. Images of photoluminescence (PL) were recorded at 360 nm excitation by an ALROSA VIEW PRO device, in order to detect inhomogeneities and color of PL. The PL spectra were recorded by a Horiba FL-3 spectrometer with an excitation of 350 and 450 nm at 300 K and by an InVia Renishaw spectrometer with an excitation of 405, 488 and 787 nm at 77 K. Results. The distribution of diamonds in terms of nitrogen concentration and NBS is specific; about 50% of the crystals are located along one isotherm, the proportion of low-nitrogen crystals is 5%. The PL spectra of 25% of crystals showed the lines of 883/885 nm of an elementary Ni-containing defect. Most crystals with this defect have less than 400 ppm of nitrogen, but they occupy the entire range according to NBS. This system is found in the spectra of 76% of twins and intergrowth; the latter are of 36% of diamonds with the lines 883/885 nm. The studied diamonds differ from those found in M.V. Lomonosov deposit in terms of a much lower content of crystals of cubic habitus (2 and 15%), a lower degree of dissolution (octahedra, respectively, 33 and 15%), a low proportion of colored stones, as well as a wide range of nitrogen concentration and NBS. Conclusion. The revealed features indicate the specific growth conditions of diamonds from V. Grib deposit, which differed from those of diamonds from other kimberlitic bodies of the East European, Siberian platforms and the Urals. The high proportion of low-nitrogen crystals and Ni-containing diamonds is a possible indicator for the presence of large CLIPPIR-type crystals.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>алмаз</kwd><kwd>трубка им. В. Гриба</kwd><kwd>ИК-спектроскопия</kwd><kwd>фотолюминесценция</kwd><kwd>азот</kwd><kwd>дефекты кристаллической структуры</kwd></kwd-group><kwd-group xml:lang="en"><kwd>diamond</kwd><kwd>V. Grib kimberlite pipe</kwd><kwd>FTIR</kwd><kwd>photoluminescence</kwd><kwd>nitrogen</kwd><kwd>crystal structure defects</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">Васильев Е.А., Клепиков И.В., Лукьянова Л.И. (2018) Сравнение кристаллов алмаза Рассольнинской депрессии и современных аллювиальных россыпей Красновишерского района (Приуралье). Зап. РМО, 147(1), 55-68.</mixed-citation><mixed-citation xml:lang="en">Baker J.M. 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