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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">nuc</journal-id><journal-title-group><journal-title xml:lang="ru">Вестник НЯЦ РК</journal-title><trans-title-group xml:lang="en"><trans-title>NNC RK Bulletin</trans-title></trans-title-group></journal-title-group><issn pub-type="ppub">1729-7516</issn><issn pub-type="epub">1729-7885</issn><publisher><publisher-name>Национальный ядерный центр Республики Казахстан</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.52676/1729-7885-2025-3-164-175</article-id><article-id custom-type="elpub" pub-id-type="custom">nuc-881</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>ИОНОСФЕРНАЯ БУРЯ 25/26 МАЯ 1967 Г. КАК МОДЕЛЬ ОТКЛИКА ИОНОСФЕРЫ НА ЭКСТРЕМАЛЬНОЕ ВОЗМУЩЕНИЕ МАГНИТНОГО ПОЛЯ ЗЕМЛИ</article-title><trans-title-group xml:lang="en"><trans-title>IONOSPHERIC STORM OF MAY 25/26, 1967 AS A MODEL OF IONOSPHERIC RESPONSE TO EXTREME DISTURBANCE OF THE EARTH'S MAGNETIC FIELD</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0001-5596-9108</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Гордиенко</surname><given-names>Г. И.</given-names></name><name name-style="western" xml:lang="en"><surname>Gordienko</surname><given-names>G. I.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Гордиенко Галина И. - заведующая лаборатории физики и моделирования ионосферы, главный научный сотрудник.</p><p>Алматы</p></bio><bio xml:lang="en"><p>Almaty</p></bio><email xlink:type="simple">ggordiyenko@mail.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/0000-0002-1838-0676</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Литвинов</surname><given-names>Ю. Г.</given-names></name><name name-style="western" xml:lang="en"><surname>Litvinov</surname><given-names>Yu. G.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Литвинов Юрий Г. - лаборатории физики и моделирования ионосферы, ведущий научный сотрудник.</p><p>Алматы</p></bio><bio xml:lang="en"><p>Almaty</p></bio><email xlink:type="simple">yurii-litvinov@mail.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/0000-0001-9250-182X</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Жиганбаев</surname><given-names>М. Ю.</given-names></name><name name-style="western" xml:lang="en"><surname>Zhiganbayev</surname><given-names>M. Yu.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Жиганбаев Мурат Ю. - лаборатория физики и моделирования ионосферы, старший научный сотрудник.</p><p>Алматы</p></bio><bio xml:lang="en"><p>Almaty</p></bio><email xlink:type="simple">zhiganbayev@ionos.kz</email><xref ref-type="aff" rid="aff-1"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru">ТОО «Институт ионосферы»<country>Казахстан</country></aff><aff xml:lang="en">“Institute of Ionosphere” LLP<country>Kazakhstan</country></aff></aff-alternatives><pub-date pub-type="collection"><year>2025</year></pub-date><pub-date pub-type="epub"><day>18</day><month>10</month><year>2025</year></pub-date><volume>0</volume><issue>3</issue><fpage>164</fpage><lpage>175</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Гордиенко Г.И., Литвинов Ю.Г., Жиганбаев М.Ю., 2025</copyright-statement><copyright-year>2025</copyright-year><copyright-holder xml:lang="ru">Гордиенко Г.И., Литвинов Ю.Г., Жиганбаев М.Ю.</copyright-holder><copyright-holder xml:lang="en">Gordienko G.I., Litvinov Y.G., Zhiganbayev M.Y.</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://journals.nnc.kz/jour/article/view/881">https://journals.nnc.kz/jour/article/view/881</self-uri><abstract><p>Представлены результаты исследования ионосферных эффектов экстремальной геомагнитной бури 25/26 мая 1967 г. (Dst = –387 nT), полученные с использованием ионосферных данных, измеренных на пяти ионосферных станциях, расположенных в регионе Средней Азии. Геомагнитная буря с начальной фазой продолжительностью примерно 9 часов, началась в ~20 UT 25 мая, что для рассматриваемого региона соответствует ночному времени (в 00:01 LT) 26 мая.</p><p>Отрицательное ионосферное возмущение продолжительностью порядка 28 часов, начавшееся на всех рассматриваемых станциях во время начала главной фазы геомагнитной бури, характеризовалось понижением критических частот слоя F2 ионосферы foF2 в 2,2 раза по сравнению с уровнем foF2 в спокойных геомагнитных условиях. Наблюдавшееся во время отрицательной фазы ионосферной бури «условие G», когда foF2 ≤ foF1, продолжалось порядка 11 часов и указывало на значительные изменения в параметрах термосферы, ответственных за формирование F-области в средних широтах.</p><p>Аномальное образование ночного E-слоя, наблюдаемое на всех ионосферных станциях, обсуждается в рамках физического механизма высыпания энергичных частиц на средних и низких широтах.</p><p>Повышенные значения и wave-like вариации критических частот foF2, наблюдаемые во время фазы восстановления геомагнитной бури, интерпретируются с точки зрения обусловленности их перемещающимися атмосферными возмущениями.</p><p>Событие black out, связанное с полным поглощением зондирующего сигнала, наблюдаемое на станциях в регионе Средней Азии и Дальнего Востока 28 мая, ассоциируется с воздействием на нижнюю ионосферу потока солнечных космических лучей высокой интенсивности, зарегистрированных в этот период.</p><p>Ионосферная буря 25/26 мая может служить моделью отклика ионосферы на экстремальное возмущение магнитного поля Земли.</p></abstract><trans-abstract xml:lang="en"><p>The article presents the results of the study of ionospheric effects of the extreme geomagnetic storm of May 25/26, 1967 (Dst = −387 nT) obtained using ionospheric data measured at five ionospheric stations located in the Central Asian region. The geomagnetic storm with an initial phase lasting approximately 9 hours began at ~20 UT on May 25, which for the region under consideration corresponds to nighttime (at 00:01 LT) on May 26.</p><p>The negative ionospheric disturbance lasting about 28 hours, which began at all stations under consideration during the onset of the main phase of the geomagnetic storm, was characterized by a decrease in the critical frequencies of the ionospheric F2 layer foF2 by 2.2 times compared to the foF2 level under quiet geomagnetic conditions. The “G condition” observed during the negative phase of the ionospheric storm, when foF2 foF1, lasted for about 11 hours and indicated significant changes in the thermospheric parameters responsible for the formation of the F-region in the middle latitudes. The anomalous formation of the nighttime E-layer observed at all ionospheric stations is discussed in the context of the physical mechanism of energetic particle precipitation at middle and low latitudes.</p><p>The increased values and wave-like variations of the critical frequencies of foF2 observed during the recovery phase of the geomagnetic storm are interpreted in terms of their being caused by traveling atmospheric disturbances (TAD).</p><p>The black out event associated with the complete absorption of the sounding signal observed at stations in the Central Asian and Far Eastern regions on May 28 is associated with the impact of the high-intensity solar cosmic ray flux recorded during this period on the lower ionosphere.</p><p>The ionospheric storm of May 25/26 can serve as a model of the ionospheric response to an extreme disturbance of the Earth's magnetic field.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>ионосфера</kwd><kwd>ионосферная буря</kwd><kwd>экстремальная геомагнитная буря</kwd></kwd-group><kwd-group xml:lang="en"><kwd>ionosphere</kwd><kwd>ionospheric storm</kwd><kwd>extreme geomagnetic storm</kwd></kwd-group><funding-group xml:lang="ru"><funding-statement>Данное исследование спонсировано Комитетом науки Министерства науки и высшего образования Республики Казахстан (Грант № BR21882375 «Создание и модернизация изделий космической техники повышенной надежности наземного и космического сегментов и исследование ионосферы»). Особенности локальных геомагнитных вариаций оценивались по данным геомагнитной обсерватории Алма-Ата. Данные по F10.7 загружены с сайта http://www.swpc. noaa.gov. Автор выражает благодарность О. Шкрамада за помощь в обработке материалов архивных ионосферных данных.</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">Gopalswamy, N., Yashiro, S., Michalek, G., Xie, H., Lepping, R. P., and Howard, R. A. Solar source of the largest geomagnetic storm of cycle 23 // Geophys. Res. Lett. – 2005. – Vol. 32. – At. no. L12S09. https://doi.org/10.1029/2004GL021639</mixed-citation><mixed-citation xml:lang="en">Gopalswamy, N., Yashiro, S., Michalek, G., Xie, H., Lepping, R. P., and Howard, R. A. Solar source of the largest geomagnetic storm of cycle 23 // Geophys. Res. Lett. – 2005. – Vol. 32. – At. no. 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