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<article 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" xmlns:ali="http://www.niso.org/schemas/ali/1.0/" article-type="research-article" dtd-version="1.2" xml:lang="en"><front><journal-meta><journal-id journal-id-type="publisher-id">Cosmic Research</journal-id><journal-title-group><journal-title xml:lang="en">Cosmic Research</journal-title><trans-title-group xml:lang="ru"><trans-title>Космические исследования</trans-title></trans-title-group></journal-title-group><issn publication-format="print">0023-4206</issn><issn publication-format="electronic">3034-5502</issn><publisher><publisher-name xml:lang="en">The Russian Academy of Sciences</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="publisher-id">682921</article-id><article-id pub-id-type="doi">10.31857/S0023420625010013</article-id><article-id pub-id-type="edn">HEXAMV</article-id><article-categories><subj-group subj-group-type="toc-heading" xml:lang="en"><subject>Articles</subject></subj-group><subj-group subj-group-type="toc-heading" xml:lang="ru"><subject>Статьи</subject></subj-group><subj-group subj-group-type="article-type"><subject>Research Article</subject></subj-group></article-categories><title-group><article-title xml:lang="en">Comparison of the results of theoretical calculations of night glow intensity with measurement data obtained by both ground-based methods and from space shuttles</article-title><trans-title-group xml:lang="ru"><trans-title>Сопоставление результатов теоретических расчетов интенсивности ночного свечения с данными измерений, полученными как наземными методами, так и с космических шаттлов</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Antonenko</surname><given-names>O. V.</given-names></name><name xml:lang="ru"><surname>Антоненко</surname><given-names>О. В.</given-names></name></name-alternatives><address><country country="RU">Russian Federation</country></address><email>antonenko@pgia.ru</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Kirillov</surname><given-names>A. S.</given-names></name><name xml:lang="ru"><surname>Кириллов</surname><given-names>А. С.</given-names></name></name-alternatives><address><country country="RU">Russian Federation</country></address><email>antonenko@pgia.ru</email><xref ref-type="aff" rid="aff1"/></contrib></contrib-group><aff-alternatives id="aff1"><aff><institution xml:lang="en">Polar Geophysical Institute (PGI)</institution></aff><aff><institution xml:lang="ru">Полярный геофизический институт (ПГИ)</institution></aff></aff-alternatives><pub-date date-type="pub" iso-8601-date="2025-01-15" publication-format="electronic"><day>15</day><month>01</month><year>2025</year></pub-date><volume>63</volume><issue>1</issue><fpage>3</fpage><lpage>12</lpage><history><date date-type="received" iso-8601-date="2025-06-05"><day>05</day><month>06</month><year>2025</year></date></history><permissions><copyright-statement xml:lang="en">Copyright ©; 2025, Russian Academy of Sciences</copyright-statement><copyright-statement xml:lang="ru">Copyright ©; 2025, Российская академия наук</copyright-statement><copyright-year>2025</copyright-year><copyright-holder xml:lang="en">Russian Academy of Sciences</copyright-holder><copyright-holder xml:lang="ru">Российская академия наук</copyright-holder></permissions><self-uri xlink:href="https://journals.eco-vector.com/0023-4206/article/view/682921">https://journals.eco-vector.com/0023-4206/article/view/682921</self-uri><abstract xml:lang="en"><p>The integral luminosity values of the Herzberg I, Chamberlain and Atmospheric bands at mid-latitudes and in the equatorial zone of the Earth are calculated. The correlation of the results of theoretical calculations of the intensity of excited molecular oxygen glow on Earth with experimental data on the night glow of O<sub>2</sub> obtained from space shuttles, from the ground-based Kitt Peak Observatory (USA) for the Herzberg I and Chamberlain bands is discussed. For the Atmospheric bands, the correlation of the results of theoretical calculations with similar calculations based on measurement data from the ground-based Keck Observatory (USA) is analyzed. The integral luminosity values of the Herzberg I and Atmospheric bands for the northern latitudes of Mars are calculated.</p></abstract><trans-abstract xml:lang="ru"><p>Рассчитаны значения интегральной светимости полос Герцберга I, Чемберлена и Атмосферных полос на средних широтах и в экваториальной зоне Земли. Обсуждается корреляция результатов теоретических расчетов интенсивности свечения возбужденного молекулярного кислорода на Земле с экспериментальными данными по ночному свечению О<sub>2 </sub>, полученными с космических шаттлов, с наземной обсерватории Китт-Пик (США) для полос Герцберга I, Чемберлена. Для Атмосферных полос анализируется корреляция результатов теоретических расчетов с аналогичными расчетами по данным измерений с наземной обсерватории Кека (США). Рассчитаны значения интегральной светимости полос и Атмосферных полос для северных широт Марса.</p></trans-abstract><funding-group/></article-meta></front><body></body><back><ref-list><ref id="B1"><label>1.</label><mixed-citation>Шефов Н.Н., Семенов А.И., Хомич В.Ю. Излучение верхней атмосферы – индикатор ее структуры и динамики. М.: ГЕОС, 2006. 741 с.</mixed-citation></ref><ref id="B2"><label>2.</label><mixed-citation>Newcomb S. Is the Airship Coming? // McClure’s magazine. 1901. V. 17(5). 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