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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">Izvestiya, Atmospheric and Oceanic Physics</journal-id><journal-title-group><journal-title xml:lang="en">Izvestiya, Atmospheric and Oceanic Physics</journal-title><trans-title-group xml:lang="ru"><trans-title>Известия РАН. Физика атмосферы и океана</trans-title></trans-title-group></journal-title-group><issn publication-format="print">0002-3515</issn><issn publication-format="electronic">3034-6487</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">698994</article-id><article-id pub-id-type="doi">10.7868/S3034648725040054</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">AN IMPROVED VERSION OF THE ATMOSPHERIC SULFUR CYCLE SCHEME FOR EARTH SYSTEM MODEL OF INTERMEDIATE COMPLEXITY</article-title><trans-title-group xml:lang="ru"><trans-title>УСОВЕРШЕНСТВОВАННАЯ ВЕРСИЯ СХЕМЫ СЕРНОГО ЦИКЛА АТМОСФЕРЫ ДЛЯ МОДЕЛЕЙ ЗЕМНОЙ СИСТЕМЫ ПРОМЕЖУТОЧНОЙ СЛОЖНОСТИ</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Nyrov</surname><given-names>A. O</given-names></name><name xml:lang="ru"><surname>Ныров</surname><given-names>А. О</given-names></name></name-alternatives><email>andrey.nyro@gmail.com</email><xref ref-type="aff" rid="aff1"/><xref ref-type="aff" rid="aff2"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Eliseev</surname><given-names>A. V</given-names></name><name xml:lang="ru"><surname>Елисеев</surname><given-names>А. В</given-names></name></name-alternatives><xref ref-type="aff" rid="aff1"/><xref ref-type="aff" rid="aff2"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Mokhov</surname><given-names>I. I</given-names></name><name xml:lang="ru"><surname>Мохов</surname><given-names>И. И</given-names></name></name-alternatives><xref ref-type="aff" rid="aff1"/><xref ref-type="aff" rid="aff2"/></contrib></contrib-group><aff-alternatives id="aff1"><aff><institution xml:lang="en">Obukhov Institute of Atmospheric Physics, RAS</institution></aff><aff><institution xml:lang="ru">Институт физики атмосферы им. А.М. Обухова РАН</institution></aff></aff-alternatives><aff-alternatives id="aff2"><aff><institution xml:lang="en">Lomonosov Moscow State University</institution></aff><aff><institution xml:lang="ru">Московский государственный университет им. М.В. Ломоносова</institution></aff></aff-alternatives><pub-date date-type="pub" iso-8601-date="2025-08-15" publication-format="electronic"><day>15</day><month>08</month><year>2025</year></pub-date><volume>61</volume><issue>4</issue><issue-title xml:lang="en">VOL 61, NO4 (2025)</issue-title><issue-title xml:lang="ru">ТОМ 61, №4 (2025)</issue-title><fpage>474</fpage><lpage>486</lpage><history><date date-type="received" iso-8601-date="2025-12-21"><day>21</day><month>12</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><ali:free_to_read xmlns:ali="http://www.niso.org/schemas/ali/1.0/" start_date="2026-08-15"/><license><ali:license_ref xmlns:ali="http://www.niso.org/schemas/ali/1.0/">https://creativecommons.org/licenses/by-nc-nd/4.0</ali:license_ref></license></permissions><self-uri xlink:href="https://journals.eco-vector.com/0002-3515/article/view/698994">https://journals.eco-vector.com/0002-3515/article/view/698994</self-uri><abstract xml:lang="en"><p>The scheme of the atmospheric sulfur cycle ChAP (Chemical and Aerosol Processes), which is developed for Earth system models of intermediate complexity, is extended by taking into account the dimethylsulfide (DMS) emissions into the atmosphere and the differences of the sulfates washout efficiency between different kinds of precipitation. In addition, the transport scheme is slightly revised. To keep the scheme computationally efficient, the new version of the scheme, ChAP–1.1, still employs the stationary approximations and the prescribed vertical profiles for sulfur compounds in the atmosphere (as it was used in ChAP–1.0 as well), which is related to relatively short lifetimes of the sulfur dioxide and sulfates in the troposphere. As a result, the horizontal distributions of the tropospheric sulfur dioxide and sulfates burdens agree better (relative to those for ChAP–1.0) with the reanalysis data CAMS (Copernicus Atmosphere Monitoring Service) and with the ACCMIP (Atmospheric Chemistry and Climate Model Intercomparison Project) data for the late 20th–early 21st centuries. According to the ChAP–1.1 simulations, the global sulfur dioxide burden in the atmosphere in 1990–2000 is 0.2 TgS, and the respective value for sulfates is 0.6–0.7 TgS with the corresponding lifetimes 1 day and 6 days.</p></abstract><trans-abstract xml:lang="ru"><p>Схема серного цикла атмосферы ChAP (Chemical and Aerosol Processes) для моделей Земной системы промежуточной сложности расширена учетом диметилсульфида (ДМС) и влияния типа осадков на интенсивность выведения сульфатов из атмосферы. Наряду с этим, изменена численная схема переноса примесей. Для сохранения вычислительной эффективности предлагаемой новой модельной версии ChAP−1.1 использовалось приближение стационарности с предписанными вертикальными профилями для концентраций соединений серы в атмосфере (как и в предыдущей версии ChAP−1.0), что связано с относительно малым временем жизни диоксида серы и сульфатов в тропосфере. В результате улучшено согласие пространственного распределения сернистого газа и сульфатов с данными рсанализа CAMS (Copernicus Atmosphere Monitoring Service), проекта ACCMIP (Atmospheric Chemistry and Climate Model Intercomparison Project) для конца XX — начала XXI в. По расчетам с новой версией ChAP−1.1 глобальное содержание сернистого газа в атмосфере в 1990–2000 гг. составляет 0.2 TrS, сульфатов — 0.6–0.7 TrS при их характерном времени жизни 1 и 6 сут соответственно.</p></trans-abstract><kwd-group xml:lang="en"><kwd>atmospheric chemistry</kwd><kwd>models of intermediate complexity</kwd><kwd>sulfur cycle</kwd><kwd>sulfates</kwd><kwd>sulfur dioxide</kwd><kwd>dimethylsulfide</kwd></kwd-group><kwd-group xml:lang="ru"><kwd>химия атмосферы</kwd><kwd>модели промежуточной сложности</kwd><kwd>цикл серы</kwd><kwd>сульфаты</kwd><kwd>диоксид серы</kwd><kwd>диметилсульфид</kwd></kwd-group><funding-group><funding-statement xml:lang="ru">Разработка схемы ChAP–1.1 поддержана государственным заданием ИФА им. А.М. Обухова РАН (проект FMWR-2022-0014) и в соответствии с общей тематикой проекта РНФ 24-17-00211.</funding-statement></funding-group></article-meta></front><body></body><back><ref-list><ref id="B1"><label>1.</label><mixed-citation>Елисеев А.В. 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