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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">Himičeskaâ fizika</journal-id><journal-title-group><journal-title xml:lang="en">Himičeskaâ fizika</journal-title><trans-title-group xml:lang="ru"><trans-title>Химическая физика</trans-title></trans-title-group></journal-title-group><issn publication-format="print">0207-401X</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">689003</article-id><article-id pub-id-type="doi">10.31857/S0207401X25080071</article-id><article-categories><subj-group subj-group-type="toc-heading" xml:lang="en"><subject>Combustion, explosion and shock waves</subject></subj-group><subj-group subj-group-type="toc-heading" xml:lang="ru"><subject>Горение, взрыв и ударные волны</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">Kinetic features of non-thermal plasma conversion of propane-air mixture at high pressure</article-title><trans-title-group xml:lang="ru"><trans-title>Кинетические особенности нетермической плазменной конверсии пропано-воздушной смеси при повышенном давлении</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Filimonova</surname><given-names>E. A.</given-names></name><name xml:lang="ru"><surname>Филимонова</surname><given-names>Е. А.</given-names></name></name-alternatives><address><country country="RU">Russian Federation</country></address><email>helfil@mail.ru</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Selivonin</surname><given-names>I. V.</given-names></name><name xml:lang="ru"><surname>Селивонин</surname><given-names>И. В.</given-names></name></name-alternatives><address><country country="RU">Russian Federation</country></address><email>helfil@mail.ru</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Moralev</surname><given-names>I. A.</given-names></name><name xml:lang="ru"><surname>Моралев</surname><given-names>И. А.</given-names></name></name-alternatives><address><country country="RU">Russian Federation</country></address><email>helfil@mail.ru</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Dobrovolskaya</surname><given-names>A. S.</given-names></name><name xml:lang="ru"><surname>Добровольская</surname><given-names>А. С.</given-names></name></name-alternatives><address><country country="RU">Russian Federation</country></address><email>helfil@mail.ru</email><xref ref-type="aff" rid="aff1"/></contrib></contrib-group><aff-alternatives id="aff1"><aff><institution xml:lang="en">Joint Institute for High Temperatures, Russian Academy of Sciences</institution></aff><aff><institution xml:lang="ru">Объединенный институт высоких температур Российской академии наук</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>44</volume><issue>8</issue><issue-title xml:lang="en"/><issue-title xml:lang="ru"/><fpage>64</fpage><lpage>80</lpage><history><date date-type="received" iso-8601-date="2025-08-11"><day>11</day><month>08</month><year>2025</year></date><date date-type="accepted" iso-8601-date="2025-08-11"><day>11</day><month>08</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://transsyst.ru/0207-401X/article/view/689003">https://transsyst.ru/0207-401X/article/view/689003</self-uri><abstract xml:lang="en"><p>The paper presents the results of modeling the conversion of a lean non-combustible propane-air mixture with initiation by a high-frequency corona discharge at a pressure of 5 bar and an initial temperature of 300 K for different equivalence ratios. The discharge creates non-thermal plasma in filament channels. Experiments on the development of such a discharge in air for different conditions were carried out. At pressures of 1 and 2 bar, the discharge has a complex morphology with branching of discharge filaments. At pressures above 3 bar, the glow region has the shape of a straight spoke. The paper presents a kinetic analysis of the conversion. The key component for propane decomposition is the O atom produced in the discharge as a result of O<sub>2</sub> dissociation by direct electron impact and excited N<sub>2</sub> molecules. In the afterglow, after completion of discharge, the source of the O atom is the reactions of ozone decomposition with N<sub>2</sub> and O<sub>2</sub>. For the formation of NO, it is necessary to take into account the production of N atoms in the excited and ground states. Intermediate oxidized hydrocarbons play a major role in increasing the concentrations of C<sub>3</sub>H<sub>6</sub>, C<sub>2</sub>H<sub>4</sub>, and CO over time. The decomposition of O<sub>3</sub> occurs to a greater extent in a cycle involving NO<sub>3</sub>. The heating of the discharge-activated zone did not exceed 600 K. The composition of the conversion products obtained as a result of modeling was compared with known experimental literature data.</p></abstract><trans-abstract xml:lang="ru"><p>В работе представлены результаты моделирования процесса конверсии бедной негорючей пропановоздушной смеси с инициацией высокочастотным коронным разрядом при давлении 5 бар и начальной температуре 300 К для разных коэффициентов избытка топлива. Разряд создает нетермическую плазму в каналах-филаментах. Проведены эксперименты развития такого разряда в воздухе для разных условий. При давлениях 1 и 2 бар разряд имеет сложную морфологию с ветвлением разрядных филаментов. При давлениях выше 3 бар область свечения имеет форму прямой спицы. В работе приведен кинетический анализ конверсии. Ключевым компонентом для разложения пропана является атом О, наработанный в разряде в результате диссоциации О<sub>2</sub> прямым электронным ударом и возбужденными молекулами N<sub>2</sub>. В послесвечении, после завершения разряда, источником атома О являются реакции разложения озона с N<sub>2</sub> и O<sub>2</sub>. Для образования NO необходимо учитывать наработку атомов N в возбужденном и основном состояниях. Большую роль в увеличении концентраций C<sub>3</sub>H<sub>6</sub>, C<sub>2</sub>H<sub>4</sub>, CO со временем играют промежуточные окисленные углеводороды. Разложение О<sub>3</sub> происходит в большей степени в цикле с участием NO<sub>3</sub>. Нагрев активированной разрядом зоны не превышал 600 К. Состав продуктов конверсии, полученный в результате моделирования, сравнивался с известными литературными экспериментальными данными.</p></trans-abstract><kwd-group xml:lang="en"><kwd>plasma chemical conversion</kwd><kwd>propane</kwd><kwd>kinetic analysis</kwd><kwd>high-frequency corona discharge</kwd><kwd>modeling</kwd><kwd>experiment</kwd></kwd-group><kwd-group xml:lang="ru"><kwd>плазмохимическая конверсия</kwd><kwd>пропан</kwd><kwd>кинетический анализ</kwd><kwd>высокочастотный коронный разряд</kwd><kwd>моделирование</kwd><kwd>эксперимент</kwd></kwd-group><funding-group><award-group><funding-source><institution-wrap><institution xml:lang="ru">Российский Научный Фонд</institution></institution-wrap><institution-wrap><institution xml:lang="en">Russian Science Foundation</institution></institution-wrap></funding-source><award-id>24-29-00791</award-id></award-group></funding-group></article-meta></front><body></body><back><ref-list><ref id="B1"><label>1.</label><mixed-citation>Bellenoue M., Labuda S., Ruttun B., Sotton J. // Combust. 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