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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">zhps</journal-id><journal-title-group><journal-title xml:lang="ru">Журнал прикладной спектроскопии</journal-title><trans-title-group xml:lang="en"><trans-title>Zhurnal Prikladnoii Spektroskopii</trans-title></trans-title-group></journal-title-group><issn pub-type="ppub">0514-7506</issn><publisher><publisher-name>B. I. Stepanov Institute of Physics of the National Academy of Sciences</publisher-name></publisher></journal-meta><article-meta><article-id custom-type="elpub" pub-id-type="custom">zhps-218</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>ТЕОРЕТИЧЕСКИЕ МОДЕЛИ МИКРОВОЛНОВЫХ ВРАЩАТЕЛЬНЫХ СПЕКТРОВ НИЗКОГО РАЗРЕШЕНИЯ МОЛЕКУЛ ЭТАНИ ПРОПАНТИОЛА</article-title><trans-title-group xml:lang="en"><trans-title>THEORETICAL MODELS OF THE LOW RESOLUTION MICROWAVE ROTATIONAL SPECTRA OF ETHANETHIOL AND PROPANETHIOL MOLECULES</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>Каджар</surname><given-names>Ч. О.</given-names></name><name name-style="western" xml:lang="en"><surname>Kadjar</surname><given-names>Ch. O.</given-names></name></name-alternatives><email xlink:type="simple">noemail@neicon.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>Казымова</surname><given-names>С. Б.</given-names></name><name name-style="western" xml:lang="en"><surname>Kazimova</surname><given-names>S. B.</given-names></name></name-alternatives><email xlink:type="simple">noemail@neicon.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>Гасанова</surname><given-names>А. С.</given-names></name><name name-style="western" xml:lang="en"><surname>Hasanova</surname><given-names>A. S.</given-names></name></name-alternatives><email xlink:type="simple">noemail@neicon.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>Исмаилзаде</surname><given-names>Г. И.</given-names></name><name name-style="western" xml:lang="en"><surname>Ismailzadeh</surname><given-names>G. I.</given-names></name></name-alternatives><email xlink:type="simple">noemail@neicon.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>Мензелеев</surname><given-names>М. Р.</given-names></name><name name-style="western" xml:lang="en"><surname>Menzeleyev</surname><given-names>M. R.</given-names></name></name-alternatives><email xlink:type="simple">mmenzeleyev@gmail.com</email><xref ref-type="aff" rid="aff-1"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru"><institution>Институт физики НАН Азербайджана</institution></aff><aff xml:lang="en"><institution>Institute of Physics, Azerbaijan National Academy of Sciences</institution></aff></aff-alternatives><pub-date pub-type="collection"><year>2018</year></pub-date><pub-date pub-type="epub"><day>10</day><month>03</month><year>2020</year></pub-date><volume>85</volume><issue>2</issue><fpage>194</fpage><lpage>198</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Каджар Ч.О., Казымова С.Б., Гасанова А.С., Исмаилзаде Г.И., Мензелеев М.Р., 2020</copyright-statement><copyright-year>2020</copyright-year><copyright-holder xml:lang="ru">Каджар Ч.О., Казымова С.Б., Гасанова А.С., Исмаилзаде Г.И., Мензелеев М.Р.</copyright-holder><copyright-holder xml:lang="en">Kadjar C.O., Kazimova S.B., Hasanova A.S., Ismailzadeh G.I., Menzeleyev M.R.</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://zhps.ejournal.by/jour/article/view/218">https://zhps.ejournal.by/jour/article/view/218</self-uri><abstract><p>Методом аддитивного моделирования микроволновых спектров низкого разрешения гетероизомерных молекул замещенных углеводородов получены теоретические спектры молекул этан- и пропантиолов в диапазоне 0-2 ТГц с максимумами 465±20 и 240±20 ГГц. Проведены уточняющие расчеты в узкой полосе частот указанных диапазонов с использованием полуширин спектральной линии 1.5, 0.8 и 0.5 МГц, моделирующих условия, характерные для соответствующих слоев тропосферы Земли. Выделены наиболее интенсивные экстремумы спектров низкого разрешения исследуемых молекул: 486±5, 446±5, 436±5 (этантиол) и 257±5, 239±5, 234±5 ГГц (пропантиол). Обсуждаются различные аспекты практического использования полученных результатов.</p></abstract><trans-abstract xml:lang="en"><p>Within the framework of the method of additive modeling of the low resolution microwave spectra of the heteroisomeric molecules of substituted hydrocarbons, the theoretical models of low resolution microwave spectra of ethanethiol and propanethiol molecules were produced for the 0-2 THz frequency range with spectral maximums at 465±20 and 240±20 GHz, respectively. More precise calculations at the narrow frequency band of the above-mentioned frequency ranges were provided using the spectral line half-width values 1.5, 0.8, and 0.5 МHz, modeling the conditions of different layers of the Earth’s troposphere. This permitted to specify the most intensive generating extrema of the low resolution spectra of the investigated species of ethanethiol and propanethiol as 486±5, 446±5, 436±5 and 257±5, 239±5, 234±5 GHz, respectively. The different aspects of the application of the obtained results were discussed. </p></trans-abstract><kwd-group xml:lang="ru"><kwd>микроволновый спектр</kwd><kwd>спектр низкого разрешения</kwd><kwd>этантиол</kwd><kwd>пропантиол</kwd><kwd>microwave spectra</kwd><kwd>low resolution spectra</kwd><kwd>ethanethiol and propanethiol</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">К. Н. Зеленин. Соросов. образоват. журн., № 4 (1998) 39-44</mixed-citation><mixed-citation xml:lang="en">К. Н. Зеленин. Соросов. образоват. журн., № 4 (1998) 39-44</mixed-citation></citation-alternatives></ref><ref id="cit2"><label>2</label><citation-alternatives><mixed-citation xml:lang="ru">О. В. Никитин. Контроль источников загрязнения атмосферного воздуха, Казань, Казан. ун-т (2014)</mixed-citation><mixed-citation xml:lang="en">О. В. Никитин. Контроль источников загрязнения атмосферного воздуха, Казань, Казан. ун-т (2014)</mixed-citation></citation-alternatives></ref><ref id="cit3"><label>3</label><citation-alternatives><mixed-citation xml:lang="ru">Ч. О. Каджар, Г. И. Исмаилзаде, М. Р. Мензелеев, И. З. Мовсумов, С. Б. Казымова. Журн. прикл. спектр., 83 (2016) 385-389 [Ch. O. Kadjar, G. I. Ismailzadeh, M. R. Menzeleyev, I. Z. Movsumov, S. B. Kazimova. J. Appl. Spectr., 83 (2016) 379-382]</mixed-citation><mixed-citation xml:lang="en">Ч. О. Каджар, Г. И. Исмаилзаде, М. Р. Мензелеев, И. З. Мовсумов, С. Б. Казымова. Журн. прикл. спектр., 83 (2016) 385-389 [Ch. O. Kadjar, G. I. Ismailzadeh, M. R. Menzeleyev, I. Z. Movsumov, S. B. Kazimova. J. Appl. Spectr., 83 (2016) 379-382]</mixed-citation></citation-alternatives></ref><ref id="cit4"><label>4</label><citation-alternatives><mixed-citation xml:lang="ru">L. Kolesnikova, B. Tercero, J. Cernicharo, J. L. Alonso, A. M. Daly, B. P. Gordon, S. T. Shipman. Am. Astronom. Soc. Astrophys. J. Lett., 784, N 1 (2014) 1-16</mixed-citation><mixed-citation xml:lang="en">L. Kolesnikova, B. Tercero, J. Cernicharo, J. L. Alonso, A. M. Daly, B. P. Gordon, S. T. Shipman. Am. Astronom. Soc. Astrophys. J. Lett., 784, N 1 (2014) 1-16</mixed-citation></citation-alternatives></ref><ref id="cit5"><label>5</label><citation-alternatives><mixed-citation xml:lang="ru">J. Nakagawa, M. Hayashi. J. Mol. Spectr., 85 (1981) 327-340</mixed-citation><mixed-citation xml:lang="en">J. Nakagawa, M. Hayashi. J. Mol. Spectr., 85 (1981) 327-340</mixed-citation></citation-alternatives></ref></ref-list><fn-group><fn fn-type="conflict"><p>The authors declare that there are no conflicts of interest present.</p></fn></fn-group></back></article>
