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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">dpg</journal-id><journal-title-group><journal-title xml:lang="ru">Динамические процессы в геосферах</journal-title><trans-title-group xml:lang="en"><trans-title>Dynamic Processes in Geospheres</trans-title></trans-title-group></journal-title-group><issn pub-type="ppub">2222-8535</issn><issn pub-type="epub">2949-0995</issn><publisher><publisher-name>IDG RAS</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.26006/29490995_2022_14_2_115</article-id><article-id custom-type="elpub" pub-id-type="custom">dpg-100</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>ПРИБОРНО-МЕТОДИЧЕСКИЕ ИССЛЕДОВАНИЯ</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>INSTRUMENT AND METHODOLOGICAL STUDIES</subject></subj-group></article-categories><title-group><article-title>ИОНОСФЕРНАЯ АНТЕННА БЕГУЩЕЙ ВОЛНЫ, ФОРМИРУЕМАЯ КВ ИНТЕРФЕРОМЕТРОМ С ПРОИЗВОЛЬНЫМ УГЛОМ НАКЛОНА ГЛАВНОГО ЛУЧА</article-title><trans-title-group xml:lang="en"><trans-title>IONOSPHERIC TRAVELING WAVE ANTENNA FORMED BY RF  INTERFEROMETER WITH AN ARBITRARY ANGLE OF TILT  OF THE MAIN BEAM</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-2121-9728</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Котик</surname><given-names>Д. С.</given-names></name><name name-style="western" xml:lang="en"><surname>Kotik</surname><given-names>D. S.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Ведущий научный сотрудник.</p><p>7432-6984</p><p> </p></bio><email xlink:type="simple">dmitry.kotik@nirfi.unn.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/0000-0002-6080-847X</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Яшнов</surname><given-names>В. А.</given-names></name><name name-style="western" xml:lang="en"><surname>Yashnov</surname><given-names>V. A.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Доцент, Радиофизический факультет</p></bio><email xlink:type="simple">vayashnov@rambler.ru</email><xref ref-type="aff" rid="aff-2"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru">Нижегородский государственный университет имени Н. И. Лобачевского,  Научно-исследовательский радиофизический институт, Нижний Новгород,<country>Россия</country></aff><aff xml:lang="en">National Research Nizhny Novgorod State University named after N.I. Lobachevsky<country>Russian Federation</country></aff></aff-alternatives><aff-alternatives id="aff-2"><aff xml:lang="ru">Нижегородский государственный университет имени Н. И. Лобачевского<country>Россия</country></aff><aff xml:lang="en">National Research Nizhny Novgorod State University named after N.I. Lobachevsky<country>Russian Federation</country></aff></aff-alternatives><pub-date pub-type="collection"><year>2022</year></pub-date><pub-date pub-type="epub"><day>26</day><month>12</month><year>2022</year></pub-date><volume>14</volume><issue>2</issue><fpage>115</fpage><lpage>121</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Котик Д.С., Яшнов В.А., 2022</copyright-statement><copyright-year>2022</copyright-year><copyright-holder xml:lang="ru">Котик Д.С., Яшнов В.А.</copyright-holder><copyright-holder xml:lang="en">Kotik D.S., Yashnov V.A.</copyright-holder><license 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://www.dyngeo.ru/jour/article/view/100">https://www.dyngeo.ru/jour/article/view/100</self-uri><abstract><p>В проведенных нами экспериментах по формированию в ионосфере движущегося источника типа антенны бегущей волны использовались два мощных радиопередатчика стенда СУРА с несущими частотами, отстроенными на частоту F в ОНЧ диапазоне [Котик и др., 1994]. Каждый из них в качестве излучателя использовал треть антенной решётки стенда с вертикальной диаграммой направленности. В работе рассмотрен более общий случай при излучении КВ волн антенными решетками с произвольным углом наклона главного луча. Показано, что частота F сильно зависит от направления главного луча и может изменяться в широких пределах от единиц до полутора десятков килогерц. При этом возможно согласование скорости волны тока ионосферного источника с фазовой скоростью первых мод волновода Земля-ионосфера.</p></abstract><trans-abstract xml:lang="en"><p>It was previously shown that when using two powerful transmitters operating on two antenna arrays with a vertical radiation pattern, the phase centers of which are separated by a distance d with a carrier frequency spacing a moving source of low-frequency radiation appears in the lower ionosphere. The phase velocity of such traveling wave antenna coincides with the phase velocity of the main mode of the Earth-ionosphere waveguide at the frequency (F is the carrier frequency difference; h is the height of the ionospheric source above the Earth's surface). At this frequency, a maximum in the radiation amplitude is observed in the experiment. The paper considers a more general case when a HF interferometer operates with an arbitrary angle of inclination of the main beam of both emitters. It is shown that the frequency F strongly depends on the direction of the main beam and can vary over a wide range from units to 15 kilohertz. In this case, it is possible to match the velocity of the current wave in the source with the phase velocity of several first modes of the waveguide. In this case, it is possible to match the current wave of the source with the phase velocity of several first modes of the waveguide. It is shown that the frequency F strongly depends on the direction of the main beam and can vary over a wide range from units to 15 kilohertz. In this case, it is possible to match the velocity of the current wave in the source with the phase velocity of several first modes of the waveguide. We note that so far no experimental verification has been carried out in this formulation, although the technical capabilities of modern heating facilities allow such experiments to be carried out.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>ионосфера</kwd><kwd>нагревный передатчик</kwd><kwd>движущийся источник</kwd><kwd>низкочастотное радиоизлучение</kwd><kwd>волновод Земля-ионосфера</kwd></kwd-group><kwd-group xml:lang="en"><kwd>ionosphere</kwd><kwd>heating transmitter</kwd><kwd>moving source</kwd><kwd>low-frequency radio emission</kwd><kwd>Earth</kwd><kwd>ionosphere waveguide</kwd></kwd-group><funding-group xml:lang="ru"><funding-statement>Дмитрий Котик, ННГУ - проект № 0729-2020-0057 базовой части Государственного задания Министерства науки; Владимир Яшнов, ННГУ - РНФ № 20-12-00197</funding-statement></funding-group></article-meta></front><back><ref-list><title>References</title></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>
