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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="other" 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">672565</article-id><article-id pub-id-type="doi">10.31857/S0023420623600204</article-id><article-id pub-id-type="edn">CFXKDA</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>Unknown</subject></subj-group></article-categories><title-group><article-title xml:lang="en">Features of Narrowband Stimulated Electromagnetic Emission Depending on the Effective Radiated Power of the EISCAT/Heating Facility</article-title><trans-title-group xml:lang="ru"><trans-title>Характеристики узкополосного искусственного радиоизлучения ионосферы в зависимости от эффективной мощности излучения нагревного стенда EISCAT/Heating</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Kalishin</surname><given-names>A. S.</given-names></name><name xml:lang="ru"><surname>Калишин</surname><given-names>А. С.</given-names></name></name-alternatives><email>askalishin@aari.ru</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Blagoveshchenskaya</surname><given-names>N. F.</given-names></name><name xml:lang="ru"><surname>Благовещенская</surname><given-names>Н. Ф.</given-names></name></name-alternatives><email>askalishin@aari.ru</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Borisova</surname><given-names>T D.</given-names></name><name xml:lang="ru"><surname>Борисова</surname><given-names>Т. Д.</given-names></name></name-alternatives><email>askalishin@aari.ru</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Egorov</surname><given-names>I. M.</given-names></name><name xml:lang="ru"><surname>Егоров</surname><given-names>И. М.</given-names></name></name-alternatives><email>askalishin@aari.ru</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Zagorskiy</surname><given-names>G. A.</given-names></name><name xml:lang="ru"><surname>Загорский</surname><given-names>Г. А.</given-names></name></name-alternatives><email>askalishin@aari.ru</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Kovalev</surname><given-names>A. S.</given-names></name><name xml:lang="ru"><surname>Ковалев</surname><given-names>А. С.</given-names></name></name-alternatives><email>askalishin@aari.ru</email><xref ref-type="aff" rid="aff1"/></contrib></contrib-group><aff-alternatives id="aff1"><aff><institution xml:lang="en">Arctic and Antarctic Research Institute, 199397, St. Petersburg, Russia</institution></aff><aff><institution xml:lang="ru">Арктический и антарктический научно-исследовательский институт</institution></aff></aff-alternatives><pub-date date-type="pub" iso-8601-date="2023-11-01" publication-format="electronic"><day>01</day><month>11</month><year>2023</year></pub-date><volume>61</volume><issue>6</issue><fpage>476</fpage><lpage>485</lpage><history><date date-type="received" iso-8601-date="2025-02-27"><day>27</day><month>02</month><year>2025</year></date></history><permissions><copyright-statement xml:lang="en">Copyright ©; 2023, А.С. Калишин, Н.Ф. Благовещенская, Т.Д. Борисова, И.М. Егоров, Г.А. Загорский, А.С. Ковалев</copyright-statement><copyright-statement xml:lang="ru">Copyright ©; 2023, А.С. Калишин, Н.Ф. Благовещенская, Т.Д. Борисова, И.М. Егоров, Г.А. Загорский, А.С. Ковалев</copyright-statement><copyright-year>2023</copyright-year><copyright-holder xml:lang="en">А.С. Калишин, Н.Ф. Благовещенская, Т.Д. Борисова, И.М. Егоров, Г.А. Загорский, А.С. Ковалев</copyright-holder><copyright-holder xml:lang="ru">А.С. Калишин, Н.Ф. Благовещенская, Т.Д. Борисова, И.М. Егоров, Г.А. Загорский, А.С. Ковалев</copyright-holder></permissions><self-uri xlink:href="https://journals.eco-vector.com/0023-4206/article/view/672565">https://journals.eco-vector.com/0023-4206/article/view/672565</self-uri><abstract xml:lang="en"><p>Estimates of excitation thresholds and the analysis of spectral features of narrowband stimulated electromagnetic emission (NSEE) depending on the electric-field intensity of an extraordinary polarized HF pump wave have been carried out. They are based on results obtained during power stepping EISCAT/Heating experiments. The HF pump wave was radiated toward the magnetic zenith at frequency of 5.423 MHz. The effective radiated power was changed from 55 to 360 MW. NSEE was recorded in the vicinity of St. Petersburg at a distance of ~1200 km away of the EISCAT/Heating facility. Calculations of the electric field of a powerful HF radio wave near the reflection altitude taking into account the nondeviation absorption in the underlying layers were performed. The threshold (minimum) values of the electric field required for the NSEE excitation were determined.</p></abstract><trans-abstract xml:lang="ru"><p id="idm45257552027552">По данным экспериментов на нагревном стенде EISCAT/Heating при ступенчатом изменении эффективной мощности излучения выполнена оценка порогов возбуждения и анализ зависимости спектральных характеристик узкополосного искусственного радиоизлучения ионосферы (УИРИ) от напряженности электрического поля мощной радиоволны КВ-диапазона (волны накачки) необыкновенной поляризации (<italic>Х</italic>-мода). Волны накачки излучались в направлении магнитного зенита на частоте 5.423 МГц. Эффективная мощность излучаемой волны изменялась от 55 до 360 МВт. УИРИ регистрировалось на научно-исследовательской станции под Санкт-Петербургом на расстоянии ∼1200 км от нагревного стенда. Выполнены расчеты напряженности электрического поля мощного КВ-излучения вблизи высоты отражения с учетом неотклоняющего поглощения на пути распространения. Определены пороговые (минимальные) значения электрического поля, необходимые для возбуждения УИРИ.</p></trans-abstract><funding-group/></article-meta></front><body></body><back><ref-list><ref id="B1"><label>1.</label><mixed-citation>Thidé B., Kopka H., Stubbe P. Observations of stimulated scattering of a strong high frequency radio wave in the ionosphere // Physics Review Lett. 1982. V. 49. P. 1561–1564. https://doi.org/10.1103/physrevlett.49.1561</mixed-citation></ref><ref id="B2"><label>2.</label><mixed-citation>Frolov V.L., Sergeev E.N., Ermakova G.P. et al. Spectral features of stimulated electromagnetic emissions, measured in the 4.3–9.5 MHz pump wave frequency range // Geophys. Res. Lett. 2001. V. 28. P. 3103–3106.</mixed-citation></ref><ref id="B3"><label>3.</label><mixed-citation>Leyser T.B. 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