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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_2023_15_3_54</article-id><article-id custom-type="elpub" pub-id-type="custom">dpg-159</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>ЭЛЕКТРОДИНАМИЧЕСКИЕ ПРОЦЕССЫ В ГЕОСФЕРАХ</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>ELECTRODYNAMIC PROCESSES IN GEOSPHERES</subject></subj-group></article-categories><title-group><article-title>ОЦЕНКА ПАРАМЕТРОВ НИЖНЕЙ ИОНОСФЕРЫ ВО ВРЕМЯ РЕНТГЕНОВСКИХ ВСПЫШЕК НА ТРАССАХ РАСПРОСТРАНЕНИЯ СИГНАЛОВ СДВ ДИАПАЗОНА, ПРИНЯТЫХ В ОБСЕРВАТОРИЯХ «МИХНЕВО» И «УЛЬЯНОВКА»</article-title><trans-title-group xml:lang="en"><trans-title>ESTIMATION OF THE PARAMETERS OF THE LOWER IONOSPHERE DURING X-RAY FLARES ON THE PROPAGATION PATHS OF VLF SIGNALS RECEIVED AT THE MIKHNEVO AND UL’YANOVKA OBSERVATORIES</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-1955-4914</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Поклад</surname><given-names>Ю. В.</given-names></name><name name-style="western" xml:lang="en"><surname>Poklad</surname><given-names>Yu. V.</given-names></name></name-alternatives><email xlink:type="simple">poklad@mail.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>Бессараб</surname><given-names>Ф. С.</given-names></name><name name-style="western" xml:lang="en"><surname>Bessarab</surname><given-names>F. S.</given-names></name></name-alternatives><xref ref-type="aff" rid="aff-2"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-7921-0371</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Гаврилов</surname><given-names>Б. Г.</given-names></name><name name-style="western" xml:lang="en"><surname>Gavrilov</surname><given-names>B. G.</given-names></name></name-alternatives><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0003-3421-9046</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Ермак</surname><given-names>В. М.</given-names></name><name name-style="western" xml:lang="en"><surname>Ermak</surname><given-names>V. M.</given-names></name></name-alternatives><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0003-4975-4164</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Ряховский</surname><given-names>И. А.</given-names></name><name name-style="western" xml:lang="en"><surname>Ryakhovskiy</surname><given-names>I. A.</given-names></name></name-alternatives><xref ref-type="aff" rid="aff-1"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru">Институт динамики геосфер имени академика М. А. Садовского РАН<country>Россия</country></aff><aff xml:lang="en">Sadovsky Institute of Geospheres Dynamics of Russian Academy of Sciences<country>Russian Federation</country></aff></aff-alternatives><aff-alternatives id="aff-2"><aff xml:lang="ru">Институт земного магнетизма, ионосферы и распространения радиоволн им. Н. В. Пушкова РАН Калининградский филиал<country>Россия</country></aff><aff xml:lang="en">Kaliningrad branch of Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of Russian Academy of Sciences<country>Russian Federation</country></aff></aff-alternatives><pub-date pub-type="collection"><year>2023</year></pub-date><pub-date pub-type="epub"><day>29</day><month>11</month><year>2023</year></pub-date><volume>15</volume><issue>3</issue><fpage>54</fpage><lpage>61</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Поклад Ю.В., Бессараб Ф.С., Гаврилов Б.Г., Ермак В.М., Ряховский И.А., 2023</copyright-statement><copyright-year>2023</copyright-year><copyright-holder xml:lang="ru">Поклад Ю.В., Бессараб Ф.С., Гаврилов Б.Г., Ермак В.М., Ряховский И.А.</copyright-holder><copyright-holder xml:lang="en">Poklad Y.V., Bessarab F.S., Gavrilov B.G., Ermak V.M., Ryakhovskiy I.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/159">https://www.dyngeo.ru/jour/article/view/159</self-uri><abstract><p>В работе проводится сравнительный анализ восстановленных ионосферных параметров по данным приема СДВ сигналов в геофизических обсерваториях (ГФО) «Михнево» ИДГ РАН и «Ульяновка» (Калининградский филиал ИЗМИРАН) во время солнечной вспышки 03.07.2021 г. Показано, что разработанная методика восстановления параметров ионосферы применима к трассам различной длины. Предлагается дальнейшее развитие методики, которая могла бы обеспечить восстановление параметров ионосферы на одночастотной трассе по измерениям в двух точках.</p></abstract><trans-abstract xml:lang="en"><p>The paper presents a comparative analysis of the reconstructed ionospheric parameters based on the data of receiving VLF signals at the Mikhnevo and Ul’yanovka observatories during the solar flare on 07/03/2021. It is shown that the developed method for reconstructing ionospheric parameters is applicable to paths of various lengths. A further development of the technique is proposed, which could ensure the reconstruction of the ionospheric parameters on a single-frequency path from measurements at two points.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>солнечные вспышки</kwd><kwd>ионосфера</kwd><kwd>рентген</kwd><kwd>ультрафиолет</kwd><kwd>распространение</kwd><kwd>радиоволны</kwd></kwd-group><kwd-group xml:lang="en"><kwd>solar flares</kwd><kwd>ionosphere</kwd><kwd>X-ray</kwd><kwd>ultraviolet</kwd><kwd>propagation</kwd><kwd>radio waves</kwd></kwd-group><funding-group xml:lang="ru"><funding-statement>Работа выполнена в рамках государственного задания Министерства науки и высшего образования РФ (тема № 122032900175-6).</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>
