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  <journal-meta>
   <journal-id journal-id-type="publisher-id">Solnechno-Zemnaya Fizika</journal-id>
   <journal-title-group>
    <journal-title xml:lang="en">Solnechno-Zemnaya Fizika</journal-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Солнечно-земная физика</trans-title>
    </trans-title-group>
   </journal-title-group>
   <issn publication-format="online">2712-9640</issn>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="publisher-id">88546</article-id>
   <article-id pub-id-type="doi">10.12737/szf-112202509</article-id>
   <article-categories>
    <subj-group subj-group-type="toc-heading" xml:lang="ru">
     <subject>Результаты  исследований</subject>
    </subj-group>
    <subj-group subj-group-type="toc-heading" xml:lang="en">
     <subject>Results of current research</subject>
    </subj-group>
    <subj-group>
     <subject>Результаты  исследований</subject>
    </subj-group>
   </article-categories>
   <title-group>
    <article-title xml:lang="en">Modelling the influence of magnetospheric storm on the large-scale structure of the high-latitude ionosphere for winter solstice conditions</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Моделирование влияния магнитной бури на крупномасштабную структуру высокоширотной ионосферы для зимних условий</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <contrib-id contrib-id-type="orcid">https://orcid.org/0000-0003-2184-8089</contrib-id>
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Гололобов</surname>
       <given-names>Артем Юрьевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Gololobov</surname>
       <given-names>Artem Yuryevich</given-names>
      </name>
     </name-alternatives>
     <email>golart87@gmail.com</email>
     <bio xml:lang="ru">
      <p>кандидат физико-математических наук;</p>
     </bio>
     <bio xml:lang="en">
      <p>candidate of physical and mathematical sciences;</p>
     </bio>
     <xref ref-type="aff" rid="aff-1"/>
     <xref ref-type="aff" rid="aff-2"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Голиков</surname>
       <given-names>Иннокентий Алексеевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Golikov</surname>
       <given-names>Innokentiy Alekseevich</given-names>
      </name>
     </name-alternatives>
     <email>gia2008@mail.ru</email>
     <bio xml:lang="ru">
      <p>доктор физико-математических наук;</p>
     </bio>
     <bio xml:lang="en">
      <p>doctor of physical and mathematical sciences;</p>
     </bio>
     <xref ref-type="aff" rid="aff-3"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Попов</surname>
       <given-names>Василий Иванович</given-names>
      </name>
      <name xml:lang="en">
       <surname>Popov</surname>
       <given-names>Vasiliy Ivanovich</given-names>
      </name>
     </name-alternatives>
     <email>volts@mail.ru</email>
     <bio xml:lang="ru">
      <p>кандидат физико-математических наук;</p>
     </bio>
     <bio xml:lang="en">
      <p>candidate of physical and mathematical sciences;</p>
     </bio>
     <xref ref-type="aff" rid="aff-4"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Институт космофизических исследований и аэрономии им. Ю.Г. Шафера СО РАН</institution>
     <city>Якутск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy SB RAS</institution>
     <city>Yakutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-2">
    <aff>
     <institution xml:lang="ru">Северо-Восточный федеральный университет им. М.К. Аммосова</institution>
     <city>Якутск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">North-Eastern Federal University</institution>
     <city>Yakutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-3">
    <aff>
     <institution xml:lang="ru">Институт космофизических исследований и аэрономии им. Ю.Г. Шафера СО РАН</institution>
     <city>Якутск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy SB RAS</institution>
     <city>Yakutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-4">
    <aff>
     <institution xml:lang="ru">Институт космофизических исследований и аэрономии им. Ю.Г. Шафера СО РАН</institution>
     <city>Якутск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy SB RAS</institution>
     <city>Yakutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <pub-date publication-format="print" date-type="pub" iso-8601-date="2025-06-26T16:59:24+03:00">
    <day>26</day>
    <month>06</month>
    <year>2025</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2025-06-26T16:59:24+03:00">
    <day>26</day>
    <month>06</month>
    <year>2025</year>
   </pub-date>
   <volume>11</volume>
   <issue>2</issue>
   <fpage>100</fpage>
   <lpage>111</lpage>
   <history>
    <date date-type="received" iso-8601-date="2024-09-16T00:00:00+03:00">
     <day>16</day>
     <month>09</month>
     <year>2024</year>
    </date>
    <date date-type="accepted" iso-8601-date="2025-01-14T00:00:00+03:00">
     <day>14</day>
     <month>01</month>
     <year>2025</year>
    </date>
   </history>
   <self-uri xlink:href="https://zh-szf.ru/en/nauka/article/88546/view">https://zh-szf.ru/en/nauka/article/88546/view</self-uri>
   <abstract xml:lang="ru">
    <p>На основе численных расчетов по модели высокоширотной ионосферы в эйлеровых переменных исследовано влияние возмущенной магнитосферной конвекции на крупномасштабную структуру ионосферы во время умеренной геомагнитной бури для условий зимнего солнцестояния. Показано, что возмущенное электрическое поле конвекции приводит к изменению форм и размеров основных структурных образований ионосферы. Выявлена зависимость эффекта влияния геомагнитной бури от времени начала возмущения вследствие несовпадения географического и геомагнитного полюсов (UT-контроль). Эффект наиболее выражен в случае бури с началом в 16 UT, когда возмущенное электрическое поле магнитосферной конвекции выносит плазму из дневной ионосферы на ночную сторону. Установлено, что в возмущенные периоды существенное влияние оказывает, наряду с горизонтальной компонентой электромагнитного дрейфа, его вертикальная компонента, которая приводит к увеличению высоты максимума F2-слоя на дневной стороне ионосферы и уменьшению на ночной.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>Using numerical calculations with a model of the high-latitude ionosphere in Eulerian variables, we study the influence of magnetospheric convection on the large-scale structure of the ionosphere during a moderate geomagnetic storm for winter solstice conditions. The disturbed electric field of convection is shown to cause changes in the shapes and sizes of the main structural formations of the ionosphere. We have found out that the effect of a geomagnetic storm depends on the time of the beginning of the disturbance due to the mismatch between the geographic and geomagnetic poles (UT control). The effect is most pronounced in the case of a storm that begins at 16 UT, when the disturbed electric field of magnetospheric convection transfers plasma of the daytime ionosphere to the nightside. It is shown that during periods of disturbances along with the horizontal component of the electromagnetic drift its vertical component, which causes an increase in the height of the F2-layer maximum on the dayside and its decrease on the nightside, also has a significant effect.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>магнитосферная конвекция</kwd>
    <kwd>магнитная буря</kwd>
    <kwd>модель ионосферы</kwd>
    <kwd>высокоширотная ионосфера</kwd>
    <kwd>субавроральная ионосферы</kwd>
    <kwd>несовпадение полюсов</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>magnetospheric convection</kwd>
    <kwd>magnetic storm</kwd>
    <kwd>ionosphere model</kwd>
    <kwd>high-latitude ionosphere</kwd>
    <kwd>subauroral ionosphere</kwd>
    <kwd>mismatch of poles</kwd>
   </kwd-group>
   <funding-group>
    <funding-statement xml:lang="ru">Работа выполнена в рамках государственного задания (номер госрегистрации № 122011700182-1)</funding-statement>
    <funding-statement xml:lang="en">The work was carried out under government as-signment (State Registration Number 122011700182-1)</funding-statement>
   </funding-group>
  </article-meta>
 </front>
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 </body>
 <back>
  <ref-list>
   <ref id="B1">
    <label>1.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Голиков И.А., Гололобов А.Ю., Попов В.И. Численное моделирование теплового режима высокоширотной ионосферы. Вестник Северо-Восточного федерального университета. 2012, т. 9, № 3, с. 22–28.</mixed-citation>
     <mixed-citation xml:lang="en">Burton R.K., McPherron R.L., Russel C.T. An empirical relationship between interplanetary conditions and Dst. J. Geophys. Res. 1975, vol. 80, no. 31. pp. 4204–4214. DOI: 10.1029/JA080i031p04204.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B2">
    <label>2.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Голиков И.А., Гололобов А.Ю., Попов В.И. Моделирование распределения температуры электронов в области F2 высокоширотной ионосферы для условий зимнего солнцестояния. Солнечно-земная физика. 2016, т. 2, № 4, c. 54–62. DOI: 10.12737/19424 / Golikov I.A., Gololobov A.Yu., Popov V.I. Modelling the electron temperature distribution in F2 region of high-latitude ionosphere for winter solstice. Solar-Terrestrial Physics. 2016, vol. 2, iss. 4, pp. 70–80. DOI: 10.12737/24269.</mixed-citation>
     <mixed-citation xml:lang="en">Chapman S. The absorption and dissociative of ionizing effect of monochromatic radiation in an atmosphere on a rotation. Earth. Proc. Phys. Soc. 1931, vol. 43. pp. 483–501. DOI: 10.1088/0959-5309/43/5/302.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B3">
    <label>3.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Голиков И.А., Гололобов А.Ю., Макаров Г.А., Баишев Д.Г. Определение зоны повышения температуры электронов в субавроральной ионосфере в глобальном масштабе во время магнитных бурь. Геомагнетизм и аэрономия. 2022, т. 62, №. 1, с. 106–118. DOI: 10.31857/S0016794022010084.</mixed-citation>
     <mixed-citation xml:lang="en">Danilov A.D. Reaction of F region to geomagnetic disturbances (review). Geliogeofizicheskie issledovaniya [Helio-Geophysic Research]. 2013, no. 5, pp. 1–33. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B4">
    <label>4.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Данилов А.Д. Реакция области F на геомагнитные возмущения (обзор). Гелиогеофизические исследования. 2013, № 5, с. 1–33.</mixed-citation>
     <mixed-citation xml:lang="en">David M., Schunk R. Sojka J. The effect of downward electron heat flow and electron cooling processes in the high-latitude ionosphere. J. Atmos. Solar-Terr. Phys. 2011, vol. 73, pp. 2399–2409. DOI: 10.1016/j.jastp.2011.08.009.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B5">
    <label>5.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Ермолаев Ю.И., Лодкина И.Г., Николаева Н.С., Ермолаев М.В. Статистическое исследование влияния межпланетных условий на геомагнитные бури. 2. Вариации параметров. Космические исследования. 2011, т. 49, № 1, с. 24–37.</mixed-citation>
     <mixed-citation xml:lang="en">Deng Y., Ridley A.J. Role of vertical ion convection in the high-latitude ionospheric plasma distribution. J. Geophys. Res. 2006, vol. 111, A09314. DOI: 10.1029/2006JA011637.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B6">
    <label>6.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Жеребцов Г.А., Мизун Ю.Г., Мингалев В.С. Физические процессы в полярной ионосфере. М.: Наука, 1988, 232 с.</mixed-citation>
     <mixed-citation xml:lang="en">Evans J.V. Millstone Hill Thomson scatter results for 1969. Technical Report 513. Massachusetts Institute of Technology, 1974, 140 p.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B7">
    <label>7.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Клименко В.В., Намгаладзе А.А. Эффекты зональных электрических полей в дневной зимней среднеширотной ионосфере. Геомагнетизм и аэрономия. 1976, т. 16, с. 1117–1119.</mixed-citation>
     <mixed-citation xml:lang="en">Fang X., Randall C., Lummerzheim D., Solomon S., Mills M.J., Marsh D.R., et al. Electron impact ionization: A new parameterization for 100 eV to 1 MeV electrons. J. Geophys. Res. 2008, vol. 113, iss. 9. DOI: 10.1029/2008 JA013384.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B8">
    <label>8.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Клименко М.В., Клименко В.В., Бессараб Ф.С. и др. Влияние геомагнитных бурь 26–30 сентября 2011 года на ионосферу и распространение радиоволн КВ-диапазона. I-ионосферные эффекты. Геомагнетизм и аэрономия. 2015, т. 55, №. 6, с. 769–789.</mixed-citation>
     <mixed-citation xml:lang="en">Golikov I.A., Gololobov A.Yu., Popov V.I. Numerical simulation of thermal regime of high-latitude ionosphere. Vestnik Severo-Vostochnogo federal'nogo universiteta [Vestnik of North-Eastern Federal University]. 2012, vol. 9, no. 3, pp. 22–28. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B9">
    <label>9.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Колесник А.Г., Голиков И.А. Исследование роли различных механизмов в формировании F2 ионосферы на двухмерной модели. Геомагнетизм и аэрономия. 1981, т. 21, № 4, с. 612–616.</mixed-citation>
     <mixed-citation xml:lang="en">Golikov I.A., Gololobov A.Yu., Popov V.I. Modelling the electron temperature distribution in F2 region of high-latitude ionosphere for winter solstice. Solar-Terr. Phys. 2016, vol. 2, iss. 4, pp. 54–62. DOI: 10.12737/24269.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B10">
    <label>10.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Колесник А.Г., Голиков И.А. Трехмерная модель высокоширотной области F с учетом несовпадения географических и геомагнитных координат. Геомагнетизм и аэрономия. 1982, т. 22, № 3, с. 435–439.</mixed-citation>
     <mixed-citation xml:lang="en">Golikov I., Gololobov A., Baishev D. Universal time control of the parameters of the electron temperature enhancement zone in the winter subauroral ionosphere. J. Atmos. Solar-Terr. Phys. 2020, vol. 211. DOI: 10.1016/j.jastp.2020.105458.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B11">
    <label>11.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Колесник А.Г., Голиков И.А. Явление «полной тени» в верхней атмосфере Земли. Доклады АН СССР. 1984, т. 279, № 4, с. 832–834.</mixed-citation>
     <mixed-citation xml:lang="en">Golikov I., Gololobov A., Baishev D., Makarov G. Determination of the enhancement in electron temperature in the subauroral ionosphere during magnetic storms on a global scale. Geomagnetism and Aeronomy. 2022, vol. 61, suppl. 1, pp. S103–S115. DOI: 10.1134/S001679322201008X.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B12">
    <label>12.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Кринберг И.А., Тащилин А.В. Ионосфера и плазмосфера. М.: Наука, 1984. 190 с.</mixed-citation>
     <mixed-citation xml:lang="en">Heppner J.P., Maynard N.C. Empirical high-latitude electric field models. J. Geophys. Res. 1987, vol. 92, pp. 4467–4489.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B13">
    <label>13.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Ларина Т.Н., Глебова Г.М. Исследование вариаций электронной концентрации в F-слое полярной ионосферы, обусловленных сменой знака By-компоненты межпланетного магнитного поля. Инженерный вестник Дона. 2019, № 1, 11 с. URL: http://www.ivdon.ru/uploads/article/pdf/IVD_120_larina_N.pdf_5a3560990a.pdf (дата обращения 10 января 2025 г.).</mixed-citation>
     <mixed-citation xml:lang="en">Klimenko V.V., Namgaladze A.A. The effects of zonal electric field in the daytime winter midlatitude ionosphere. Geomagnetizm i ajeronomija [Geomagnetism and aeronomy]. 1976, vol. 16, pp. 1117–1119. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B14">
    <label>14.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Мизун Ю.Г. Полярная ионосфера. Л.: Наука, 1980, 216 с.</mixed-citation>
     <mixed-citation xml:lang="en">Klimenko M.V., Klimenko V.V., Bessarab F.S., Ratovsky K.G., Zakharenkova I.E., Nosikov I.A., Stepanov A.E., et al. Influence of geomagnetic storms of September 26–30, 2011, on the ionosphere and HF radiowave propagation. I. Ionospheric effects.Geomagnetism and Aeronomy. 2015, vol. 55, no. 6, pp. 744–762.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B15">
    <label>15.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Мингалев В.С. Влияние электрических полей на полярную ионосферу. Полярная ионосфера и магнитосферно-ионосферные связи. Апатиты: КФ АН СССР, 1978, с. 43–48.</mixed-citation>
     <mixed-citation xml:lang="en">Klimenko M.V., Zakharenkova I.E., Klimenko V.V., Lukianova R.Yu., Cherniak I.V. Simulation and observation of the polar tongue of ionization at different heights during the 2015 St. Patric’s day storms. Space Weather. 2019, vol. 17, pp. 1073–1089. DOI: 10.1029/2018SW002143.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B16">
    <label>16.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Ратовский К.Г, Клименко М.В., Клименко В.В. и др. Эффекты последствий геомагнитных бурь: Статистический анализ и теоретическое объяснение. Солнечно-земная физика. 2018, т. 4, № 4, с. 32–42. DOI: 10.12737/szf44201804 // Ratovsky K.G., Klimenko M.V., Klimenko V.V., Chirik N.V., Korenkova N.A., Kotova D.S. After-effects of geomagnetic storms: statistical analysis and theoretical explanation. Solar-Terrestrial Physics. 2018, vol. 4, iss. 4, рр. 26–32. DOI: 10.12737/stp-44201804.</mixed-citation>
     <mixed-citation xml:lang="en">Kolesnik A.G., Golikov I.A. Study of the role of various mechanisms in formation of the F2 region of the ionosphere on a two-dimensional model Geomagnetizm i ajeronomiya [Geomagnetism and Aeronomy]. 1981, vol. 21, no. 4, pp. 612–616. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B17">
    <label>17.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Уваров В.М., Барашков П.Д. Типы распределения электрических полей и соответствующие им типы конвекции в полярной ионосфере. Модель. Геомагнетизм и аэрономия. 1989, т. 29, № 4, c. 621–628.</mixed-citation>
     <mixed-citation xml:lang="en">Kolesnik A.G., Golikov I.A. Three-dimensional model of the high-latitude F region with taking into account the mistmach of geographic and geomagnetic coordinates. Geomagnetizm i ajeronomiya [Geomagnetism and Aeronomy], 1982, vol. 22, no 3, pp. 435–439. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B18">
    <label>18.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Уваров В.М., Лукьянова Р.Ю. Моделирование высокоширотной ионосферы с учетом влияния параметров межпланетной среды. Гелиогеофизические исследования. 2014, № 7, c. 108–118.</mixed-citation>
     <mixed-citation xml:lang="en">Kolesnik A.G., Golikov I.A. The “full shadow” phenomena in Earth upper atmosphere. Doklady AN SSSR [Report of Academy of Sciences USSR]. 1984, vol. 279, no. 4, pp. 832–834. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B19">
    <label>19.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Burton R.K., McPherron R.L., Russel C.T. An empirical relationship between interplanetary conditions and Dst. J. Geophys. Res. 1975, vol. 80, no. 31, рр. 4204–4214. DOI: 10.1029/JA080i031p04204.</mixed-citation>
     <mixed-citation xml:lang="en">Krinberg I.A., Taschilin A.V.Ionosfera i plazmosfera [Ionosphere and Plasmasphere]. Moscow, Nauka Publ., 1984, p. 190. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B20">
    <label>20.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Chapman S. The absorption and dissociative of ionizing effect of monochromatic radiation in an atmosphere on a rotation. Earth. Proc. Phys. Soc. 1931, vol. 43, рр. 483–501. DOI: 10.1088/0959-5309/43/5/302.</mixed-citation>
     <mixed-citation xml:lang="en">Larina T.N., Glebova G.M. Investigation of electron density variation in the polar ionosphere F-layer influenced by interplanetary magnetic field By component sign. Inzhenernyi vestnik Dona [Engineering Bull. of Don]. 2019, vol. 1, 11 p. URL: http://www.ivdon.ru/uploads/article/pdf/IVD_120__larina_N.pdf_5a3560990a.pdf (accessed January 10, 2025).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B21">
    <label>21.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">David M., Schunk R. Sojka J. The effect of downward electron heat flow and electron cooling processes in the high-latitude ionosphere. J. Atmos. Solar-Terrestrial Physics. 2011, vol. 73, рр. 2399–2409. DOI: 10.1016/j.jastp.2011.08.009.</mixed-citation>
     <mixed-citation xml:lang="en">Liu J., Wang W., Burns A., Liu L., McInerney J. A TIEGCM numerical study of the source and evolution of ionospheric F-region tongues of ionization: Universal time and interplanetary magnetic field dependence. J. Atmos. Solar-Terr. Phys. 2017, vol. 156, pp. 87–96. DOI: 10.1016/j.jastp.2017.03.005.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B22">
    <label>22.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Deng Y., Ridley A.J. Role of vertical ion convection in the high-latitude ionospheric plasma distribution. J. Geophyus. Res. 2006, vol. 111, A09314. DOI: 10.1029/2006JA011637.</mixed-citation>
     <mixed-citation xml:lang="en">Lukianova R.Yu., Uvarov V.M., Coisson P. High-latitude F region large-scale ionospheric irregularities under different solar wind and zenith angle conditions. Adv. Space. Res. 2016, vol. 59, pp. 557–570. DOI: 10.1016/j.asr.2016.10.010.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B23">
    <label>23.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Evans J.V. Millstone Hill Thomson scatter results for 1969. Technical Report 513. Massachusetts Institute of Technology, 1974, 140 p.</mixed-citation>
     <mixed-citation xml:lang="en">Mingalev V.S. Electric field influence on the polar ionosphere. Polyarnaya ionosfera i magnitosferno-ionosfernye svyazi [Polar ionosphere and magnetosphere-ionosphere coupling]. Apatity, 1978, pp. 43–48. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B24">
    <label>24.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Fang X., Randall C., Lummerzheim D., et al. Electron impact ionization: A new parameterization for 100 eV to 1 MeV electrons. J. Geophys. Res. 2008, vol. 113, iss. 9. DOI: 10.1029/2008JA013384.</mixed-citation>
     <mixed-citation xml:lang="en">Mizun Yu.G. Polyarnaya ionosfera [Polar ionosphere]. Leningrad, Nauka Publ., 1980, 216 p. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B25">
    <label>25.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Golikov I., Gololobov A., Baishev D. Universal time control of the parameters of the electron temperature enhancement zone in the winter subauroral ionosphere. J. Atmos. Solar-Terr. Phys. 2020, vol. 211, 105458. DOI: 10.1016/j.jastp.2020.105458.</mixed-citation>
     <mixed-citation xml:lang="en">Murayama T. Coupling function between solar wind parameters and geomagnetic indices. Rev. Geophys. Space Phys. 1982, vol. 20, no. 3, pp. 623–629. DOI: 10.1029/RG020i003p00623.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B26">
    <label>26.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Heppner J.P., Maynard N.C. Empirical high-latitude electric field models. J. Geophys. Res. 1987, vol. 92, pp. 4467–4489. DOI: 10.1029/JA092iA05p04467.</mixed-citation>
     <mixed-citation xml:lang="en">Murayama T., Aoki T., Nakai H., Hakamada K. Empirical formula to relate the auroral electrojet intensity with interplanetary parameters. Planet Space. Sci. 1980, vol. 28, pp. 803–813.DOI: 10.1016/0032-0633(80)90078-1.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B27">
    <label>27.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Klimenko M.V., Zakharenkova I.E., Klimenko V.V., et al. Simulation and observation of the polar tongue of ionization at different heights during the 2015 St. Patric’s day storms. Space Weather. 2019, vol. 17, pp. 1073–1089. DOI: 10.1029/2018SW002143.</mixed-citation>
     <mixed-citation xml:lang="en">Picone J.M., Hedin A.E., Drob D.P. Aikin A. NRLMSISE-00 empirical model of the atmosphere: Statistical comparison and scientific issues. J. Geophys. Res. 2002, vol. 107, pp. 1501–1516. DOI: 10.1029/2002JA009430.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B28">
    <label>28.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Liu J., Wang W., Burns A., et al. A TIEGCM numerical study of the source and evolution of ionospheric F-region tongues of ionization: Universal time and interplanetary magnetic field dependence. J. Atmos. Solar-Terr. Phys. 2017, vol. 156, pp. 87–96. DOI: 10.1016/j.jastp.2017.03.005.</mixed-citation>
     <mixed-citation xml:lang="en">Prölss G.W. Ionospheric F-region storms. Handbook of Atmospheric Electrodynamics II. Eds. H. Volland. Boca Raton, CRC Press, 1995, pp. 195–248.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B29">
    <label>29.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Lukianova R.Yu., Uvarov V.M., Coisson P. High-latitude F region large-scale ionospheric irregularities under different solar wind and zenith angle conditions. Adv. Space. Res. 2016, vol. 59, pp. 557–570. DOI: 10.1016/j.asr.2016.10.010.</mixed-citation>
     <mixed-citation xml:lang="en">Ratovsky K.G., Klimenko M.V., Klimenko V.V., Chirik N.V., Korenkova N.A., Kotova D.S. After-effects of geomagnetic storms: statistical analysis and theoretical explanation. Solar-Terr. Phys. 2018, vol. 4, iss. 4, pp. 26–32. DOI: 10.12737/stp-44201804.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B30">
    <label>30.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Murayama T. Coupling function between solar wind parameters and geomagnetic indices. Rev. Geophys. Space Phys. 1982, vol. 20, no. 3, pp. 623–629. DOI: 10.1029/RG020i003p00623.</mixed-citation>
     <mixed-citation xml:lang="en">Samarskii A. The Theory of Difference Schemes. New York, Marcel Dekker, 2001, 761 p.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B31">
    <label>31.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Murayama T., Aoki T., Nakai H., Hakamada K. Empirical formula to relate the auroral electrojet intensity with interplanetary parameters. Planet Space. Sci. 1980, vol. 28, pp. 803–813. DOI: 10.1016/0032-0633(80)90078-1.</mixed-citation>
     <mixed-citation xml:lang="en">Schunk R., Nagy A. Electron temperature in the F regions of the ionosphere: theory and observations. Rev. Geophys. 1978, vol. 16, pp. 355–399. DOI: 10.1029/RG016i003p00355.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B32">
    <label>32.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Picone J.M., Hedin A.E., Drob D.P. Aikin A. NRLMSISE-00 empirical model of the atmosphere: Statistical comparison and scientific issues. J. Geophys. Res. 2002, vol. 107, pp. 1501–1516. DOI: 10.1029/2002JA009430.</mixed-citation>
     <mixed-citation xml:lang="en">Schunk R.W., Nagy A. Ionospheres: Physics, Plasma Physics, and Chemistry. New York, Cambridge University Press, 2009, 628 p.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B33">
    <label>33.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Prölss G.W. Ionospheric F-Region Storms. Handbook of Atmospheric Electrodynamics II. Eds. H. Volland. Boca Raton: CRC Press, 1995, pp. 195–248.</mixed-citation>
     <mixed-citation xml:lang="en">Sojka J.J., Raitt W.J., Schunk R.W. Effect of displaced geomagnetic and geographic poles on high-latitude plasma convection and ionospheric depletions. J. Geophys. Res. 1979, vol. 85, no. A10, pp. 5943–5951. DOI: 10.1029/JA084iA10p05943.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B34">
    <label>34.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Samarskii A. The Theory of Difference Schemes. New York: Marcel Dekker, 2001, 761 p.</mixed-citation>
     <mixed-citation xml:lang="en">Tashchilin A.V., Romanova E.B. Numerical modeling the high-latitude ionosphere. Proc. of the COSPAR Colloquim on Solar-Terrestrial Magnetic Activity and Space Environment (STMASE). Beijing, China. Pergamon, 2002, vol. 14, pp. 315–325.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B35">
    <label>35.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Schunk R., Nagy A. Electron temperature in the F regions of the ionosphere: theory and observations. Rev. Geophys. 1978, vol. 16, pp. 355–399. DOI: 10.1029/RG016i003p00355.</mixed-citation>
     <mixed-citation xml:lang="en">Tashchilin A.V., Romanova E.B. Influence of magnetospheric inputs definition on modeling of ionospheric storms. Physics of Auroral Phenomena, Proc. XXX Annual Seminar, 2007, pp. 189–192.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B36">
    <label>36.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Schunk R.W., Nagy A. Ionospheres: Physics, Plasma Physics, and Chemistry. New York: Cambridge University Press, 2009, 628 p.</mixed-citation>
     <mixed-citation xml:lang="en">Uvarov V.M., Barashkov P.D. The electric field distribution types and related convection types in the polar ionosphere. Model.Geomagnetizm i ajeronomiya [Geomagnetism and Aeronomy]. 1989, vol. 29, no. 4, pp. 621–628. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B37">
    <label>37.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Sojka J.J., Raitt W.J., Schunk R.W. Effect of displaced geomagnetic and geographic poles on high-latitude plasma convection and ionospheric depletions. J. Geophys. Res. 1979, vol. 85, no. A10, pp. 5943–5951. DOI: 10.1029/JA084iA10p05943.</mixed-citation>
     <mixed-citation xml:lang="en">Uvarov V.M., Lukianova R.Yu. The high-latitude ionosphere modelling with considering interplanetary medium.Geliogeofizicheskie issledovaniya [Helio-geophysical research]. 2014, no 7, pp. 108–118. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B38">
    <label>38.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Tashchilin A.V., Romanova E.B. Numerical modeling the high-latitude ionosphere. Proc. of the COSPAR Colloquim on Solar-Terrestrial Magnetic Activity and Space Environment (STMASE). Beijing, China. Pergamon, 2002, vol. 14, pp. 315–325.</mixed-citation>
     <mixed-citation xml:lang="en">Uvarov V.M., Lukianova R.Yu. Numerical modeling of the polar F region ionosphere taking into account the solar wind conditions. Adv. Space. Res. 2015, vol. 56, no. 11, pp. 2563–2574. DOI: 10.1016/j.asr.2015.10.004.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B39">
    <label>39.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Tashchilin A.V., Romanova E.B. Influence of magnetospheric inputs definition on modeling of ionospheric storms. Physics of Auroral Phenomena, Proc. XXX Annual Seminar. 2007, pp. 189–192.</mixed-citation>
     <mixed-citation xml:lang="en">Vorobjev V.G., Yagodkina O.I., Katkalov Yu.V. Auroral Precipitation Model and its application to ionospheric and magnetospheric studies. J. Atmos. Solar-Terr. Phys. 2013, vol. 102, pp. 157–171. DOI: 10.1016/j.jastp.2013.05.007.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B40">
    <label>40.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Uvarov V.M., Lukianova R.Yu. Numerical modeling of the polar F region ionosphere taking into account the solar wind conditions. Adv. Space. Res. 2015, vol. 56, no. 11, pp. 2563–2574. DOI: 10.1016/j.asr.2015.10.004.</mixed-citation>
     <mixed-citation xml:lang="en">Watkins B.J. A numerical computer investigation of the polar F-region ionosphere. Planet. Space Sci. 1978, vol. 26, pp. 559–569. DOI: 10.1016/0032-0633(78)90048-X.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B41">
    <label>41.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Vorobjev V.G., Yagodkina O.I., Katkalov Yu.V. Auroral Precipitation Model and its application to ionospheric and magnetospheric studies. J. Atmos. Solar-Terr. Phys. 2013, vol. 102, pp. 157–171. DOI: 10.1016/j.jastp.2013.05.007.</mixed-citation>
     <mixed-citation xml:lang="en">Weimer D.R. A flexible, IMG dependent model of high-latitude electric potentials having “space weather” applications. Geophys. Res. Lett. 1996, vol. 23, no. 18. pp. 2549–2552.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B42">
    <label>42.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Watkins B.J. A numerical computer investigation of the polar F-region ionosphere. Planet. Space Sci. 1978, vol. 26, pp. 559–569. DOI: 10.1016/0032-0633(78)90048-X.</mixed-citation>
     <mixed-citation xml:lang="en">Yermolaev Yu.I., Lodkina I.G., Nikolaeva N.S., Yermolaev M.Yu. Statistical study of interplanetary condition effect on geomagnetic storms: 2. Variations of parameters. Cosmic Res. 2011, vol. 49, no 1, pp. 21–34. DOI: 10.1134/S0010 952511010035.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B43">
    <label>43.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Weimer D.R. A flexible, IMG dependent model of high-latitude electric potentials having “space weather” applications. Geophys. Res. Lett. 1996, vol. 23, no. 18, pp. 2549–2552.</mixed-citation>
     <mixed-citation xml:lang="en">Zherebtsov G.A., Mizun Yu.G., Mingalev V.S. Fizicheskie protsessy v polyarnoi ionosfere [Physical processes in the polar ionosphere]. Moscow, Nauka Publ., 1988, 231 p. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B44">
    <label>44.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Zou S., Ridley A., Moldwin M.B., et al. Multi-instrument observations of SED during 24–25 October 2011 storm: Implications for SED formation processes. J. Geophys. Res.: Space Phys. 2013, vol. 118, pp. 7798–7809. DOI: 10.1002/2013JA018860.</mixed-citation>
     <mixed-citation xml:lang="en">Zou S., Ridley A., Moldwin M.B., Nicolls M.J., Coster A.J., Thomas E.G., Ruohoniemi J.M. Multi-instrument observations of SED during 24-25 October 2011 storm: Implications for SED formation processes. J. Geophys. Res.: Space Phys. vol. 118. pp. 7798–7809. DOI: 10.1002/2013JA018860.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B45">
    <label>45.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: http://omniweb.gsfc.nasa.gov (дата обращения 10 января 2025 г.).</mixed-citation>
     <mixed-citation xml:lang="en">URL: http://omniweb.gsfc.nasa.gov (accessed January 10, 2025).</mixed-citation>
    </citation-alternatives>
   </ref>
  </ref-list>
 </back>
</article>
