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 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">Solar-Terrestrial Physics</journal-id>
   <journal-title-group>
    <journal-title xml:lang="en">Solar-Terrestrial Physics</journal-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Солнечно-земная физика / Solnechno-Zemnaya Fizika / Solar-Terrestrial Physics</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">51392</article-id>
   <article-id pub-id-type="doi">10.12737/szf-84202203</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">Geomagnetic indices ASY-H and SYM-H and their relation to interplanetary parameters</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Геомагнитные индексы ASYH и SYMH и их связь с межпланетными параметрами</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Макаров</surname>
       <given-names>Георгий Афанасьевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Makarov</surname>
       <given-names>Georgy Afanasyevich</given-names>
      </name>
     </name-alternatives>
     <email>gmakarov@ikfia.sbras.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-1"/>
    </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>
   <pub-date publication-format="print" date-type="pub" iso-8601-date="2022-12-24T19:09:02+03:00">
    <day>24</day>
    <month>12</month>
    <year>2022</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2022-12-24T19:09:02+03:00">
    <day>24</day>
    <month>12</month>
    <year>2022</year>
   </pub-date>
   <volume>8</volume>
   <issue>4</issue>
   <fpage>38</fpage>
   <lpage>45</lpage>
   <history>
    <date date-type="received" iso-8601-date="2022-06-23T00:00:00+03:00">
     <day>23</day>
     <month>06</month>
     <year>2022</year>
    </date>
    <date date-type="accepted" iso-8601-date="2022-09-20T00:00:00+03:00">
     <day>20</day>
     <month>09</month>
     <year>2022</year>
    </date>
   </history>
   <self-uri xlink:href="https://naukaru.ru/en/nauka/article/51392/view">https://naukaru.ru/en/nauka/article/51392/view</self-uri>
   <abstract xml:lang="ru">
    <p>За период времени с 1981 по 2015 г. исследуются зависимости геомагнитных индексов SYM-H и ASY-H от межпланетных параметров по их среднесуточным значениям. Исследование проводится двумя путями: первый — анализируется весь массив данных, второй — данные разбиваются на девять групп активности в соответствии со среднесуточными значениями планетарного геомагнитного индекса Ар. Выполнен корреляционный анализ индексов кольцевого тока ASY-H, SYM-H и скорости солнечного ветра, модуля и северо-южной компоненты межпланетного магнитного поля (ММП). Поиск связи индексов ASY-H и SYM-H с межпланетными параметрами оказался более успешным при рассмотрении всего массива данных, чем в случае разбивки данных по группам магнитной активности. Определены регрессионные уравнения, связывающие ASY-H и SYM-H с межпланетными параметрами. Обнаружено, что при описании связи индексов ASY-H и SYM-H с северо-южной компонентой ММП необходимо учитывать вклад модуля ММП.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>The dependences of the geomagnetic indices SYM-H and ASY-H on interplanetary parameters for the period from 1981 to 2015 according to their daily averages are studied. The study is carried out in two ways: the first — the entire data array is analyzed, the second — the data are divided into 9 activity groups in accordance with the average daily values of the planetary geomagnetic index Ap. A correlation analysis of the indices with the solar wind speed, magnitude, and the north-south component of the interplanetary magnetic field (IMF) has been performed. The search for a relationship between the ASY-H and SYM-H indices and interplanetary parameters turned out to be more successful when considering the entire data array than in the case of splitting the data into groups of magnetic activity. Regression equations relating ASY-H and SYM-H to interplanetary parameters are determined. It has been found that when describing the relationship between the ASY-H and SYM-H indices and the IMF north-south component, it is necessary to take into account the contribution of the IMF modulus.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>геомагнитные индексы SYM-H и ASY-H</kwd>
    <kwd>геомагнитная активность</kwd>
    <kwd>магнитосферный кольцевой ток</kwd>
    <kwd>межпланетные параметры</kwd>
    <kwd>космическая погода</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>geomagnetic indices SYM-H and ASY-H</kwd>
    <kwd>geomagnetic activity</kwd>
    <kwd>magnetospheric ring current</kwd>
    <kwd>interplanetary parameters</kwd>
    <kwd>space weather</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 financially supported by the Ministry of Science and Higher Education of the Russian Federation (Grant No. 075-GZ/Ts3569/278)</funding-statement>
   </funding-group>
  </article-meta>
 </front>
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 <back>
  <ref-list>
   <ref id="B1">
    <label>1.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Вайсберг О.Л., Смирнов В.Н., Застенкер Г.Н. и др. Взаимодействие солнечного ветра с внешней магнитосферой Земли. Плазменная гелиогеофизика. Т. 1 / Под ред. Л.М. Зеленого, И.С. Веселовского. М.: ФИЗМАТЛИТ, 2008. С. 378-422.</mixed-citation>
     <mixed-citation xml:lang="en">Akasofu S.-I. Interplanetary energy flux associated with magnetospheric substroms. Planet. Space Sci. 1979, vol. 27, iss. 4, pp. 425-431. DOI: 10.1016/0032-0633(79)90119-3.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B2">
    <label>2.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Ермолаев Ю.И., Лодкина И.Г., Николаева Н.С., Ермолаев М.Ю. Статистическое исследование влияния межпланетных условий на геомагнитные бури. Космические исследования. 2010. T. 48, № 6. C. 499-515.</mixed-citation>
     <mixed-citation xml:lang="en">Alexeev I.I., Belenkaya E.S., Kalegaev V.V., Feldstein Y.I., Grafe A. Magnetic storms and magnetotail currents. J. Geophys. Res. 1996, vol. 101, iss. A4, pp. 7737-7747. DOI: 10.1029/95JA03509.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B3">
    <label>3.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Макаров Г.А. Смещения значений геомагнитных индексов магнитосферного кольцевого тока. Солнечно-земная физика. 2021. Т. 7, № 3. С. 31-38. DOI: 10.12737/szf-73202103.</mixed-citation>
     <mixed-citation xml:lang="en">Ballif J.R., Jones D.E., Coleman P.J. Further evidence on the correlation between transverse fluctuations in the interplanetary magnetic field and Kp. J. Geophys. Res. 1969, vol. 74, iss. 9, pp. 2289-2301. DOI: 10.1029/JA074i009p02289.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B4">
    <label>4.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Akasofu S.-I. Interplanetary energy flux associated with magnetospheric substroms. Planet. Space Sci. 1979. Vol. 27, iss. 4. P. 425-431. DOI: 10.1016/0032-0633(79)90119-3.</mixed-citation>
     <mixed-citation xml:lang="en">Burton R.K., McPherron R.L., Russell C.T. An empirical relationship between interplanetary conditions and Dst. J. Geophys. Res. 1975, vol. 80, iss. 31, pp. 4204-4214. DOI: 10.1029/ja080i031p04204.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B5">
    <label>5.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Alexeev I.I., Belenkaya E.S., Kalegaev V.V., et al. Magnetic storms and magnetotail currents. J. Geophys. Res. 1996. Vol. 101, iss. A4. P. 7737-7747. DOI: 10.1029/95JA03509.</mixed-citation>
     <mixed-citation xml:lang="en">Dubyagin S., Ganushkina N., Kubyshkina M., Liemohn M. Contribution from different current systems to SYM and ASY midlatitude indices. J. Geophys. Res. 2014, vol. 119, pp. 7243-7263. DOI: 10.1002/2014JA020122.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B6">
    <label>6.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Ballif J.R., Jones D.E., Coleman P.J. Further evidence on the correlation between transverse fluctuations in the interplanetary magnetic field and Kp. J. Geophys. Res. 1969. Vol. 74, iss. 9. P. 2289-2301. DOI: 10.1029/JA074i009p02289.</mixed-citation>
     <mixed-citation xml:lang="en">Echer E., Tsurutani B.T., Gonzalez W.D. Interplanetary origins of moderate (-100 nT &lt; Dst ≤ -50 nT) geomagnetic storms during solar cycle 23 (1996-2008). J. Geophys. Res. 2013, vol. 118, iss. 1, pp. 385-392. DOI: 10.1029/2012JA018086.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B7">
    <label>7.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Burton R.K., McPherron R.L., Russell C.T. An empirical relationship between interplanetary conditions and Dst. J. Geophys. Res. 1975. Vol. 80, iss. 31. P. 4204-4214. DOI: 10.1029/ja080i031p04204.</mixed-citation>
     <mixed-citation xml:lang="en">Friis-Christensen E., Lassen K., Wilhjelm J., Wilcox J.M., Gonzalez W., Colburn D.S. Critical component of the interplanetary magnetic field responsible for large geomagnetic effects in the polar cap. J. Geophys. Res. 1972, vol. 77, iss 19, pp. 3371-3376. DOI: 10.1029/JA077i019p03371.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B8">
    <label>8.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Dubyagin S., Ganushkina N., Kubyshkina M., Liemohn M. Contribution from different current systems to SYM and ASY midlatitude indices. J. Geophys. Res. 2014. Vol. 119. P. 7243-7263. DOI: 10.1002/2014JA020122.</mixed-citation>
     <mixed-citation xml:lang="en">Holser R.E., Slavin J.A. An evaluation of three predictors of geomagnetic activity. J. Geophys. Res. 1982, vol. 87, iss. A4, pp. 2558-2562. DOI: 10.1029/JA087iA04p02558.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B9">
    <label>9.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Echer E., Tsurutani B.T., Gonzalez W.D. Interplanetary origins of moderate (-100 nT &lt; Dst ≤ -50 nT) geomagnetic storms during solar cycle 23 (1996-2008). J. Geophys. Res. 2013. Vol. 118, iss. 1. P. 385-392. DOI: 10.1029/2012JA018086.</mixed-citation>
     <mixed-citation xml:lang="en">Iyemori T., Araki T., Kamei T., Takeda M. Mid-latitude geomagnetic indices ASY and SYM (Provisional) No. 1 (1989-1990). Data Analysis Center for Geomagnetism and Space Magnetism; Kyoto University, Kyoto, 1992, 110 p.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B10">
    <label>10.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Friis-Christensen E., Lassen K., Wilhjelm J., et al. Critical component of the interplanetary magnetic field responsible for large geomagnetic effects in the polar cap. J. Geophys. Res. 1972. Vol. 77, iss 19. P. 3371-3376. DOI: 10.1029/JA077i019p03371.</mixed-citation>
     <mixed-citation xml:lang="en">Liemohn M.W., McCollough J.P., Jordanova V.K., Ngwira C.M., Morley S.K., Cid C., et al. Model evaluation guidelines for geomagnetic index predictions. Space Weather. 2018, vol. 16, pp. 2079-2102. DOI: 10.1029/2018SW002067.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B11">
    <label>11.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Holser R.E., Slavin J.A. An evaluation of three predictors of geomagnetic activity. J. Geophys. Res. 1982. Vol. 87, iss. A4. P. 2558-2562. DOI: 10.1029/JA087iA04p02558.</mixed-citation>
     <mixed-citation xml:lang="en">Lockwood M., McWilliams K.A. On optimum solar wind magnetosphere coupling functions for transpolar voltage and planetary geomagnetic activity. J. Geophys. Res. 2021, vol. 126, e2021JA029946. DOI: 10.1029/2021JA029946.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B12">
    <label>12.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Iyemori T., Araki T., Kamei T., Takeda M. Mid-latitude geomagnetic indices ASY and SYM (Provisional) No. 1 (1989-1990). Data Analysis Center for Geomagnetism and Space Magnetism; Kyoto University, Kyoto, 1992. 110 р.</mixed-citation>
     <mixed-citation xml:lang="en">Makarov G.A. Offset in the geomagnetic indices of the magnetospheric ring current. Solar-Terr. Phys. 2021, vol. 7, iss. 3, pp. 29-35. DOI: 10.12737/stp-73202103.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B13">
    <label>13.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Liemohn M.W., McCollough J.P., Jordanova V.K., et al. Model evaluation guidelines for geomagnetic index predictions. Space Weather. 2018. Vol. 16. P. 2079-2102. DOI: 10.1029/ 2018SW002067.</mixed-citation>
     <mixed-citation xml:lang="en">Maltsev Y.P., Arykov A.A., Belova E.G., Gvozdevsky B.B., Safargaleev V.V. Magnetic flux redistribution in the storm time magnetosphere. J. Geophys. Res. 1996, vol. 101, no. A4, pp. 7697-7704. DOI: 10.1029/95JA03709.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B14">
    <label>14.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Lockwood M., McWilliams K.A. On optimum solar wind magnetosphere coupling functions for transpolar voltage and planetary geomagnetic activity. J. Geophys. Res. 2021. Vol. 126, e2021JA029946. DOI: 10.1029/2021JA029946.</mixed-citation>
     <mixed-citation xml:lang="en">Meng X., Tsurutani B.T., Mannucci A.J. The solar and interplanetary causes of superstorms (minimum Dst≤−250 nT) during the space age. J. Geophys. Res. 2019, vol. 124, iss. 6, pp. 3926-3948. DOI: 10.1029/2018JA026425.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B15">
    <label>15.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Maltsev Y.P., Arykov A.A., Belova E.G., et al. Magnetic flux redistribution in the storm time magnetosphere. J. Geophys. Res. 1996. Vol. 101, no. A4. P. 7697-7704. DOI: 10.1029/95JA03709.</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, iss. 8, pp. 803-813. DOI: 10.1016/0032-0633(80)90078-1.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B16">
    <label>16.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Meng X., Tsurutani B.T., Mannucci A.J. The solar and interplanetary causes of superstorms (minimum Dst ≤ −250 nT) during the space age. J. Geophys. Res. 2019. Vol. 124, iss. 6. P. 3926-3948. DOI: 10.1029/2018JA026425.</mixed-citation>
     <mixed-citation xml:lang="en">Newell P.T., Sotirelis T., Liou K., Meng C.-I., Rich F.J. A nearly universal solar wind-magnetosphere coupling function inferred from 10 magnetospheric state variables. J. Geophys. Res. 2007, vol. 112, A01206. DOI: 10.1029/2006JA012015.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B17">
    <label>17.</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, iss. 8. P. 803-813. DOI: 10.1016/0032-0633(80)90078-1.</mixed-citation>
     <mixed-citation xml:lang="en">Rostoker G., Falthammer C.-G. Relationship between changes in the interplanetary magnetic field and variations in the magnetic field at the Earth’s surface. J. Geophys. Res. 1967, vol. 72, iss. 23, pp. 5853-5863. DOI: 10.1029/JZ072i023p05853.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B18">
    <label>18.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Newell P.T., Sotirelis T., Liou K., et al. A nearly universal solar wind-magnetosphere coupling function inferred from 10 magnetospheric state variables. J. Geophys. Res. 2007. Vol. 112. A01206. DOI: 10.1029/2006JA012015.</mixed-citation>
     <mixed-citation xml:lang="en">Snyder C.W., Neugebauer M., Rao N.R. The solar wind velocity and its correlation with cosmic ray variations and with solar and geomagnetic activity. J. Geophys. Res. 1963, vol. 68, iss. 24, pp. 6361-6370. DOI: 10.1029/ JZ068i024p06361.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B19">
    <label>19.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Rostoker G., Falthammer C.-G. Relationship between changes in the interplanetary magnetic field and variations in the magnetic field at the Earth’s surface. J. Geophys. Res. 1967. Vol. 72, iss. 23. P. 5853-5863. DOI: 10.1029/JZ072i023p05853.</mixed-citation>
     <mixed-citation xml:lang="en">Tsyganenko N.A., Sitnov M.I. Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms. J. Geophys. Res. 2005, vol. 110, A03208. DOI: 10.1029/2004 JA010798.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B20">
    <label>20.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Snyder C.W., Neugebauer M., Rao N.R. The solar wind velocity and its correlation with cosmic ray variations and with solar and geomagnetic activity. J. Geophys. Res. 1963. Vol. 68, iss. 24. P. 6361-6370. DOI: 10.1029/JZ068i024p06361.</mixed-citation>
     <mixed-citation xml:lang="en">Vaisberg O.L., Smirnov V.N., Zastenker G.N., Savin S.P., Verigin M.I. Plazmennaya geliogeofizika. T. 1: Vzaimodeistvie solnechnogo vetra s vneshnei magnitosferoi Zemli [Plasma Geliogeophysics. Ed. L.M. Zeleny, I.S. Veselovsky. Vol. 1: Interaction of the solar wind with the outer magnetosphere of the Earth]. Moscow, FIZMATLIT Publ., 2008. P. 378-422. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B21">
    <label>21.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Tsyganenko N.A., Sitnov M.I. Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms. J. Geophys. Res. 2005. Vol. 110, A03208. DOI: 10.1029/2004 JA010798.</mixed-citation>
     <mixed-citation xml:lang="en">Weygand J.M., McPherron R.L. Dependence of ring current asymmetry on storm phase. J. Geophys. Res. 2006, vol. 111, A11221. DOI: 10.1029/2006JA011808.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B22">
    <label>22.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Weygand J.M., McPherron R.L. Dependence of ring current asymmetry on storm phase. J. Geophys. Res. 2006. Vol. 111, A11221. DOI: 10.1029/2006JA011808.</mixed-citation>
     <mixed-citation xml:lang="en">Wilcox J.M., Schatten K.H., Ness N.F. Influence of interplanetary magnetic field and plasma on geomagnetic activity during quiet-sun condition. J. Geophys. Res. 1967, vol. 72, iss. 1, pp. 19-26. DOI: 10.1029/JZ072i001p00019.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B23">
    <label>23.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Wilcox J.M., Schatten K.H., Ness N.F. Influence of interplanetary magnetic field and plasma on geomagnetic activity during quiet-sun condition. J. Geophys. Res. 1967. Vol. 72, iss. 1. P. 19-26. DOI: 10.1029/JZ072i001p00019.</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. Cosmic Research. 2010, vol. 48, iss. 6, pp. 485-500. DOI: 10.1134/S0010952510060018.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B24">
    <label>24.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Yermolaev Yu.I., Lodkina I.G., Nikolaeva N.S., et al. Statistic study of the geoeffectiveness of compression regions CIRs and Sheaths. J. Atmos. Solar-Terr. Phys. 2018. Vol. 180. P. 52-59. DOI: 10.1016/j.jastp.2018.01.027.</mixed-citation>
     <mixed-citation xml:lang="en">Yermolaev Yu.I., Lodkina I.G., Nikolaeva N.S., Yermolaev M.Yu., Riazantseva M.O., Rakhmanova L.S. Statistic study of the geoeffectiveness of compression regions CIRs and Sheaths. J. Atmos. Solar-Terr. Phys. 2018, vol. 180, pp. 52-59. DOI: 10.1016/j.jastp.2018.01.027.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B25">
    <label>25.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: http://wdc.kugi.kyoto-u.ac.jp/aeasy/asy.pdf (дата обращения 29 марта 2022 г.).</mixed-citation>
     <mixed-citation xml:lang="en">URL: http://wdc.kugi.kyoto-u.ac.jp/aeasy/asy.pdf (accessed March 29, 2022).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B26">
    <label>26.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: http://omniweb.gsfc.nasa.gov (дата обращения 29 марта 2022 г.).</mixed-citation>
     <mixed-citation xml:lang="en">URL: http://omniweb.gsfc.nasa.gov (accessed March 29, 2022).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B27">
    <label>27.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: https://wdc.kugi.kyoto-u.ac.jp/index.html (дата обращения 29 марта 2022 г.).</mixed-citation>
     <mixed-citation xml:lang="en">URL: https://wdc.kugi.kyoto-u.ac.jp/index.html (accessed March 29, 2022).</mixed-citation>
    </citation-alternatives>
   </ref>
  </ref-list>
 </back>
</article>
