<?xml version="1.0"?>
<!DOCTYPE article
PUBLIC "-//NLM//DTD JATS (Z39.96) Journal Publishing DTD v1.4 20190208//EN"
       "JATS-journalpublishing1.dtd">
<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" article-type="research-article" dtd-version="1.4" xml:lang="en">
 <front>
  <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">43812</article-id>
   <article-id pub-id-type="doi">10.12737/szf-74202103</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">Studying auroral activity using the SME index at the magnetic storm main phase during CIR and ICME events</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Исследование авроральной активности по данным SME-индекса на главных фазах магнитных бурь во время CIR- и ICME-событий</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Бороев</surname>
       <given-names>Роман Николаевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Boroev</surname>
       <given-names>Roman Nikolaevich</given-names>
      </name>
     </name-alternatives>
     <email>boroyev@ikfia.ysn.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"/>
     <xref ref-type="aff" rid="aff-2"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Васильев</surname>
       <given-names>Михаил Семенович</given-names>
      </name>
      <name xml:lang="en">
       <surname>Vasiliev</surname>
       <given-names>Mikhail Semenovich</given-names>
      </name>
     </name-alternatives>
     <email>m.s.vasiliev@ikfia.ysn.ru</email>
     <xref ref-type="aff" rid="aff-3"/>
     <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">M.K. Ammosov 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 of SB RAS</institution>
     <city>Yakutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-4">
    <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">M.K. Ammosov North-Eastern Federal University</institution>
     <city>Yakutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <pub-date publication-format="print" date-type="pub" iso-8601-date="2021-12-20T00:00:00+03:00">
    <day>20</day>
    <month>12</month>
    <year>2021</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2021-12-20T00:00:00+03:00">
    <day>20</day>
    <month>12</month>
    <year>2021</year>
   </pub-date>
   <volume>7</volume>
   <issue>4</issue>
   <fpage>19</fpage>
   <lpage>24</lpage>
   <history>
    <date date-type="received" iso-8601-date="2021-04-28T00:00:00+03:00">
     <day>28</day>
     <month>04</month>
     <year>2021</year>
    </date>
    <date date-type="accepted" iso-8601-date="2021-08-16T00:00:00+03:00">
     <day>16</day>
     <month>08</month>
     <year>2021</year>
    </date>
   </history>
   <self-uri xlink:href="https://zh-szf.ru/en/nauka/article/43812/view">https://zh-szf.ru/en/nauka/article/43812/view</self-uri>
   <abstract xml:lang="ru">
    <p>В работе исследована связь SME-ин-декса с характеристиками магнитной бури и параметрами межпланетной среды на главных фазах магнитных бурь, вызванных разными типами солнечного ветра (СВ). За период 1990–2017 гг. было отобрано 107 магнитных бурь, индуцированных событиями (64) CIR и (43) ICME. Показано, что, по сравнению с АЕ и Kр, наблюдается более сильная корреляция между средним значением SME-индекса (SMEaver) и параметрами межпланетной среды на главных фазах магнитных бурь. Получены близкие значения коэффициентов корреляций между SMEaver и электрическим полем СВ (южной Bz ММП) для событий CIR и  ICME. Установлено, что значения SMEaver-индекса увеличиваются с ростом скорости развития магнитной бури и |Dstmin|. Различий в уравнениях линейных регрессий между SMEaver и |Dstmin| для событий CIR и ICME не обнаружено.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>. In this paper, we examine the relationship of the SME index with magnetic storm characteristics and interplanetary medium parameters during the main phase of magnetic storms caused by CIR and ICME events. Over the period 1990–2017, 107 magnetic storms driven by (64) CIR and (43) ICME events have been selected. In contrast to AE and Kp, a stronger correlation is shown to exist between the average SME index (SMEaver) and interplanetary medium parameters during the magnetic storm main phase. Close correlation coefficients between SMEaver and the SW electric field (southward IMF Bz) have been obtained for CIR and ICME events. SMEaver has been found to increase with the rate of magnetic storm development and |Dstmin|. For CIR and ICME events, no difference has been revealed between SMEaver and |Dstmin| in linear regression equations.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>магнитная буря</kwd>
    <kwd>SME-индекс</kwd>
    <kwd>Dst-индекс</kwd>
    <kwd>солнечный ветер</kwd>
    <kwd>электрическое поле</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>magnetic storm</kwd>
    <kwd>SME index</kwd>
    <kwd>Dst index</kwd>
    <kwd>solar wind</kwd>
    <kwd>electric field</kwd>
   </kwd-group>
   <funding-group>
    <funding-statement xml:lang="ru">Работа выполнена в рамках государственного задания (номер госрегистрации № АААА-А21-121012 000007-4).</funding-statement>
    <funding-statement xml:lang="en">The work was carried out in the framework of Government Assignment (State Registration Number AAAA A21-121012000007-4).</funding-statement>
   </funding-group>
  </article-meta>
 </front>
 <body>
  <p></p>
 </body>
 <back>
  <ref-list>
   <ref id="B1">
    <label>1.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Акасофу С.Е., Чепмен С. Солнечно-земная физика. Часть 1. М.: Мир, 1974. 384 с.</mixed-citation>
     <mixed-citation xml:lang="en">Akasofu S.-I., Chapman S. Solnechno-zemnaya fizika. Chast’1. [Solar-Terrestrial Physics. Pt. 1]. Moscow, Mir Publ., 1974, 384 p. (In Russian). (English edition: Akasofu S.-I., Chapman S. Solar-Terrestrial Physics. Oxford, Clarendon Press, 1972, 901 p.)</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B2">
    <label>2.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Дремухина Л.А., Лодкина И.Г., Ермолаев Ю.И. Cвязь параметров солнечного ветра разных типов c индексами геомагнитной активности. Космические исследования. 2018а. Т. 56, № 6. С. 410-419. DOI: 10.31857/S002342060002487-3.</mixed-citation>
     <mixed-citation xml:lang="en">Bartels J. The standardized index Ks and the planetary index Kp. IATME Bull. 1949, no. 12b, pp. 97-120.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B3">
    <label>3.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Дремухина Л.А., Лодкина И.Г., Ермолаев Ю.И. Статистическое исследование воздействия солнечного ветра разных типов на генерацию магнитных бурь в период 1995-2016 гг. Геомагнетизм и аэрономия. 2018б. Т. 58, № 6. C. 760-768. DOI: 10.1134/S0016794018060032.</mixed-citation>
     <mixed-citation xml:lang="en">Borovsky J.E., Denton M.H. Differences between CME driven storms and CIR driven storms. J. Geophys. Res. 2006, vol. 111, A07S08. DOI: 10.1029/2005JA011447.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B4">
    <label>4.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Ермолаев Ю.И., Николаева Н.С., Лодкина И.Г., Ермолаев М.Ю. Каталог крупномасштабных явлений солнечного ветра для периода 1976-2000 гг. Космические исследования. 2009. Т. 47, № 2. С. 99-113.</mixed-citation>
     <mixed-citation xml:lang="en">Borovsky J.E., Birn J. The solar wind electric field does not control the dayside reconnection rate.  J. Geophys. Res. 2014, vol. 119, pp. 751-760. DOI: 10.1002/2013JA019193.</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.Ю. Зависит ли длительность фазы восстановления магнитной бури от скорости развития бури на ее главной фазе? Геомагнетизм и аэрономия. 2015. Т. 55, № 4. C. 435-439. DOI: 10.7868/S0016794015040033.</mixed-citation>
     <mixed-citation xml:lang="en">Boroyev R.N., Vasiliev M.S. Substorm activity during the main phase of magnetic storms induced by the CIR and ICME events. Adv. Space Res. 2018, vol. 61, pp. 348-354.DOI: 10.1016/j.asr.2017.10.031.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B6">
    <label>6.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Николаева Н.С., Ермолаев Ю.И., Лодкина И.Г. Зависимость геомагнитной активности во время магнитных бурь от параметров солнечного ветра для разных типов течений. Геомагнетизм и аэрономия. 2011. Т. 51, № 1. C. 51-67.</mixed-citation>
     <mixed-citation xml:lang="en">Boroyev R.N., Vasiliev M.S., Baishev D.G. The relationship between geomagnetic indices and the interplanetary medium parameters in magnetic storm main phases during CIR and ICME events. J. Atmos. Solar-Terr. Phys. 2020, vol. 204, 105290. DOI: 10.1016/j.jastp.2020.105290.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B7">
    <label>7.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Николаева Н.С., Ермолаев Ю.И., Лодкина И.Г., Ермолаев М.Ю. Зависит ли генерация магнитной бури от типа солнечного ветра? Геомагнетизм и аэрономия. 2017. Т. 57, № 5. С. 555-561. DOI: 10.7868/S0016794017050169.</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, pp. 4204-4214. DOI: 10.1029/JA 080i031p04204.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B8">
    <label>8.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Хорошева О.В. Связь геомагнитных возмущений с динамикой магнитосферы и параметрами межпланетной среды. Геомагнетизм и аэрономия. 2007. Т. 47, № 5. C. 579-583.</mixed-citation>
     <mixed-citation xml:lang="en">Cramer W.D., Turner N.E., Fok M.C., Buzulukova N.Y. Effects of different geomagnetic storm drivers on the ring current: CRCM results. J. Geophys. Res. 2013, vol. 118, pp. 1062-1073. DOI: 10.1002/jgra.50138.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B9">
    <label>9.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Bartels J. The standardized index Ks and the planetary index Kp. IATME Bull. 1949. No. 12b. P. 97-120.</mixed-citation>
     <mixed-citation xml:lang="en">Davis T.N., Sugiura M. Auroral electrojet activity index AE and its universal time variations. J. Geophys. Res. 1966, vol. 71, pp. 785-801. DOI: 10.1029/JZ071i003p00785.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B10">
    <label>10.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Borovsky J.E., Denton M.H. Differences between CME driven storms and CIR driven storms. J. Geophys. Res. 2006. Vol. 111, A07S08. DOI: 10.1029/2005JA011447.</mixed-citation>
     <mixed-citation xml:lang="en">Dremukhina L.A., Lodkina I.G., Yermolaev Y.I. Relationship between the parameters of various solar wind types and geomagnetic activity indices. Cosmic Res. 2018a, vol. 56, no. 6, pp. 426-433. DOI: 10.1134/S0010952518060011.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B11">
    <label>11.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Borovsky J.E., Birn J. The solar wind electric field does not control the dayside reconnection rate. J. Geophys. Res. 2014. Vol. 119. P. 751-760. DOI: 10.1002/2013JA019193.</mixed-citation>
     <mixed-citation xml:lang="en">Dremukhina L.A., Lodkina I.G., Yermolaev Y.I. Statistical study of the effect of different solar wind types on magnetic storm generation during 1995-2016. Geomagnetism and Aeronomy. 2018b, vol. 58, no. 6, pp. 737-743. DOI: 10.1134/S0016793218060038.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B12">
    <label>12.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Boroyev R.N., Vasiliev M.S. Substorm activity during the main phase of magnetic storms induced by the CIR and ICME events. Adv. Space Res. 2018. Vol. 61. P. 348-354. DOI: 10.1016/j.asr.2017.10.031.</mixed-citation>
     <mixed-citation xml:lang="en">Du A.M., Wang K.T., Luo H., Tsurutani B.T., JesperGjerloev, Wei Sun, Wang Y., Jiaming Ou, Yasong Ge. Coupling of semiannual and annual variations in the SuperMAG SML and SMU indices. Planet. Space Sci. 2018, vol. 158, pp. 87-95. DOI: 10.1016/j.pss.2018.05.001.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B13">
    <label>13.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Boroyev R.N., Vasiliev M.S., Baishev D.G. The relationship between geomagnetic indices and the interplanetary medium parameters in magnetic storm main phases during CIR and ICME events. J. Atmos. Solar-Terr. Phys. 2020. Vol. 204, 105290. DOI: 10.1016/j.jastp.2020.105290.</mixed-citation>
     <mixed-citation xml:lang="en">Gonzalez W.D., Joselyn J.A., Kamide Y., Kroehl H.W., Rostoker G., Tsurutani B.T., Vasyliunas V.M. What is a geomagnetic storm? J. Geophys. Res. 1994, vol. 99, iss. A4, pp. 5771-5792. DOI: 10.1029/93JA02867.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B14">
    <label>14.</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. P. 4204-4214. DOI: 10.1029/ JA080i031p04204.</mixed-citation>
     <mixed-citation xml:lang="en">Gonzalez W.D., Tsurutani B.T., Gonzalez A.L.C. Interplanetary origin of geomagnetic storms. Space Sci. Rev. 1999, vol. 88, pp. 529-562. DOI: 10.1023/A:1005160129098.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B15">
    <label>15.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Cramer W.D., Turner N.E., Fok M.C., Buzulukova N.Y. Effects of different geomagnetic storm drivers on the ring cur-rent: CRCM results. J. Geophys. Res. 2013. Vol. 118. P. 1062-1073. DOI: 10.1002/jgra.50138.</mixed-citation>
     <mixed-citation xml:lang="en">Grafe A., Feldstein Y.I. About the relationship between auroral electrojets and ring currents. Ann. Geophys. 2000, vol. 18, pp. 874-886. DOI: 10.1007/s00585-000-0874-4.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B16">
    <label>16.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Davis T.N., Sugiura M. Auroral electrojet activity index AE and its universal time variations. J. Geophys. Res. 1966. Vol. 71. P. 785-801. DOI: 10.1029/JZ071i003p00785.</mixed-citation>
     <mixed-citation xml:lang="en">Grafe A., Bespalov P.A., Trakhtengerts V.Y., Demekhov A.G. Afternoon mid-latitude current system and low-latitude geomagnetic field asymmetry during geomagnetic storms. Ann. Geophys. 1997, vol. 15, pp. 1537-1547. DOI: 10.1007/s00585-997-1537-5.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B17">
    <label>17.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Du A.M., Wang K.T., Luo H., et al. Coupling of semiannual and annual variations in the SuperMAG SML and SMU indices. Planet. Space Sci. 2018. Vol. 158. P. 87-95. DOI: 10.1016/ j.pss.2018.05.001.</mixed-citation>
     <mixed-citation xml:lang="en">Guo J., Feng X., Emery B.A., Zhang J., Xiang C., Shen F., Song W. Energy transfer during intense geomagnetic storms driven by interplanetary coronal mass ejections and their sheath regions. J. Geophys. Res. 2011, vol. 116, A05106. DOI: 10.1029/ 2011jA016490.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B18">
    <label>18.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Gonzalez W.D., Joselyn J.A., Kamide Y., et al.  What is a geomagnetic storm? J. Geophys. Res. 1994. Vol. 99, iss. A4. P. 5771-5792. DOI: 10.1029/93JA02867.</mixed-citation>
     <mixed-citation xml:lang="en">Kane R.P. How good is the relationship of solar and interplanetary plasma parameters with geomagnetic storms? J. Geophys. Res. 2005, vol. 110, A02213. DOI: 10.1029/2004JA 010799.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B19">
    <label>19.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Gonzalez W.D., Tsurutani B.T., Gonzalez A.L.C. Interplanetary origin of geomagnetic storms. Space Sci. Rev. 1999. Vol. 88. P. 529-562. DOI: 10.1023/A:1005160129098.</mixed-citation>
     <mixed-citation xml:lang="en">Kane R.P. Scatter in the plots of Dst(min) versus Bz(min). Planet. Space Sci. 2010, vol. 58, pp. 1792-1801. DOI: 10.1016/j.pss.2010.07.026.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B20">
    <label>20.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Grafe A., Feldstein Y.I. About the relationship between auroral electrojets and ring currents. Ann. Geophys. 2000. Vol. 18. P. 874-886. DOI: 10.1007/s00585-000-0874-4.</mixed-citation>
     <mixed-citation xml:lang="en">Khorosheva O.V. Relation of geomagnetic disturbances to the dynamics of the magnetosphere and the parameters of the interplanetary medium. Geomagnetism and Aeronomy. 2007, vol. 47, no. 5, pp. 543-547. DOI: 10.1134/S0016793207050015.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B21">
    <label>21.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Grafe A., Bespalov P.A., Trakhtengerts V.Y., Demekhov A.G. Afternoon mid-latitude current system and low-latitude geomagnetic field asymmetry during geomagnetic storms. Ann. Geophys. 1997. Vol. 15. P. 1537-1547. DOI: 10.1007/s00585-997-1537-5.</mixed-citation>
     <mixed-citation xml:lang="en">Maltsev Yu.P., Rezhenov B.V. Relation of the Dst index to solar wind parameters. International Journal of Geomagnetism and Aeronomy. 2003, vol. 4, no. 1, pp. 1-9.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B22">
    <label>22.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Guo J., Feng X., Emery B.A., et al. Energy transfer during intense geomagnetic storms driven by interplanetary coronal mass ejections and their sheath regions. J. Geophys. Res. 2011. Vol. 116, A05106. DOI: 10.1029/2011jA016490.</mixed-citation>
     <mixed-citation xml:lang="en">Newell P.T., Gjerloev J.W. Substorm and magnetosphere characteristic scales inferred from the SuperMAG auroral electrojet indices. J. Geophys. Res. 2011, vol. 116, A12232. DOI: 10.1029/2011JA016936.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B23">
    <label>23.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Kane R.P. How good is the relationship of solar and interplanetary plasma parameters with geomagnetic storms? J. Geophys. Res. 2005. Vol. 110, A02213. DOI: 10.1029/2004J A010799.</mixed-citation>
     <mixed-citation xml:lang="en">Newell P.T., Gjerloev J.W. SuperMAG-based partial ring current indices. J. Geophys. Res. 2012, vol. 117, A05215. DOI: 10.1029/2012JA017586.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B24">
    <label>24.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Kane R.P. Scatter in the plots of Dst(min) versus Bz(min). Planet. Space Sci. 2010. Vol. 58. P. 1792-1801. DOI: 10.1016/j.pss.2010.07.026.</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="B25">
    <label>25.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Maltsev Yu.P., Rezhenov B.V. Relation of the Dst-index to solar wind parameters. International Journal of Geomagnetism and Aeronomy. 2003. Vol. 4, no. 1. P. 1-9.</mixed-citation>
     <mixed-citation xml:lang="en">Newell P.T., Gjerloev J.W., Mitchell E.J. Space climate implications from substorm frequency. J. Geophys. Res. 2013, vol. 118, pp. 6254-6265. DOI: 10.1002/jgra.50597.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B26">
    <label>26.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Newell P.T., Gjerloev J.W. Substorm and magnetosphere characteristic scales inferred from the SuperMAG auroral electrojet indices. J. Geophys. Res. 2011. Vol. 116, A12232. DOI: 10.1029/2011JA016936.</mixed-citation>
     <mixed-citation xml:lang="en">Nikolaeva N.S., Yermolaev Y.I., Lodkina I.G. Dependence of geomagnetic activity during magnetic storms on the solar wind parameters for different types of streams. Geomagnetism and Aeronomy. 2011, vol. 51, no. 1, pp. 49-65. DOI: 10.1134/S0016793211010099.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B27">
    <label>27.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Newell P.T., Gjerloev J.W. SuperMAG-based partial ring current indices. J. Geophys. Res. 2012. Vol. 117, A05215. DOI: 10.1029/2012JA017586.</mixed-citation>
     <mixed-citation xml:lang="en">Nikolaeva N.S., Yermolaev Y.I., Lodkina I.G., Yermolaev M.Y. Does magnetic storm generation depend on the solar wind type? Geomagnetism and Aeronomy. 2017, vol. 57, no. 5, pp. 512-518. DOI: 10.1134/S0016793217050152.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B28">
    <label>28.</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">Plotnikov I.Ya., Barkova E.S. Advances in space research nonlinear dependence of Dst and AE indices on the electric field of magnetic clouds. Adv. Space Res. 2007, vol. 40, pp. 1858-1862. DOI: 10.1016/j.asr.2007.09.025.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B29">
    <label>29.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Newell P.T., Gjerloev J.W., Mitchell E.J. Space climate implications from substorm frequency. J. Geophys. Res. 2013. Vol. 118. P. 6254-6265. DOI: 10.1002/jgra.50597.</mixed-citation>
     <mixed-citation xml:lang="en">Sugiura M. Hourly values of the equatorial Dst for IGY. Annales of the International Geophysical Year. 1964, vol. 35. pp. 9-45.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B30">
    <label>30.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Plotnikov I.Ya., Barkova E.S. Advances in space research nonlinear dependence of Dst and AE indices on the electric field of magnetic clouds. Adv. Space Res. 2007. Vol. 40. P. 1858-1862. DOI: 10.1016/j.asr.2007.09.025.</mixed-citation>
     <mixed-citation xml:lang="en">Yermolaev Yu.I., Nikolaeva N.S., Lodkina I.G., Yermolaev M.Yu. Catalog of large-scale solar wind phenomena during 1976-2000. Cosmic Res. 2009, vol. 47, no. 2, pp. 81-94. DOI: 10.1134/S0010952509020014.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B31">
    <label>31.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Sugiura M. Hourly values of the equatorial Dst for IGY. Annales of the International Geophysical Year. 1964. Vol. 35. P. 9-45.</mixed-citation>
     <mixed-citation xml:lang="en">Yermolaev Yu.I., Nikolaeva N.S., Lodkina I.G., Yermolaev M.Yu. Specific interplanetary conditions for CIR-, Sheath-, and ICME-induced geomagnetic storms obtained by double superposed epoch analysis. Ann. Geophys. 2010, vol. 28, pp. 2177-2186. DOI: 10.5194/angeo-28-1-2010.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B32">
    <label>32.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Yermolaev Yu.I., Nikolaeva N.S., Lodkina I.G., Yermolaev M.Yu. Specific interplanetary conditions for CIR-, Sheath-, and ICME- induced geomagnetic storms obtained by double superposed epoch analysis. Ann. Geophys. 2010. Vol. 28. P. 2177-2186. DOI: 10.5194/angeo-28-1-2010.</mixed-citation>
     <mixed-citation xml:lang="en">Yermolaev Y.I., Nikolaeva N.S., Lodkina I.G., Yermolaev M.Y. Geoeffectiveness and efficiency of CIR, sheath, and ICME in generation of magnetic storms. J. Geophys. Res. 2012, vol. 117, A00L07. DOI: 10.1029/2011JA017139.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B33">
    <label>33.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Yermolaev Y.I., Nikolaeva N.S., Lodkina I.G., Yermolaev M.Y. Geoeffectiveness and efficiency of CIR, sheath, and ICME in generation of magnetic storms. J. Geophys. Res. 2012. Vol. 117, A00L07. DOI: 10.1029/2011JA017139.</mixed-citation>
     <mixed-citation xml:lang="en">Yermolaev Y.I., Lodkina I.G., Nikolaeva N.S., Yermolaev M.Y. Does the duration of the magnetic storm recovery phase depend on the storm development rate in its main phase? Geomagnetism and Aeronomy. 2015, vol. 55, no. 4, pp. 421-424. DOI: 10.1134/S0016793215040039.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B34">
    <label>34.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Yermolaev, Y.I., Lodkina, I.G., Nikolaeva, N.S., Yermolaev M.Y. Dynamics of large-scale solar-wind streams obtained by the double superposed epoch analysis: 2. Comparisons of CIRs vs. Sheaths and MCs vs. Ejecta. Solar Phys. 2017. Vol. 292, 193. DOI: 10.1007/s11207-017-1205-1.</mixed-citation>
     <mixed-citation xml:lang="en">Yermolaev Y.I., Lodkina I.G., Nikolaeva N.S., Yermolaev M.Y. Dynamics of large-scale solar-wind streams obtained by the double superposed epoch analysis: 2. Comparisons of CIRs vs. Sheaths and MCs vs. Ejecta. Solar Phys. 2017, vol. 292, 193. DOI: 10.1007/s11207-017-1205-1.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B35">
    <label>35.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Yermolaev Y.I., Lodkina I.G., Dremukhina L.A., et al. What solar-terrestrial link researchers should know about interplanetary drivers. Universe. 2021. Vol. 7, iss. 5, 138. DOI: 10.3390/ universe7050138.</mixed-citation>
     <mixed-citation xml:lang="en">Yermolaev Y.I., Lodkina I.G., Dremukhina L.A., Yermolaev M.Y., Khokhlachev A.A. What solar-terrestrial link researchers should know about interplanetary drivers. Universe. 2021, vol. 7, iss. 5, 138. DOI: 10.3390/universe7050138.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B36">
    <label>36.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: https://supermag.jhuapl.edu (дата обращения 2 марта 2021 г.).</mixed-citation>
     <mixed-citation xml:lang="en">URL: https://supermag.jhuapl.edu (accessed March 2, 2021).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B37">
    <label>37.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: http://wdc.kugi.kyoto-u.ac.jp/dstae/index.html (дата обращения 2 марта 2021 г.).</mixed-citation>
     <mixed-citation xml:lang="en">URL: http://wdc.kugi.kyoto-u.ac.jp/dstae/index.html (accessed March 2, 2021).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B38">
    <label>38.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: ftp.iki.rssi.ru/pub/omni/catalog (дата обращения 2 марта 2021 г.).</mixed-citation>
     <mixed-citation xml:lang="en">URL: ftp.iki.rssi.ru/pub/omni/catalog (accessed March 2, 2021).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B39">
    <label>39.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: http://www.omniweb.com (дата обращения 2 марта 2021 г.).</mixed-citation>
     <mixed-citation xml:lang="en">URL: http://www.omniweb.com (accessed March 2, 2021).</mixed-citation>
    </citation-alternatives>
   </ref>
  </ref-list>
 </back>
</article>
