<!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">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>Solar-Terrestrial Physics</trans-title>
    </trans-title-group>
   </journal-title-group>
   <issn publication-format="online">2500-0535</issn>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="publisher-id">23004</article-id>
   <article-id pub-id-type="doi">10.12737/stp-43201803</article-id>
   <article-categories>
    <subj-group subj-group-type="toc-heading" xml:lang="ru">
     <subject>Results of current research</subject>
    </subj-group>
    <subj-group subj-group-type="toc-heading" xml:lang="en">
     <subject>Results of current research</subject>
    </subj-group>
    <subj-group>
     <subject>Results of current research</subject>
    </subj-group>
   </article-categories>
   <title-group>
    <article-title xml:lang="en">Heliolatitude regularities of magnetically disturbed days with daily average geomagnetic index Dst&lt;–100 nT</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Heliolatitude regularities of magnetically disturbed days with daily average geomagnetic index Dst&lt;–100 nT</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>
   <volume>4</volume>
   <issue>3</issue>
   <fpage>20</fpage>
   <lpage>23</lpage>
   <self-uri xlink:href="https://zh-szf.ru/en/nauka/article/23004/view">https://zh-szf.ru/en/nauka/article/23004/view</self-uri>
   <abstract xml:lang="ru">
    <p>This paper considers storm days for a period 1966–2015 when the daily average geomagnetic Dst index was &lt;–100 nT. The distribution of the number of days with a high daily average Dst is shown to depend on Earth’s heliolatitude φ: the number of days increases with the absolute value of φ in both solar hemispheres. It is found, as expected, that the seasonal distribution of storm days with Dst&lt;–100 nT has equinoctial maxima. Moreover, there is a noticeable increase in the number of such days in July and November. It is noted that at Earth’s heliolatitudes 4.1°–5.0° there is a sharp increase in the number of storm days. It is established that this increase occurs during storm events in July and November, which stand out against the seasonal distribution of highly disturbed days.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>This paper considers storm days for a period 1966–2015 when the daily average geomagnetic Dst index was &lt;–100 nT. The distribution of the number of days with a high daily average Dst is shown to depend on Earth’s heliolatitude φ: the number of days increases with the absolute value of φ in both solar hemispheres. It is found, as expected, that the seasonal distribution of storm days with Dst&lt;–100 nT has equinoctial maxima. Moreover, there is a noticeable increase in the number of such days in July and November. It is noted that at Earth’s heliolatitudes 4.1°–5.0° there is a sharp increase in the number of storm days. It is established that this increase occurs during storm events in July and November, which stand out against the seasonal distribution of highly disturbed days.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>geomagnetic Dst index</kwd>
    <kwd>geomagnetic storm</kwd>
    <kwd>seasonal variation of magnetic activity</kwd>
    <kwd>Earth’s heliolatitude</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>geomagnetic Dst index</kwd>
    <kwd>geomagnetic storm</kwd>
    <kwd>seasonal variation of magnetic activity</kwd>
    <kwd>Earth’s heliolatitude</kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <p></p>
 </body>
 <back>
  <ref-list>
   <ref id="B1">
    <label>1.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Akasofu S.-I. Energy coupling between the solar wind and the magnetosphere. Space Sci. Rev. 1981, vol. 28, iss. 2, pp. 121-190. DOI: 10.1007/BF00218810.</mixed-citation>
     <mixed-citation xml:lang="en">Akasofu S.-I. Energy coupling between the solar wind and the magnetosphere. Space Sci. Rev. 1981, vol. 28, iss. 2, pp. 121-190. DOI: 10.1007/BF00218810.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B2">
    <label>2.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Bartels J. Terrestrial magnetic activity and its relations to solar phenomena. Terrestrial Magnetism. 1932, vol. 37, pp. 1-52.</mixed-citation>
     <mixed-citation xml:lang="en">Bartels J. Terrestrial magnetic activity and its relations to solar phenomena. Terrestrial Magnetism. 1932, vol. 37, pp. 1-52.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B3">
    <label>3.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Clúa de Gonzalez A.L., Silbergleit V.M., Gonzalez W.D., Tsurutani B.T. Irregularities in the semiannual variation of the geomagnetic activity. Adv. Space Res. 2002, vol. 30, iss. 10, pp. 2215-2218.</mixed-citation>
     <mixed-citation xml:lang="en">Clúa de Gonzalez A.L., Silbergleit V.M., Gonzalez W.D., Tsurutani B.T. Irregularities in the semiannual variation of the geomagnetic activity. Adv. Space Res. 2002, vol. 30, iss. 10, pp. 2215-2218.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B4">
    <label>4.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Cortie A.L. Sunspots and terrestrial magnetic phenomena, 1898-1911. Monthly Notices of the Royal Astronomical Society.1912, vol. 73, pp. 52-60.</mixed-citation>
     <mixed-citation xml:lang="en">Cortie A.L. Sunspots and terrestrial magnetic phenomena, 1898-1911. Monthly Notices of the Royal Astronomical Society.1912, vol. 73, pp. 52-60.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B5">
    <label>5.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Echer E., Gonzalez W.D., Tsurutani B.T., Clúa de Gonzalez A.L. Interplanetary conditions causing intense geomagnetic storms (Dst≤−100 nT) during solar cycle 23 (1996-2006). J. Geophys. Res. 2008, vol. 113, A05221. DOI: 10.1029/2007 JA012744.</mixed-citation>
     <mixed-citation xml:lang="en">Echer E., Gonzalez W.D., Tsurutani B.T., Clúa de Gonzalez A.L. Interplanetary conditions causing intense geomagnetic storms (Dst≤−100 nT) during solar cycle 23 (1996-2006). J. Geophys. Res. 2008, vol. 113, A05221. DOI: 10.1029/2007 JA012744.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B6">
    <label>6.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Echer E., Gonzalez W.D., Tsurutani B.T. Statistic studies of geomagnetic storms with peak Dst≤-50 nT from 1957 to 2008. J. Atmos. Solar-Terr. Phys. 2011, vol. 73, iss. 11-12, pp. 1454-1459. DOI: 10.1016/j.jastp.2011.04.021.</mixed-citation>
     <mixed-citation xml:lang="en">Echer E., Gonzalez W.D., Tsurutani B.T. Statistic studies of geomagnetic storms with peak Dst≤-50 nT from 1957 to 2008. J. Atmos. Solar-Terr. Phys. 2011, vol. 73, iss. 11-12, pp. 1454-1459. DOI: 10.1016/j.jastp.2011.04.021.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B7">
    <label>7.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Feldstein Y.I., Dremukhina L.A., Levitin A.E., Mall U., Alexeev I.I., Kalegaev V.V. Energetics of the magnetosphere during the magnetic storm. J. Atmos. Solar-Terr. Phys. 2003, vol. 65, iss. 4, pp. 429-446. DOI: 10.1016/S1364-6826(02)00339-5.</mixed-citation>
     <mixed-citation xml:lang="en">Feldstein Y.I., Dremukhina L.A., Levitin A.E., Mall U., Alexeev I.I., Kalegaev V.V. Energetics of the magnetosphere during the magnetic storm. J. Atmos. Solar-Terr. Phys. 2003, vol. 65, iss. 4, pp. 429-446. DOI: 10.1016/S1364-6826(02)00339-5.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B8">
    <label>8.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">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, pp. 5771-5792. DOI: 10.1029/93JA02867</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, pp. 5771-5792. DOI: 10.1029/93JA02867</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B9">
    <label>9.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Gonzalez W.D., Echer E., Tsurutani B.T., Clúa de Gonzalez A.L., Lago A.D. Interplanetary origin of intense, superintense and extreme geomagnetic storms. Space Sci. Rev. 2011, vol. 158, pp. 69-89. DOI: 10.1007/s11214-010-9715-2.</mixed-citation>
     <mixed-citation xml:lang="en">Gonzalez W.D., Echer E., Tsurutani B.T., Clúa de Gonzalez A.L., Lago A.D. Interplanetary origin of intense, superintense and extreme geomagnetic storms. Space Sci. Rev. 2011, vol. 158, pp. 69-89. DOI: 10.1007/s11214-010-9715-2.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B10">
    <label>10.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Gopalswamy N. Halo coronal mass ejections and geomagnetic storms. Earth, Planets and Space. 2009, vol. 61, pp. 1-3. DOI: 10.1186/BF03352930.</mixed-citation>
     <mixed-citation xml:lang="en">Gopalswamy N. Halo coronal mass ejections and geomagnetic storms. Earth, Planets and Space. 2009, vol. 61, pp. 1-3. DOI: 10.1186/BF03352930.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B11">
    <label>11.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Kovalenko V.A. Solnechnyi veter [Solar Wind]. Moscow, Nauka Publ., 1983. 271 p. (In Russian).</mixed-citation>
     <mixed-citation xml:lang="en">Kovalenko V.A. Solnechnyi veter [Solar Wind]. Moscow, Nauka Publ., 1983. 271 p. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B12">
    <label>12.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Mursula K., Tanskanen E., Love J.J. Spring-fall asymmetry of substorm strength, geomagnetic activity and solar wind: implications for semiannual variation and solar hemispheric asymmetry. Geophys. Res. Lett. 2011, vol. 38, L06104. DOI: 10.1029/2011GL046751.</mixed-citation>
     <mixed-citation xml:lang="en">Mursula K., Tanskanen E., Love J.J. Spring-fall asymmetry of substorm strength, geomagnetic activity and solar wind: implications for semiannual variation and solar hemispheric asymmetry. Geophys. Res. Lett. 2011, vol. 38, L06104. DOI: 10.1029/2011GL046751.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B13">
    <label>13.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Nikolaeva N.S., Yermolaev Yu.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>
     <mixed-citation xml:lang="en">Nikolaeva N.S., Yermolaev Yu.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="B14">
    <label>14.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Nikolaeva N.S., Yermolaev Yu.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>
     <mixed-citation xml:lang="en">Nikolaeva N.S., Yermolaev Yu.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="B15">
    <label>15.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Uwamahoro J., McKinnell L.-A. Solar and interplanetary precursors of geomagnetic storms in solar cycle 23. Adv. Space Res. 2013, vol. 51, iss. 3, pp. 395-410. DOI: 10.1016/j. asr.2012.09.034.</mixed-citation>
     <mixed-citation xml:lang="en">Uwamahoro J., McKinnell L.-A. Solar and interplanetary precursors of geomagnetic storms in solar cycle 23. Adv. Space Res. 2013, vol. 51, iss. 3, pp. 395-410. DOI: 10.1016/j. asr.2012.09.034.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B16">
    <label>16.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Yanovskii B.M. Zemnoi magnetizm [Terrestrial magnetism]. Leningrad, Leningrad State University Publ., 1978. 592 p. (In Russian).</mixed-citation>
     <mixed-citation xml:lang="en">Yanovskii B.M. Zemnoi magnetizm [Terrestrial magnetism]. Leningrad, Leningrad State University Publ., 1978. 592 p. (In Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B17">
    <label>17.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Yermolaev Yu.I., Yermolaev M.Yu. Statistical relationships between solar, interplanetary, and geomagnetospheric disturbances, 1976-2000. Cosmic Res. 2002. vol. 40, no. 1, pp. 1-14.</mixed-citation>
     <mixed-citation xml:lang="en">Yermolaev Yu.I., Yermolaev M.Yu. Statistical relationships between solar, interplanetary, and geomagnetospheric disturbances, 1976-2000. Cosmic Res. 2002. vol. 40, no. 1, pp. 1-14.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B18">
    <label>18.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Yermolaev Y.I., Yermolaev M.Y. Comment on ‘‘Interplanetary origin of intense geomagnetic storms (Dst&lt;-100 nT) during solar cycle 23’’ by W. D. Gonzalez et al. Geophys. Res. Lett. 2008, vol. 35, L01101. DOI: 10.1029/2007GL030281.</mixed-citation>
     <mixed-citation xml:lang="en">Yermolaev Y.I., Yermolaev M.Y. Comment on ‘‘Interplanetary origin of intense geomagnetic storms (Dst&lt;-100 nT) during solar cycle 23’’ by W. D. Gonzalez et al. Geophys. Res. Lett. 2008, vol. 35, L01101. DOI: 10.1029/2007GL030281.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B19">
    <label>19.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Yermolaev Y.I., Lodkina I.G., Nikolaeva N.S., Yermolaev M.Y., Riazantseva M.O. Some problems of identifying types of large-scale solar wind and their role in the physics of the magnetosphere. Cosmic Res. 2017, vol. 55, no. 3, pp. 178-189. DOI: 10.1134/S0010952517030029.</mixed-citation>
     <mixed-citation xml:lang="en">Yermolaev Y.I., Lodkina I.G., Nikolaeva N.S., Yermolaev M.Y., Riazantseva M.O. Some problems of identifying types of large-scale solar wind and their role in the physics of the magnetosphere. Cosmic Res. 2017, vol. 55, no. 3, pp. 178-189. DOI: 10.1134/S0010952517030029.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B20">
    <label>20.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Watari S. Geomagnetic storms of cycle 24 and their solar sources. Earth, Planets and Space. 2017, vol. 69, article 70. DOI: 10.1186/s40623-017-0653-z.</mixed-citation>
     <mixed-citation xml:lang="en">Watari S. Geomagnetic storms of cycle 24 and their solar sources. Earth, Planets and Space. 2017, vol. 69, article 70. DOI: 10.1186/s40623-017-0653-z.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B21">
    <label>21.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: http://wdc.kugi.kyoto-u.ac.jp/dstdir/index.html (accessed April 12, 2018).</mixed-citation>
     <mixed-citation xml:lang="en">URL: http://wdc.kugi.kyoto-u.ac.jp/dstdir/index.html (accessed April 12, 2018).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B22">
    <label>22.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: http://omniweb.gsfc.nasa.gov (accessed April 12, 2018).</mixed-citation>
     <mixed-citation xml:lang="en">URL: http://omniweb.gsfc.nasa.gov (accessed April 12, 2018).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B23">
    <label>23.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: http://sidc.oma.be (accessed April 12, 2018).</mixed-citation>
     <mixed-citation xml:lang="en">URL: http://sidc.oma.be (accessed April 12, 2018).</mixed-citation>
    </citation-alternatives>
   </ref>
  </ref-list>
 </back>
</article>
