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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>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">33960</article-id>
   <article-id pub-id-type="doi">10.12737/stp-54201903</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">Solar spectropolarimeter for space weather forecast</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Solar spectropolarimeter for space weather forecast</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/0009-0006-7712-9330</contrib-id>
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Иванов</surname>
       <given-names>Евгений Федорович</given-names>
      </name>
      <name xml:lang="en">
       <surname>Ivanov</surname>
       <given-names>Evgeniy Fedorovich</given-names>
      </name>
     </name-alternatives>
     <email>eugenessrt@gmail.com</email>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Губин</surname>
       <given-names>Алексей Владимирович</given-names>
      </name>
      <name xml:lang="en">
       <surname>Gubin</surname>
       <given-names>Aleksey Vladimirovich</given-names>
      </name>
     </name-alternatives>
     <email>gubin@iszf.irk.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-2"/>
    </contrib>
    <contrib contrib-type="author">
     <contrib-id contrib-id-type="orcid">https://orcid.org/0009-0004-1651-1259</contrib-id>
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Лесовой</surname>
       <given-names>Сергей Владимирович</given-names>
      </name>
      <name xml:lang="en">
       <surname>Lesovoi</surname>
       <given-names>Sergey Vladimirovich</given-names>
      </name>
     </name-alternatives>
     <email>lesovoi@iszf.irk.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-3"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Эстрада</surname>
       <given-names>Рамзес Сальдивар </given-names>
      </name>
      <name xml:lang="en">
       <surname>Estrada</surname>
       <given-names>Ramses Zaldivar </given-names>
      </name>
     </name-alternatives>
     <email>ramses@iga.cu</email>
     <xref ref-type="aff" rid="aff-4"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Институт солнечно-земной физики СО РАН</institution>
     <city>Иркутск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Solar Terrestrial Physics SB RAS</institution>
     <city>Irkutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-2">
    <aff>
     <institution xml:lang="ru">Институт солнечно-земной физики СО РАН</institution>
     <city>Иркутск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Solar Terrestrial Physics SB RAS</institution>
     <city>Irkutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-3">
    <aff>
     <institution xml:lang="ru">Институт солнечно-земной физики СО РАН</institution>
     <city>Иркутск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Solar Terrestrial Physics SB RAS</institution>
     <city>Irkutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-4">
    <aff>
     <institution xml:lang="ru">Институт геофизики и астрономии Академии наук Кубы</institution>
     <city>Гавана</city>
     <country>Куба</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Geophysics and Astronomy, Cuban Academy of Sciences</institution>
     <city>Havana</city>
     <country>Cuba</country>
    </aff>
   </aff-alternatives>
   <volume>5</volume>
   <issue>4</issue>
   <fpage>21</fpage>
   <lpage>26</lpage>
   <self-uri xlink:href="https://naukaru.ru/en/nauka/article/33960/view">https://naukaru.ru/en/nauka/article/33960/view</self-uri>
   <abstract xml:lang="ru">
    <p>We propose a project of the meter wavelength range solar spectropolarimeter designed for a ground-based network developing for space weather forecast. The Software-Defined Radio (SDR) solution is chosen to meet such instrument network requirements as specification identity, low cost, possibility of controlling and transmitting data remotely via the Internet. Along with these requirements, the proposed SDR solution allows us to measure Stokes I and V easily, which contrasts the proposed instrument with e-CALLISTO network spectropolarimeters, most of which can record only one linear polarization. Deployment of such instruments at various longitudes will allow continuous observation of type II bursts, often related to coronal mass ejections (CMEs) — the most geoeffective solar activity events that affect the space weather significantly.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>We propose a project of the meter wavelength range solar spectropolarimeter designed for a ground-based network developing for space weather forecast. The Software-Defined Radio (SDR) solution is chosen to meet such instrument network requirements as specification identity, low cost, possibility of controlling and transmitting data remotely via the Internet. Along with these requirements, the proposed SDR solution allows us to measure Stokes I and V easily, which contrasts the proposed instrument with e-CALLISTO network spectropolarimeters, most of which can record only one linear polarization. Deployment of such instruments at various longitudes will allow continuous observation of type II bursts, often related to coronal mass ejections (CMEs) — the most geoeffective solar activity events that affect the space weather significantly.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>space weather</kwd>
    <kwd>solar radio emission</kwd>
    <kwd>dynamic spectrum</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>space weather</kwd>
    <kwd>solar radio emission</kwd>
    <kwd>dynamic spectrum</kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <p></p>
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     <mixed-citation xml:lang="ru">URL: https://wiki.analog.com/resources/eval/userguides/ arradio (accessed 30 September 2019).</mixed-citation>
     <mixed-citation xml:lang="en">URL: https://wiki.analog.com/resources/eval/userguides/ arradio (accessed 30 September 2019).</mixed-citation>
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    <label>28.</label>
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     <mixed-citation xml:lang="ru">URL: https://rocketboards.org/foswiki/Documentation/DE10 Standard (accessed 30 September 2019).</mixed-citation>
     <mixed-citation xml:lang="en">URL: https://rocketboards.org/foswiki/Documentation/DE10 Standard (accessed 30 September 2019).</mixed-citation>
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    <label>29.</label>
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     <mixed-citation xml:lang="ru">URL: https://www.analog.com/en/design-center/landing-pages/001/integrated-rf-agile-transceiver-design-resources.html (accessed 30 September 2019).</mixed-citation>
     <mixed-citation xml:lang="en">URL: https://www.analog.com/en/design-center/landing-pages/001/integrated-rf-agile-transceiver-design-resources.html (accessed 30 September 2019).</mixed-citation>
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    <label>30.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: https://www.analog.com/ru/analog-dialogue/articles/ mirror-mirror-on-the-wall-understanding-image-rejection-and-its-impact-on-desired-signals.html (accessed 30 September 2019).</mixed-citation>
     <mixed-citation xml:lang="en">URL: https://www.analog.com/ru/analog-dialogue/articles/ mirror-mirror-on-the-wall-understanding-image-rejection-and-its-impact-on-desired-signals.html (accessed 30 September 2019).</mixed-citation>
    </citation-alternatives>
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   <ref id="B31">
    <label>31.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: http://www.ntp.org/ntpfaq/NTP-s-algo.htm (accessed 30 September 2019).</mixed-citation>
     <mixed-citation xml:lang="en">URL: http://www.ntp.org/ntpfaq/NTP-s-algo.htm (accessed 30 September 2019).</mixed-citation>
    </citation-alternatives>
   </ref>
  </ref-list>
 </back>
</article>
