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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" article-type="magnetism-and-activity-of-the-sun-and-stars--–-2021-conference-proceedings" xml:lang="en">
  <front>
    <journal-meta>
      <journal-id journal-id-type="ojs">aat</journal-id>
      <journal-id journal-id-type="publisher-id" xml:lang="en">
                       Acta Astrophys. Tau.
                </journal-id>
      <journal-title-group>
        <journal-title xml:lang="en">
                    Acta Astrophysica Taurica
                </journal-title>
      </journal-title-group>
      <issn pub-type="epub">2712-925X</issn>
      <publisher>
        <publisher-name>Kiselev Nikolai Nikolaevich,  Mosсow, settlement Moskovskii, Tat'yanin Park Str., 12, Moscow, Russia.</publisher-name>
        <publisher-loc>RU</publisher-loc>
      </publisher>
      <self-uri xlink:href="https://astrophysicatauricum.org/index.php/aat"/>
    </journal-meta>
    <article-meta>
      <article-id pub-id-type="publisher-id">41</article-id>
      <article-id pub-id-type="doi">10.34898/aat.vol3.iss2.pp22-26</article-id>
      <article-categories>
        <subj-group xml:lang="en" subj-group-type="heading">
          <subject>Magnetism and activity of the Sun and stars  – 2021 Conference proceedings</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title xml:lang="en">Characteristics of the radiation of polar coronal holes on the Sun in a wide range of radio waves</article-title>
      </title-group>
      <contrib-group content-type="author">
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Golubchina</surname>
              <given-names>O.A. </given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-1"/>
        </contrib>
      </contrib-group>
      <aff id="aff-1">
        <institution content-type="orgname" xml:lang="en">St. Petersburg Branch of the Special Astrophysical Observatory, St. Petersburg 196140, Russia</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2022-06-15">
        <day>15</day>
        <month>06</month>
        <year>2022</year>
      </pub-date>
      <volume>3</volume>
      <issue>2</issue>
      <fpage>22</fpage>
      <lpage>26</lpage>
      <history>
        <date date-type="received" iso-8601-date="2022-06-15">
          <day>15</day>
          <month>06</month>
          <year>2022</year>
        </date>
      </history>
      <permissions>
        <copyright-statement>
					Copyright (c)  Golubchina O.
				</copyright-statement>
        <copyright-year>
					
				</copyright-year>
        <copyright-holder>
					Golubchina O.
				</copyright-holder>
        <license xlink:href="http://creativecommons.org/licenses/by/4.0">
          <license-p> The metadata for this submission is licensed under a  Creative Commons Attribution 4.0 International License.  
 Copyright and publishing rights for texts published in  Acta Astrophysica Taurica  is retained by the authors, with first publication rights granted to the journal.Texts are free to use with proper attribution and link to the licensing  (Creative Commons Attribution 4.0 International).  
     </license-p>
        </license>
      </permissions>
      <self-uri xlink:href="https://astrophysicatauricum.org/index.php/aat/article/view/41"/>
      <abstract xml:lang="en">
        <p>  The paper presents a brief overview of the main results of observations of the radio emission in polar coronal holes on the Sun obtained in a wide range of wavelengths with various radio telescopes. We analyze the results of observations of the polar coronal hole with RATAN–600 in a wide centimeter wavelength range of (1.03–30.7) cm. The obtained physical characteristics of the coronal hole above the north pole of the Sun are compared with the characteristics of the coronal holes located at lower latitudes.   </p>
      </abstract>
      <kwd-group xml:lang="en">
        <kwd>Sun</kwd>
        <kwd>coronal holes</kwd>
        <kwd>radio emission</kwd>
      </kwd-group>
      <counts>
        <page-count count="5"/>
      </counts>
    </article-meta>
  </front>
  <body/>
  <back>
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</article>
