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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">77</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">Precursors of solar flares in the microwave range</article-title>
      </title-group>
      <contrib-group content-type="author">
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Abramov-Maximov</surname>
              <given-names>Vladimir</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-1"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Bakunina</surname>
              <given-names>Irina</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-2"/>
        </contrib>
      </contrib-group>
      <aff id="aff-1">
        <institution content-type="orgname" xml:lang="en">Central (Pulkovo) Astronomical Observatory of RAS, Pulkovskoye sh. 65/1, St. Petersburg 196140, Russia</institution>
      </aff>
      <aff id="aff-2">
        <institution content-type="orgname" xml:lang="en">HSE University, Bolshaya Pecherskaya 25/12, Nizhny Novgorod 603155, Russia</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2024-06-23">
        <day>23</day>
        <month>06</month>
        <year>2024</year>
      </pub-date>
      <volume>5</volume>
      <issue>2</issue>
      <fpage>13</fpage>
      <lpage>16</lpage>
      <history>
        <date date-type="received" iso-8601-date="2024-06-16">
          <day>16</day>
          <month>06</month>
          <year>2024</year>
        </date>
      </history>
      <permissions>
        <copyright-statement xml:lang="en">Copyright (c) 2024 Vladimir Abramov-Maximov, Irina Bakunina</copyright-statement>
        <copyright-year>
					2024
				</copyright-year>
        <copyright-holder xml:lang="en">Vladimir Abramov-Maximov, Irina Bakunina</copyright-holder>
        <license license-type="open-access" xlink:href="http://creativecommons.org/licenses/by/4.0" xml:lang="en">
          <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/77"/>
      <abstract xml:lang="en">
        <p> We present a study of the spatial distribution of quasiperiodic oscillations of microwave emission in two active regions before M-class flares. We have studied two events: NOAA 11283 on September 6 and NOAA 11302 on September 25, 2011. We used the Nobeyama Radioheliograph (NoRH) daily observations at a frequency of 17 GHz. In both cases we found the preflare wave trains of brightness temperature oscillations of microwave emission in active regions. The duration of wave trains is about 3–4 oscillation cycles. We found that the source of oscillations was a compact zone in the active region, which coincides with the area of maximum brightness during a flare. </p>
      </abstract>
      <kwd-group xml:lang="en">
        <kwd>Sun</kwd>
        <kwd>flares</kwd>
        <kwd>radio emission</kwd>
        <kwd>quasiperiodic oscillations</kwd>
      </kwd-group>
      <funding-group>
        <funding-statement xml:lang="en">
                                                    The work was carried out within the framework of the state assignment No. 1021032422589-5.
                                                </funding-statement>
      </funding-group>
      <counts>
        <page-count count="4"/>
      </counts>
    </article-meta>
  </front>
  <body/>
  <back>
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</article>
