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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">122591</article-id>
   <article-id pub-id-type="doi">10.12737/stp-122202609</article-id>
   <article-id pub-id-type="edn">nrjatv</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">Method for estimating parameters of multi-mode signals measured at SECIRA radars</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Method for estimating parameters of multi-mode signals measured at SECIRA radars</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/0000-0002-3837-8207</contrib-id>
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Бернгардт</surname>
       <given-names>Олег Игоревич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Berngardt</surname>
       <given-names>Oleg Igorevich</given-names>
      </name>
     </name-alternatives>
     <email>berng@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-1"/>
    </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>
   <volume>12</volume>
   <issue>2</issue>
   <fpage>76</fpage>
   <lpage>88</lpage>
   <history>
    <date date-type="received" iso-8601-date="2025-07-18T00:00:00+03:00">
     <day>18</day>
     <month>07</month>
     <year>2025</year>
    </date>
    <date date-type="accepted" iso-8601-date="2026-01-23T00:00:00+03:00">
     <day>23</day>
     <month>01</month>
     <year>2026</year>
    </date>
   </history>
   <self-uri xlink:href="https://naukaru.ru/en/nauka/article/122591/view">https://naukaru.ru/en/nauka/article/122591/view</self-uri>
   <abstract xml:lang="ru">
    <p>The paper presents the algorithm for evaluating parameters of coherent scattering signals, which is based on the assessment of their parametric spectra by the well-known autoregression ARMA(10,10) model. The assessment consists of autoregression over 10 sequence members, moving average over residuals for 10 sequence members, and subsequent fitting of the resulting spectra with the sum of gaussian functions. The algorithm is a development of Burg’s method, previously proposed for the analysis of SuperDARN data. It differs from the method in the use of a more complex regression model, consideration of characteristics of the correlation function, and determination of three parameters for each peak (mode) — amplitude, Doppler velocity, and spectral width. Comparison shows that the best continuity between the parameters of multi-mode signals, obtained by new and standard signal processing methods, is provided by analysis of the mode with maximum integral power. The analysis has revealed that new and standard methods in the case of single-mode signals give close Doppler velocities. The multi-mode analysis presented in the paper increases the number of detected signals of various types, and can be employed to expand the diagnostic capabilities of SECIRA/SuperDARN radars, including automatic classification of each mode.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>The paper presents the algorithm for evaluating parameters of coherent scattering signals, which is based on the assessment of their parametric spectra by the well-known autoregression ARMA(10,10) model. The assessment consists of autoregression over 10 sequence members, moving average over residuals for 10 sequence members, and subsequent fitting of the resulting spectra with the sum of gaussian functions. The algorithm is a development of Burg’s method, previously proposed for the analysis of SuperDARN data. It differs from the method in the use of a more complex regression model, consideration of characteristics of the correlation function, and determination of three parameters for each peak (mode) — amplitude, Doppler velocity, and spectral width. Comparison shows that the best continuity between the parameters of multi-mode signals, obtained by new and standard signal processing methods, is provided by analysis of the mode with maximum integral power. The analysis has revealed that new and standard methods in the case of single-mode signals give close Doppler velocities. The multi-mode analysis presented in the paper increases the number of detected signals of various types, and can be employed to expand the diagnostic capabilities of SECIRA/SuperDARN radars, including automatic classification of each mode.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>decameter radar</kwd>
    <kwd>SECIRA</kwd>
    <kwd>ionosphere</kwd>
    <kwd>multi-mode signals</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>decameter radar</kwd>
    <kwd>SECIRA</kwd>
    <kwd>ionosphere</kwd>
    <kwd>multi-mode signals</kwd>
   </kwd-group>
   <funding-group>
    <funding-statement xml:lang="ru">The work was financially supported by the Ministry of Science and Higher Education in terms of maintaining the EKB and MAGW radars and by RSF in terms of research (grant No. 24-22-00436) [https://rscf.ru/project/24-22-00436/]</funding-statement>
    <funding-statement xml:lang="en">The work was financially supported by the Ministry of Science and Higher Education in terms of maintaining the EKB and MAGW radars and by RSF in terms of research (grant No. 24-22-00436) [https://rscf.ru/project/24-22-00436/]</funding-statement>
   </funding-group>
  </article-meta>
 </front>
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    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: https://pgia.ru/data/spaceweather/ (accessed December 12, 2025).</mixed-citation>
     <mixed-citation xml:lang="en">URL: https://pgia.ru/data/spaceweather/ (accessed December 12, 2025).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B28">
    <label>28.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">URL: https://ckp-rf.ru/catalog/ckp/3056/ (accessed December 12, 2025).</mixed-citation>
     <mixed-citation xml:lang="en">URL: https://ckp-rf.ru/catalog/ckp/3056/ (accessed December 12, 2025).</mixed-citation>
    </citation-alternatives>
   </ref>
  </ref-list>
 </back>
</article>
