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 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">Russian Journal of Earth Sciences</journal-id>
   <journal-title-group>
    <journal-title xml:lang="en">Russian Journal of Earth Sciences</journal-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Russian Journal of Earth Sciences</trans-title>
    </trans-title-group>
   </journal-title-group>
   <issn publication-format="online">1681-1208</issn>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="publisher-id">56812</article-id>
   <article-id pub-id-type="doi">10.2205/2023ES000841</article-id>
   <article-categories>
    <subj-group subj-group-type="toc-heading" xml:lang="ru">
     <subject>ОРИГИНАЛЬНЫЕ СТАТЬИ</subject>
    </subj-group>
    <subj-group subj-group-type="toc-heading" xml:lang="en">
     <subject>ORIGINAL ARTICLES</subject>
    </subj-group>
    <subj-group>
     <subject>ОРИГИНАЛЬНЫЕ СТАТЬИ</subject>
    </subj-group>
   </article-categories>
   <title-group>
    <article-title xml:lang="en">Linear perturbations of the Bloch type of space-periodic magnetohydrodynamic steady states. III. Asymptotics of branching</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Linear perturbations of the Bloch type of space-periodic magnetohydrodynamic steady states. III. Asymptotics of branching</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/0000-0002-5179-4344</contrib-id>
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Чертовских</surname>
       <given-names>Роман Александрович</given-names>
      </name>
      <name xml:lang="en">
       <surname>Chertovskih</surname>
       <given-names>R A</given-names>
      </name>
     </name-alternatives>
     <email>cadabr@rambler.ru</email>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Желиговский</surname>
       <given-names>Владислав Александрович</given-names>
      </name>
      <name xml:lang="en">
       <surname>Zheligovsky</surname>
       <given-names>V A</given-names>
      </name>
     </name-alternatives>
     <email>vlad@mitp.ru</email>
     <bio xml:lang="ru">
      <p>доктор физико-математических наук;</p>
     </bio>
     <bio xml:lang="en">
      <p>doctor of physical and mathematical sciences;</p>
     </bio>
     <xref ref-type="aff" rid="aff-2"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Институт теории прогноза землетрясений и математической геофизики Российской академии наук</institution>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Earthquake Prediction Theory and Mathematical Geophysics Russian academy of sciences</institution>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-2">
    <aff>
     <institution xml:lang="ru">Институт теории прогноза землетрясений и математической геофизики Российской академии наук</institution>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Earthquake Prediction Theory and Mathematical Geophysics Russian academy of sciences</institution>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <pub-date publication-format="print" date-type="pub" iso-8601-date="2023-12-15T00:00:00+03:00">
    <day>15</day>
    <month>12</month>
    <year>2023</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2023-12-15T00:00:00+03:00">
    <day>15</day>
    <month>12</month>
    <year>2023</year>
   </pub-date>
   <volume>23</volume>
   <issue>5</issue>
   <fpage>1</fpage>
   <lpage>16</lpage>
   <history>
    <date date-type="received" iso-8601-date="2022-11-22T00:00:00+03:00">
     <day>22</day>
     <month>11</month>
     <year>2022</year>
    </date>
    <date date-type="accepted" iso-8601-date="2023-03-07T00:00:00+03:00">
     <day>07</day>
     <month>03</month>
     <year>2023</year>
    </date>
   </history>
   <self-uri xlink:href="https://rjes.ru/en/nauka/article/56812/view">https://rjes.ru/en/nauka/article/56812/view</self-uri>
   <abstract xml:lang="ru">
    <p>The previous paper of this series presented the results of a numerical investigation of the dependence of the dominant growth rates of Bloch eigenmodes on the diffusivity parameters (the molecular viscosity ν and molecular magnetic diffusivity η) in three linear stability problems: the kinematic dynamo problem, and the hydrodynamic and MHD stability problems for steady spaceperiodic flows and MHD states. The dominant eigenmodes (i.e., the stability modes, whose growth rates are maximum over the wave vector q of the planar wave involved in the Bloch modes) comprise branches. In some branches, the dominant growth rates are attained for constant half-integer q. In all the three stability problems for parity-invariant steady states, offshoot branches, stemming from the branches of this type, were found, in which the dominant growth rates are attained for q depending on ν and/or η. We consider now such a branching of the dominant magnetic modes in the kinematic dynamo problem, where an offshoot stems from a branch of neutral eigenmodes for q = 0, and construct power series expansions for the offshoots and the associated eigenvalues of the magnetic induction operator near the point of bifurcation. We show that the branching occurs for the molecular magnetic diffusivities, for which the two eigenvalues of the eddy diffusivity operator become imaginary, and magnetic field generation by the mechanism of the negative eddy diffusivity ceases. The details of branching in the other linear stability problems under consideration are distinct.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>The previous paper of this series presented the results of a numerical investigation of the dependence of the dominant growth rates of Bloch eigenmodes on the diffusivity parameters (the molecular viscosity ν and molecular magnetic diffusivity η) in three linear stability problems: the kinematic dynamo problem, and the hydrodynamic and MHD stability problems for steady spaceperiodic flows and MHD states. The dominant eigenmodes (i.e., the stability modes, whose growth rates are maximum over the wave vector q of the planar wave involved in the Bloch modes) comprise branches. In some branches, the dominant growth rates are attained for constant half-integer q. In all the three stability problems for parity-invariant steady states, offshoot branches, stemming from the branches of this type, were found, in which the dominant growth rates are attained for q depending on ν and/or η. We consider now such a branching of the dominant magnetic modes in the kinematic dynamo problem, where an offshoot stems from a branch of neutral eigenmodes for q = 0, and construct power series expansions for the offshoots and the associated eigenvalues of the magnetic induction operator near the point of bifurcation. We show that the branching occurs for the molecular magnetic diffusivities, for which the two eigenvalues of the eddy diffusivity operator become imaginary, and magnetic field generation by the mechanism of the negative eddy diffusivity ceases. The details of branching in the other linear stability problems under consideration are distinct.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>Power series expansion</kwd>
    <kwd>asymptotics</kwd>
    <kwd>kinematic dynamo problem</kwd>
    <kwd>Bloch magnetic mode</kwd>
    <kwd>branching</kwd>
    <kwd>neutral eigenmodes</kwd>
    <kwd>magnetic eddy diffusivity</kwd>
    <kwd>scale separation.</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>Power series expansion</kwd>
    <kwd>asymptotics</kwd>
    <kwd>kinematic dynamo problem</kwd>
    <kwd>Bloch magnetic mode</kwd>
    <kwd>branching</kwd>
    <kwd>neutral eigenmodes</kwd>
    <kwd>magnetic eddy diffusivity</kwd>
    <kwd>scale separation.</kwd>
   </kwd-group>
   <funding-group>
    <funding-statement xml:lang="ru">The project was financed by the grant No. 22-17-00114 of the Russian Science Foundation, https://rscf.ru/project/22-17-00114/.</funding-statement>
    <funding-statement xml:lang="en">The project was financed by the grant No. 22-17-00114 of the Russian Science Foundation, https://rscf.ru/project/22-17-00114/.</funding-statement>
   </funding-group>
  </article-meta>
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</article>
