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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">53254</article-id>
   <article-id pub-id-type="doi">10.2205/2023ES000834</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. I. Mathematical preliminaries</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Linear perturbations of the Bloch type of space-periodic magnetohydrodynamic steady states. I. Mathematical preliminaries</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="2023-07-18T00:00:00+03:00">
    <day>18</day>
    <month>07</month>
    <year>2023</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2023-07-18T00:00:00+03:00">
    <day>18</day>
    <month>07</month>
    <year>2023</year>
   </pub-date>
   <volume>23</volume>
   <issue>3</issue>
   <fpage>1</fpage>
   <lpage>20</lpage>
   <history>
    <date date-type="received" iso-8601-date="2022-11-11T00:00:00+03:00">
     <day>11</day>
     <month>11</month>
     <year>2022</year>
    </date>
    <date date-type="accepted" iso-8601-date="2023-05-11T00:00:00+03:00">
     <day>11</day>
     <month>05</month>
     <year>2023</year>
    </date>
   </history>
   <self-uri xlink:href="https://rjes.ru/en/nauka/article/53254/view">https://rjes.ru/en/nauka/article/53254/view</self-uri>
   <abstract xml:lang="ru">
    <p>We consider Bloch eigenmodes in three linear stability problems: the kinematic dynamo problem, the hydrodynamic and MHD stability problem for steady space-periodic flows and MHD states. A Bloch mode is a product of a field of the same periodicity, as the state subjected to perturbation, and a planar harmonic wave, eiq·x. The complex exponential cancels out from the equations of the respective eigenvalue problem, and the wave vector q remains in the equations as a numeric parameter. The resultant problem has a significant advantage from the numerical viewpoint: while the Bloch mode involves two independent spatial scales, its growth rate can be computed in the periodicity box of the perturbed state. The three-dimensional space, where q resides, splits into a number of regions, inside which the growth rate is a smooth function of q. In preparation for a numerical study of the dominant (i.e., the largest over q) growth rates, we have derived expressions for the gradient of the growth rate in q and proven that, for parity-invariant flows and MHD steady states or when the respective eigenvalue of the stability operator is real, half-integer q (whose all components are integer or half-integer) are stationary points of the growth rate. In prior works it was established by asymptotic methods that high spatial scale separation (small q) gives rise to the phenomena of the α-effect or, for parity-invariant steady states, of the eddy diffusivity. We review these findings tailoring them to the prospective numerical applications.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>We consider Bloch eigenmodes in three linear stability problems: the kinematic dynamo problem, the hydrodynamic and MHD stability problem for steady space-periodic flows and MHD states. A Bloch mode is a product of a field of the same periodicity, as the state subjected to perturbation, and a planar harmonic wave, eiq·x. The complex exponential cancels out from the equations of the respective eigenvalue problem, and the wave vector q remains in the equations as a numeric parameter. The resultant problem has a significant advantage from the numerical viewpoint: while the Bloch mode involves two independent spatial scales, its growth rate can be computed in the periodicity box of the perturbed state. The three-dimensional space, where q resides, splits into a number of regions, inside which the growth rate is a smooth function of q. In preparation for a numerical study of the dominant (i.e., the largest over q) growth rates, we have derived expressions for the gradient of the growth rate in q and proven that, for parity-invariant flows and MHD steady states or when the respective eigenvalue of the stability operator is real, half-integer q (whose all components are integer or half-integer) are stationary points of the growth rate. In prior works it was established by asymptotic methods that high spatial scale separation (small q) gives rise to the phenomena of the α-effect or, for parity-invariant steady states, of the eddy diffusivity. We review these findings tailoring them to the prospective numerical applications.</p>
   </trans-abstract>
   <kwd-group xml:lang="en">
    <kwd>Kinematic dynamo problem</kwd>
    <kwd>hydrodynamic linear stability problem</kwd>
    <kwd>magnetohydrodynamic linear stability problem</kwd>
    <kwd>Bloch mode</kwd>
    <kwd>magnetic α-effect</kwd>
    <kwd>AKA-effect</kwd>
    <kwd>combined magnetohydrodynamic α-effect</kwd>
    <kwd>magnetic eddy diffusivity</kwd>
    <kwd>eddy viscosity</kwd>
    <kwd>scale separation.</kwd>
   </kwd-group>
   <funding-group>
    <funding-statement xml:lang="en">The project was financed by the grant №22-17-00114 of the Russian Science Foundation (https://rscf.ru/project/22-17-00114/).</funding-statement>
   </funding-group>
  </article-meta>
 </front>
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 </body>
 <back>
  <ref-list>
   <ref id="B1">
    <label>1.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Andrievsky, A., A. Brandenburg, A. Noullez, and V. Zheligovsky (2015), Negative magnetic eddy diffusivities from test-field method and multiscale stability theory, The Astrophysical Journal, 811(2), 135, DOI: 10.1088/0004-637x/811/2/135</mixed-citation>
     <mixed-citation xml:lang="en">Andrievsky, A., A. Brandenburg, A. Noullez, and V. Zheligovsky (2015), Negative magnetic eddy diffusivities from test-field method and multiscale stability theory, The Astrophysical Journal, 811(2), 135, DOI: 10.1088/0004-637x/811/2/135.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B2">
    <label>2.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Bloch, F. (1929), Über die Quantenmechanik der Elektronen in Kristallgittern, Zeitschrift für Physik A. Hadrons and Nuclei, 52, 555-600.</mixed-citation>
     <mixed-citation xml:lang="en">Bloch, F. (1929), Über die Quantenmechanik der Elektronen in Kristallgittern, Zeitschrift für Physik A. Hadrons and Nuclei, 52, 555-600.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B3">
    <label>3.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Braginskii, S. I. (1964a), Self-excitation of a magnetic field during the motion of a highly conducting fluid, Sov. Phys. JETP, 20, 726-735.</mixed-citation>
     <mixed-citation xml:lang="en">Braginskii, S. I. (1964a), Self-excitation of a magnetic field during the motion of a highly conducting fluid, Sov. Phys. JETP, 20, 726-735.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B4">
    <label>4.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Braginskii, S. I. (1964b), Theory of the hydromagnetic dynamo, Sov. Phys. JETP, 20, 1462- 1471.</mixed-citation>
     <mixed-citation xml:lang="en">Braginskii, S. I. (1964b), Theory of the hydromagnetic dynamo, Sov. Phys. JETP, 20, 1462- 1471.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B5">
    <label>5.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Braginskii, S. I. (1964c), Kinematic models of the Earth’s hydromagnetic dynamo, Geomagn. Aeron., 4, 572-583.</mixed-citation>
     <mixed-citation xml:lang="en">Braginskii, S. I. (1964c), Kinematic models of the Earth’s hydromagnetic dynamo, Geomagn. Aeron., 4, 572-583.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B6">
    <label>6.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Braginskii, S. I. (1964d), Magnetohydrodynamics of the Earth’s core, Geomagn. Aeron., 4, 698-711.</mixed-citation>
     <mixed-citation xml:lang="en">Braginskii, S. I. (1964d), Magnetohydrodynamics of the Earth’s core, Geomagn. Aeron., 4, 698-711.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B7">
    <label>7.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Braginskii, S. I. (1975), An almost axially symmetric model of the hydromagnetic dynamo of the Earth, I, Geomagn. Aeron., 15, 149-156.</mixed-citation>
     <mixed-citation xml:lang="en">Braginskii, S. I. (1975), An almost axially symmetric model of the hydromagnetic dynamo of the Earth, I, Geomagn. Aeron., 15, 149-156.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B8">
    <label>8.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Brandenburg, A., and K. Subramanian (2005), Astrophysical magnetic fields and nonlinear dynamo theory, Physics Reports, 417(1-4), 1-209, https://doi.org/10.1016/j.physrep.20 05.06.005.</mixed-citation>
     <mixed-citation xml:lang="en">Brandenburg, A., and K. Subramanian (2005), Astrophysical magnetic fields and nonlinear dynamo theory, Physics Reports, 417(1-4), 1-209, https://doi.org/10.1016/j.physrep.20 05.06.005.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B9">
    <label>9.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Brandenburg, A., D. Sokoloff, and K. Subramanian (2012), Current status of turbulent dynamo theory. From large-scale to small-scale dynamos, Space Science Reviews, 169(1-4), 123-157, https://doi.org/10.1007/s11214-012-9909-x.</mixed-citation>
     <mixed-citation xml:lang="en">Brandenburg, A., D. Sokoloff, and K. Subramanian (2012), Current status of turbulent dynamo theory. From large-scale to small-scale dynamos, Space Science Reviews, 169(1-4), 123-157, https://doi.org/10.1007/s11214-012-9909-x.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B10">
    <label>10.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Cameron, R. H., M. Dikpati, and A. Brandenburg (2016), The Global Solar Dynamo, Space Science Reviews, 210(1-4), 367-395, https://doi.org/10.1007/s11214-015-0230-3.</mixed-citation>
     <mixed-citation xml:lang="en">Cameron, R. H., M. Dikpati, and A. Brandenburg (2016), The Global Solar Dynamo, Space Science Reviews, 210(1-4), 367-395, https://doi.org/10.1007/s11214-015-0230-3.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B11">
    <label>11.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Charbonneau, P. (2005), Dynamo Models of the Solar Cycle, Living Rev. Solar Phys., 2, https://doi.org/10.12942/lrsp-2005-2.</mixed-citation>
     <mixed-citation xml:lang="en">Charbonneau, P. (2005), Dynamo Models of the Solar Cycle, Living Rev. Solar Phys., 2, https://doi.org/10.12942/lrsp-2005-2.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B12">
    <label>12.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Charbonneau, P. (2014), Solar Dynamo Theory, Annual Review of Astronomy and Astrophysics, 52(1), 251-290, DOI: 10.1146/annurev-astro-081913-040012</mixed-citation>
     <mixed-citation xml:lang="en">Charbonneau, P. (2014), Solar Dynamo Theory, Annual Review of Astronomy and Astrophysics, 52(1), 251-290, DOI: 10.1146/annurev-astro-081913-040012</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B13">
    <label>13.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Chertovskih, R., and V. Zheligovsky (2015), Large-scale weakly nonlinear perturbations of convective magnetic dynamos in a rotating layer, Physica D: Nonlinear Phenomena, 313, 99-116, https://doi.org/10.1016/j.physd.2015.09.012.</mixed-citation>
     <mixed-citation xml:lang="en">Chertovskih, R., and V. Zheligovsky (2015), Large-scale weakly nonlinear perturbations of convective magnetic dynamos in a rotating layer, Physica D: Nonlinear Phenomena, 313, 99-116, https://doi.org/10.1016/j.physd.2015.09.012.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B14">
    <label>14.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Dubrulle, B., and U. Frisch (1991), Eddy viscosity of parity-invariant flow, Physical Review A, 43(10), 5355-5364, https://doi.org/10.1103/physreva.43.5355.</mixed-citation>
     <mixed-citation xml:lang="en">Dubrulle, B., and U. Frisch (1991), Eddy viscosity of parity-invariant flow, Physical Review A, 43(10), 5355-5364, https://doi.org/10.1103/physreva.43.5355.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B15">
    <label>15.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Krause, F., and K.-H. Rädler (1980), Mean-Field Magnetohydrodynamics and Dynamo Theory, Elsevier, Berlin, https://doi.org/10.1016/c2013-0-03269-0.</mixed-citation>
     <mixed-citation xml:lang="en">Krause, F., and K.-H. Rädler (1980), Mean-Field Magnetohydrodynamics and Dynamo Theory, Elsevier, Berlin, https://doi.org/10.1016/c2013-0-03269-0.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B16">
    <label>16.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Lanotte, A., A. Noullez, M. Vergassola, and A. Wirth (1999), Large-scale dynamo by negative magnetic eddy diffusivities, Geophys. Astrophys. Fluid Dyn., 91, 131-146, https://doi.org/10.1080/03091929908203701.</mixed-citation>
     <mixed-citation xml:lang="en">Lanotte, A., A. Noullez, M. Vergassola, and A. Wirth (1999), Large-scale dynamo by negative magnetic eddy diffusivities, Geophys. Astrophys. Fluid Dyn., 91, 131-146, https://doi.org/10.1080/03091929908203701.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B17">
    <label>17.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Miesch, M. S. (2012), The Solar Dynamo, Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 370(1970), 3049-3069, https://doi.org/ 10.1098/rsta.2011.0507.</mixed-citation>
     <mixed-citation xml:lang="en">Miesch, M. S. (2012), The Solar Dynamo, Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 370(1970), 3049-3069, https://doi.org/ 10.1098/rsta.2011.0507.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B18">
    <label>18.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Moffatt, H. K. (1978), Magnetic field generation in electrically conducting fluids, Cambridge University Press.</mixed-citation>
     <mixed-citation xml:lang="en">Moffatt, H. K. (1978), Magnetic field generation in electrically conducting fluids, Cambridge University Press.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B19">
    <label>19.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Ossendrijver, M. A. J. H. (2000), Grand minima in a buoyancy-driven solar dynamo, Astron. Astrophys., 359, 364-372.</mixed-citation>
     <mixed-citation xml:lang="en">Ossendrijver, M. A. J. H. (2000), Grand minima in a buoyancy-driven solar dynamo, Astron. Astrophys., 359, 364-372.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B20">
    <label>20.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Parker, E. N. (1955), Hydrodynamic Dynamo Models, Astrophys J., 122, 293-314, https://doi.org/10.1086/146087.</mixed-citation>
     <mixed-citation xml:lang="en">Parker, E. N. (1955), Hydrodynamic Dynamo Models, Astrophys J., 122, 293-314, https://doi.org/10.1086/146087.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B21">
    <label>21.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Popova, H. P. (2016), Current results on the asymptotics of dynamo models, Physics-Uspekhi, 59(6), 513, https://doi.org/10.3367/UFNe.2016.02.037727.</mixed-citation>
     <mixed-citation xml:lang="en">Popova, H. P. (2016), Current results on the asymptotics of dynamo models, Physics-Uspekhi, 59(6), 513, https://doi.org/10.3367/UFNe.2016.02.037727.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B22">
    <label>22.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Press, W. H., S. A. Teukolsky, W. T. Vetterling, and B. P. Flannery (1992), Numerical recipes in Fortran. The art of scientific computing, 2nd ed., Cambridge University Press.</mixed-citation>
     <mixed-citation xml:lang="en">Press, W. H., S. A. Teukolsky, W. T. Vetterling, and B. P. Flannery (1992), Numerical recipes in Fortran. The art of scientific computing, 2nd ed., Cambridge University Press.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B23">
    <label>23.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Rädler, K.-H. (2007), Mean-Field Dynamo Theory: Early Ideas and Today’s Problems, in Magnetohydrodynamics: Historical Evolution and Trends, edited by S. S. Molokov, R. Moreau, and H. K. Moffatt, pp. 55-72, Springer Netherlands, Dordrecht, https://doi.org/10.1007/978-1-4020-4833-3_4.</mixed-citation>
     <mixed-citation xml:lang="en">Rädler, K.-H. (2007), Mean-Field Dynamo Theory: Early Ideas and Today’s Problems, in Magnetohydrodynamics: Historical Evolution and Trends, edited by S. S. Molokov, R. Moreau, and H. K. Moffatt, pp. 55-72, Springer Netherlands, Dordrecht, https://doi.org/10.1007/978-1-4020-4833-3_4.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B24">
    <label>24.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Rasskazov, A., R. Chertovskih, and V. Zheligovsky (2018), Magnetic field generation by pointwise zero-helicity three-dimensional steady flow of incompressible electrically conducting fluid, Phys. Rev. E, 97, 043210, https://doi.org/10.1103/PhysRevE.97.043201.</mixed-citation>
     <mixed-citation xml:lang="en">Rasskazov, A., R. Chertovskih, and V. Zheligovsky (2018), Magnetic field generation by pointwise zero-helicity three-dimensional steady flow of incompressible electrically conducting fluid, Phys. Rev. E, 97, 043210, https://doi.org/10.1103/PhysRevE.97.043201.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B25">
    <label>25.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Roberts, G. O. (1970), Spatially Periodic Dynamos, Phil. Trans. Roy. Soc. Lond. A, 266(1179), 535-558.</mixed-citation>
     <mixed-citation xml:lang="en">Roberts, G. O. (1970), Spatially Periodic Dynamos, Phil. Trans. Roy. Soc. Lond. A, 266(1179), 535-558.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B26">
    <label>26.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Roberts, G. O. (1972), Dynamo action of fluid motions with two-dimensional periodicity, Phil. Trans. Roy. Soc. Lond. A, 271, 411-454, https://doi.org/10.1098/rsta.1972.0015.</mixed-citation>
     <mixed-citation xml:lang="en">Roberts, G. O. (1972), Dynamo action of fluid motions with two-dimensional periodicity, Phil. Trans. Roy. Soc. Lond. A, 271, 411-454, https://doi.org/10.1098/rsta.1972.0015.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B27">
    <label>27.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Ruzmaikin, A. A., D. D. Sokolov, A. A. Soloviev, and A. M. Shukurov (1989), Couette- Poiseuille flow as a screw dynamo, Magnitnaya Gidrodinamika, 1(9), 6-11 (in Russian).</mixed-citation>
     <mixed-citation xml:lang="en">Ruzmaikin, A. A., D. D. Sokolov, A. A. Soloviev, and A. M. Shukurov (1989), Couette- Poiseuille flow as a screw dynamo, Magnitnaya Gidrodinamika, 1(9), 6-11 (in Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B28">
    <label>28.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Soloviev, A. A. (1985a), Magnetic dynamo existence for a dynamically possible motion of conducting fluid, Transactions (Doklady) of the Academy of Sciences of the USSR, (1), 44-48 (in Russian).</mixed-citation>
     <mixed-citation xml:lang="en">Soloviev, A. A. (1985a), Magnetic dynamo existence for a dynamically possible motion of conducting fluid, Transactions (Doklady) of the Academy of Sciences of the USSR, (1), 44-48 (in Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B29">
    <label>29.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Soloviev, A. A. (1985b), Magnetic field excitation by an axisymmetric motion of conducting fluid, Proc. of the Academy of Sciences of the USSR, Physics of the Earth, (4), 101-103 (in Russian).</mixed-citation>
     <mixed-citation xml:lang="en">Soloviev, A. A. (1985b), Magnetic field excitation by an axisymmetric motion of conducting fluid, Proc. of the Academy of Sciences of the USSR, Physics of the Earth, (4), 101-103 (in Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B30">
    <label>30.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Soloviev, A. A. (1985c), Description of the parameter region of the spiral couette-poiseuille flow of conducting fluid, for which magnetic field excitation is possible, Proc. of the Academy of Sciences of the USSR, Physics of the Earth, (12), 40-47 (in Russian).</mixed-citation>
     <mixed-citation xml:lang="en">Soloviev, A. A. (1985c), Description of the parameter region of the spiral couette-poiseuille flow of conducting fluid, for which magnetic field excitation is possible, Proc. of the Academy of Sciences of the USSR, Physics of the Earth, (12), 40-47 (in Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B31">
    <label>31.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Soloviev, A. A. (1987), Magnetic field excitation by a motion of conducting fluid at high magnetic reynolds numbers, Proc. of the Academy of Sciences of the USSR, Physics of the Earth, 5(5), 77-80 (in Russian).</mixed-citation>
     <mixed-citation xml:lang="en">Soloviev, A. A. (1987), Magnetic field excitation by a motion of conducting fluid at high magnetic reynolds numbers, Proc. of the Academy of Sciences of the USSR, Physics of the Earth, 5(5), 77-80 (in Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B32">
    <label>32.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Steenbeck, M., F. Krause, and K.-H. Rädler (1971), A calculation of the mean electromotive force in an electrically conducting fluid in turbulent motion, under the influence of Coriolis forces, in The Turbulent Dynamo: A Translation of a Series of Papers by F. Krause, K.-H. Rädler, and M. Steenbeck, edited by P. H. Roberts and M. Stix, pp. 29-47, Tech. Note UCAR/NCAR/IA-60, Boulder, Colorado, https://doi.org/10.5065/D6DJ5CK7.</mixed-citation>
     <mixed-citation xml:lang="en">Steenbeck, M., F. Krause, and K.-H. Rädler (1971), A calculation of the mean electromotive force in an electrically conducting fluid in turbulent motion, under the influence of Coriolis forces, in The Turbulent Dynamo: A Translation of a Series of Papers by F. Krause, K.-H. Rädler, and M. Steenbeck, edited by P. H. Roberts and M. Stix, pp. 29-47, Tech. Note UCAR/NCAR/IA-60, Boulder, Colorado, https://doi.org/10.5065/D6DJ5CK7.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B33">
    <label>33.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Vishik, M. M. (1986), Periodic Dynamo, in Mathematical methods in seismology and geody- namics, Computational seismology, vol. 19, edited by V. I. Keilis-Borok and A. L. Levshin, pp. 186-215, Nauka, Moscow (in Russian).</mixed-citation>
     <mixed-citation xml:lang="en">Vishik, M. M. (1986), Periodic Dynamo, in Mathematical methods in seismology and geody- namics, Computational seismology, vol. 19, edited by V. I. Keilis-Borok and A. L. Levshin, pp. 186-215, Nauka, Moscow (in Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B34">
    <label>34.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Vishik, M. M. (1987), Periodic Dynamo II, in Numerical modelling and analysis of geophysical processes, Computational seismology, vol. 20, edited by V. I. Keilis-Borok and A. L. Levshin, pp. 12-22, Nauka, Moscow (in Russian).</mixed-citation>
     <mixed-citation xml:lang="en">Vishik, M. M. (1987), Periodic Dynamo II, in Numerical modelling and analysis of geophysical processes, Computational seismology, vol. 20, edited by V. I. Keilis-Borok and A. L. Levshin, pp. 12-22, Nauka, Moscow (in Russian).</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B35">
    <label>35.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Zheligovsky, V. (1991), α-effect in generation of magnetic field by a flow of conducting fluid with internal scale in an axisymmetric volume, Geophys. Astrophys. Fluid Dynamics, 59, 235-251, https://doi.org/10.1080/03091929108227781.</mixed-citation>
     <mixed-citation xml:lang="en">Zheligovsky, V. (1991), α-effect in generation of magnetic field by a flow of conducting fluid with internal scale in an axisymmetric volume, Geophys. Astrophys. Fluid Dynamics, 59, 235-251, https://doi.org/10.1080/03091929108227781.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B36">
    <label>36.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Zheligovsky, V. (2011), Large-scale perturbations of magnetohydrodynamic regimes: linear and weakly nonlinear stability theory, Lecture Notes in Physics, 829, https://doi.org/10.1 007/978-3-642-18170-2.</mixed-citation>
     <mixed-citation xml:lang="en">Zheligovsky, V. (2011), Large-scale perturbations of magnetohydrodynamic regimes: linear and weakly nonlinear stability theory, Lecture Notes in Physics, 829, https://doi.org/10.1 007/978-3-642-18170-2.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B37">
    <label>37.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Zheligovsky, V. A. (2003), On the Linear Stability of Spatially Periodic Steady Magnetohy- drodynamic Systems with Respect to Long-Period Perturbations, Izvestiya, Physics of the Solid Earth, 39(5), 409-418.</mixed-citation>
     <mixed-citation xml:lang="en">Zheligovsky, V. A. (2003), On the Linear Stability of Spatially Periodic Steady Magnetohy- drodynamic Systems with Respect to Long-Period Perturbations, Izvestiya, Physics of the Solid Earth, 39(5), 409-418.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B38">
    <label>38.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Zheligovsky, V. A., and R. A. Chertovskih (2020), On Kinematic Generation of the Magnetic Modes of Bloch Type, Izvestiya, Physics of the Solid Earth, 56(1), 103-116, https://doi.org/ 10.1134/s1069351320010152.</mixed-citation>
     <mixed-citation xml:lang="en">Zheligovsky, V. A., and R. A. Chertovskih (2020), On Kinematic Generation of the Magnetic Modes of Bloch Type, Izvestiya, Physics of the Solid Earth, 56(1), 103-116, https://doi.org/ 10.1134/s1069351320010152.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B39">
    <label>39.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Zheligovsky, V. A., O. M. Podvigina, and U. Frisch (2001), Dynamo effect in parity-invariant flow with large and moderate separation of scales, Geophysical &amp; Astrophysical Fluid Dynamics, 95(3-4), 227-268, https://doi.org/10.1080/03091920108203726.</mixed-citation>
     <mixed-citation xml:lang="en">Zheligovsky, V. A., O. M. Podvigina, and U. Frisch (2001), Dynamo effect in parity-invariant flow with large and moderate separation of scales, Geophysical &amp; Astrophysical Fluid Dynamics, 95(3-4), 227-268, https://doi.org/10.1080/03091920108203726.</mixed-citation>
    </citation-alternatives>
   </ref>
  </ref-list>
 </back>
</article>
