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<front>
<journal-meta>
<journal-id journal-id-type="publisher">NPG</journal-id>
<journal-title-group>
<journal-title>Nonlinear Processes in Geophysics</journal-title>
<abbrev-journal-title abbrev-type="publisher">NPG</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Nonlin. Processes Geophys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1607-7946</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/npg-11-241-2004</article-id>
<title-group>
<article-title>Generation of zonal flows by Rossby waves in the atmosphere</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Onishchenko</surname>
<given-names>O. G.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Pokhotelov</surname>
<given-names>O. A.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sagdeev</surname>
<given-names>R. Z.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Shukla</surname>
<given-names>P. K.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Stenflo</surname>
<given-names>L.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Institute of Physics of the Earth, 12 3810 Moscow, 10 B. Gruzinskaya Str., Russia</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Department of Physics, University of Maryland, College Park, Maryland 20 740, USA</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Institut für Theoretische Physik IV, Fakultät für Physik und Astronomie, Ruhr-Univ. Bochum, D-44780 Bochum, Germany</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Department of Plasma Physics, Umeå University S-90 187 Umeå, Sweden</addr-line>
</aff>
<pub-date pub-type="epub">
<day>14</day>
<month>04</month>
<year>2004</year>
</pub-date>
<volume>11</volume>
<issue>2</issue>
<fpage>241</fpage>
<lpage>244</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2004 O. G. Onishchenko et al.</copyright-statement>
<copyright-year>2004</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Generic License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by-nc-sa/2.5/">https://creativecommons.org/licenses/by-nc-sa/2.5/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://npg.copernicus.org/articles/11/241/2004/npg-11-241-2004.html">This article is available from https://npg.copernicus.org/articles/11/241/2004/npg-11-241-2004.html</self-uri>
<self-uri xlink:href="https://npg.copernicus.org/articles/11/241/2004/npg-11-241-2004.pdf">The full text article is available as a PDF file from https://npg.copernicus.org/articles/11/241/2004/npg-11-241-2004.pdf</self-uri>
<abstract>
<p>A novel mechanism for the short-scale Rossby waves
interacting with long-scale zonal flows in the Earth&apos;s atmosphere is
studied. The model is based on the parametric excitation of convective cells
by finite amplitude Rossby waves. We use a set of coupled equations
describing the nonlinear interaction of Rossby waves and zonal flows which
admits the excitation of zonal flows. The generation of such flows is due to
the Reynolds stresses of the finite amplitude Rossby waves. It is found that
the wave vector of the fastest growing mode is perpendicular to that of the
pump Rossby wave. We calculate the maximum instability growth rate and
deduce the optimal spatial dimensions of the zonal flows as well as their
azimuthal propagation speed. A comparison with previous results is made. The
present theory can be used for the interpretation of existing observations
of Rossby type waves in the Earth&apos;s atmosphere.</p>
</abstract>
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