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<front>
<journal-meta>
<journal-id journal-id-type="publisher">WCDD</journal-id>
<journal-title-group>
<journal-title>Weather and Climate Dynamics Discussions</journal-title>
<abbrev-journal-title abbrev-type="publisher">WCDD</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Weather Clim. Dynam. Discuss.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">2698-4024</issn>
<publisher><publisher-name></publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/wcd-2021-21</article-id>
<title-group>
<article-title>Observed wavenumber-frequency spectrum of global, normal mode function decomposed, fields: a possible evidence for nonlinear effects on the wave dynamics</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Teruya</surname>
<given-names>André Seiji Wakate</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>Raphaldini</surname>
<given-names>Breno</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>Mayta</surname>
<given-names>Victor Chavez</given-names>
<ext-link>https://orcid.org/0000-0003-4037-1722</ext-link>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Raupp</surname>
<given-names>Carlos Frederico Mendonça</given-names>
<ext-link>https://orcid.org/0000-0001-7225-864X</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>da Silva Dias</surname>
<given-names>Pedro Leite</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Sao Paulo, Brazil</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Department of Mathematical Sciences, Durham University, Durham, UK</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Department of Climate and Space Science and Engineering, University of Michigan, Ann Arbor, Michigan, and Department of Atmospheric and Oceanic Sciences, University of Wisconsin-Madison, Madison, United States</addr-line>
</aff>
<pub-date pub-type="epub">
<day>30</day>
<month>04</month>
<year>2021</year>
</pub-date>
<volume>2021</volume>
<fpage>1</fpage>
<lpage>29</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2021 André Seiji Wakate Teruya et al.</copyright-statement>
<copyright-year>2021</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://wcd.copernicus.org/preprints/wcd-2021-21/">This article is available from https://wcd.copernicus.org/preprints/wcd-2021-21/</self-uri>
<self-uri xlink:href="https://wcd.copernicus.org/preprints/wcd-2021-21/wcd-2021-21.pdf">The full text article is available as a PDF file from https://wcd.copernicus.org/preprints/wcd-2021-21/wcd-2021-21.pdf</self-uri>
<abstract>
<p>&lt;p&gt;The study of tropical tropospheric disturbances has led to important challenges from both observational and theoretical points of view. In particular, the observed wavenumber-frequency spectrum of tropical oscillations, also known as Wheeler-Kiladis diagram, has helped bridging the gap between observations and the linear theory of equatorial waves. Here we have obtained a similar wavenumber-frequency spectrum for each equatorial wave type by performing a normal mode function (NMF) decomposition of global Era-Interim reanalysis data, with the NMF basis being given by the eigensolutions of the primitive equations in spherical coordinates, linearized around a resting background state. In this methodology, the global multi-level horizontal velocity and geopotential height fields are projected onto the normal mode functions characterized by a vertical mode, a zonal wavenumber, a meridional quantum index and a mode type, namely Rossby, Kelvin, mixed Rossby-gravity and westward and eastward propagating inertio-gravity modes. The horizontal velocity and geopotential height fields associated with each mode type are then reconstructed on the physical space, and the corresponding wavenumber-frequency spectrum is calculated for the 200&amp;thinsp;hPa zonal wind. The results reveal some expected structures, such as the dominant global-scale Rossby and Kelvin waves constituting the intraseasonal frequency associated with the Madden-Julian Oscillation. On the other hand, some unexpected features such as westward propagating Kelvin waves and eastward propagating westward inertio-gravity waves are also revealed by our observed 200&amp;thinsp;hPa zonal wind spectrum. These intriguing behaviours represent a large departure from the linear equatorial wave theory and can be a result of strong nonlinearities in the wave dynamics.&lt;/p&gt;</p>
</abstract>
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<funding-group>
<award-group id="gs1">
<funding-source>Fundação de Amparo à Pesquisa do Estado de São Paulo</funding-source>
<award-id>15/50122-0</award-id>
</award-group>
</funding-group>
</article-meta>
</front>
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