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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ANGEO</journal-id>
<journal-title-group>
<journal-title>Annales Geophysicae</journal-title>
<abbrev-journal-title abbrev-type="publisher">ANGEO</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Ann. Geophys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1432-0576</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/angeo-32-57-2014</article-id>
<title-group>
<article-title>Investigation of convectively generated gravity wave characteristics and generation mechanisms during the passage of thunderstorm and squall line over Gadanki (13.5° N, 79.2° E)</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Arunachalam Srinivasan</surname>
<given-names>M.</given-names>
<ext-link>https://orcid.org/0000-0003-0991-7985</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>Rao</surname>
<given-names>S. V. B.</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>Suresh</surname>
<given-names>R.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Department of Physics, Sri Venkateswara University, Tirupati-517 502, India</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>India Meteorological Department, Chennai-600 001, India</addr-line>
</aff>
<pub-date pub-type="epub">
<day>30</day>
<month>01</month>
<year>2014</year>
</pub-date>
<volume>32</volume>
<issue>1</issue>
<fpage>57</fpage>
<lpage>68</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2014 M. Arunachalam Srinivasan et al.</copyright-statement>
<copyright-year>2014</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions>
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<self-uri xlink:href="https://angeo.copernicus.org/articles/32/57/2014/angeo-32-57-2014.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/32/57/2014/angeo-32-57-2014.pdf</self-uri>
<abstract>
<p>This study illustrates the convectively generated gravity wave generation
mechanisms during the passage of thunderstorms and squall line using Indian
MST radar. For the first time, it has been shown that all three generation
mechanisms have been involved in the generation of gravity waves during the
passage of squall line event. It is observed that the periodicities in the
range of 8–80 min in the tropospheric and 8–32 min in the lower
stratospheric regions and vertical wavelengths in the range of 3.2–4.8 km
in the tropospheric and 1.2–1.92 km in the lower stratospheric regions are
found to be dominant in the present study and are distinctly different during
initial, mature and dissipative phases of convection. Amplitude of vertical
wind has been weakened (from ~ 4–6 m s&lt;sup&gt;−1&lt;/sup&gt; to
~ 1 m s&lt;sup&gt;−1&lt;/sup&gt;) considerably after 10–30 min of a convection event.
It appears that the wind shear associated with the convective clouds acted
like an obstacle to the mean background flow during the squall line passage
generated gravity waves. The phase profiles corresponding to the dominant
period show both downward and upward propagation of waves. The vertical
extent of heating is found to be deeper during squall line event compared
with thunderstorm event. From the phase profiles, during 27 September 2004,
two peaks of constant phase region are observed. One is due to convective
elements and the other is due to strong background wind shear; however, only
one peak is observed on 29 September 2004, which is only due to convective
processes.</p>
</abstract>
<counts><page-count count="12"/></counts>
</article-meta>
</front>
<body/>
<back>
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