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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-27-3957-2009</article-id>
<title-group>
<article-title>Speed evolution of fast CME/shocks with SOHO/LASCO, WIND/WAVES, IPS and in-situ WIND data: analysis of  kilometric type-II emissions</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Gonzalez-Esparza</surname>
<given-names>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>Aguilar-Rodriguez</surname>
<given-names>E.</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 Geofisica, Universidad Nacional Autonoma de Mexico, Morelia Mich., Mexico</addr-line>
</aff>
<pub-date pub-type="epub">
<day>21</day>
<month>10</month>
<year>2009</year>
</pub-date>
<volume>27</volume>
<issue>10</issue>
<fpage>3957</fpage>
<lpage>3966</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2009 A. Gonzalez-Esparza</copyright-statement>
<copyright-year>2009</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>
<self-uri xlink:href="https://angeo.copernicus.org/articles/27/3957/2009/angeo-27-3957-2009.html">This article is available from https://angeo.copernicus.org/articles/27/3957/2009/angeo-27-3957-2009.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/27/3957/2009/angeo-27-3957-2009.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/27/3957/2009/angeo-27-3957-2009.pdf</self-uri>
<abstract>
<p>Fast CME/shocks propagating in the interplanetary medium can generate
kilometric Type II (km-TII) radio emissions at the local plasma
frequency and/or its harmonic, so these radio emissions provide a
means of remotely tracking CME/shocks. We apply a new analysis
technique, using the frequency drift of km-TII spectrum obtained by
the Thermal Noise Receiver (TNR) of the WIND/WAVES experiment, to
infer, at some adequate intervals, the propagation speed of six
CME/shocks. We combine these results with previously reported speeds
from coronagraph white light and interplanetary scintillation observations, and
in-situ measurements, to study the temporal speed evolution of the six
events. The speed values obtained by the km-TII analysis are in a
reasonable agreement with the speed measurements obtained by other
techniques at different heliocentric distance ranges. The combination
of all the speed measurements show a gradual deceleration of the
CME/shocks as they propagate to 1 AU. This new technique can be
useful in studying the evolution of fast CME/shocks when adequate
intervals of km-TII emissions are available.</p>
</abstract>
<counts><page-count count="10"/></counts>
</article-meta>
</front>
<body/>
<back>
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</article>