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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-24-2333-2006</article-id>
<title-group>
<article-title>Probing of medium-scale traveling ionospheric disturbances using HF-induced  scatter targets</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Blagoveshchenskaya</surname>
<given-names>N. F.</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>Borisova</surname>
<given-names>T. D.</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>Kornienko</surname>
<given-names>V. 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>Moskvin</surname>
<given-names>I. V.</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>Rietveld</surname>
<given-names>M. T.</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>Frolov</surname>
<given-names>V. L.</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>Uryadov</surname>
<given-names>V. P.</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>Kagan</surname>
<given-names>L. M.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Yampolski</surname>
<given-names>Yu. M.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Galushko</surname>
<given-names>V. L.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Koloskov</surname>
<given-names>A. V.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kasheev</surname>
<given-names>S. B.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Zalizovski</surname>
<given-names>A. V.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Vertogradov</surname>
<given-names>G. G.</given-names>
</name>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Vertogradov</surname>
<given-names>V. G.</given-names>
</name>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kelley</surname>
<given-names>M. C.</given-names>
</name>
<xref ref-type="aff" rid="aff7">
<sup>7</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Arctic and Antarctic Research Institute, St. Petersburg, Russia</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>EISCAT Scientific Association, Ramfjordbotn, Norway</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Radiophysical Research Institute, Nizhny Novgorod, Russia</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>University of Western Ontario, London, ON, Canada</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Institute of Radio Astronomy NAS, Kharkov, Ukraine</addr-line>
</aff>
<aff id="aff6">
<label>6</label>
<addr-line>Rostov-on-Don State University, Rostov-on-Don, Russia</addr-line>
</aff>
<aff id="aff7">
<label>7</label>
<addr-line>Cornell University, Ithaca NY, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>20</day>
<month>09</month>
<year>2006</year>
</pub-date>
<volume>24</volume>
<issue>9</issue>
<fpage>2333</fpage>
<lpage>2345</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2006 N. F. Blagoveshchenskaya et al.</copyright-statement>
<copyright-year>2006</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/24/2333/2006/angeo-24-2333-2006.html">This article is available from https://angeo.copernicus.org/articles/24/2333/2006/angeo-24-2333-2006.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/24/2333/2006/angeo-24-2333-2006.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/24/2333/2006/angeo-24-2333-2006.pdf</self-uri>
<abstract>
<p>Experimental results from the Tromsø and Sura heating
experiments at high and mid-latitudes are examined. It is shown that the
combination of HF-induced target and bi-static HF Doppler radio scatter
observations is a profitable method for probing medium-scale traveling
ionospheric disturbances (TIDs) at high and mid-latitudes. HF ionospheric
modification experiments provide a way of producing the HF-induced scatter
target in a controlled manner at altitudes where the sensitivity to TIDs is
highest. Bi-static HF Doppler radio scatter observations were carried out on
the London-Tromsø-St. Petersburg path in the course of a Tromsø
heating experiment on 16 November 2004 when the pump wave was reflected from
an auroral Es-layer. During Sura heating experiments on 19 and 20 August 2004,
when the HF pump wave was reflected from the F2 ionospheric layer,
multi-position bi-static HF Doppler radio scatter observations were
simultaneously performed at three reception points including St. Petersburg,
Kharkov, and Rostov-on-Don. Ray tracing and Doppler shift simulations were
made for all experiments. A computational technique has been developed
allowing the reconstruction of the TID phase velocities from multi-position
bi-static HF Doppler scatters. Parameters of medium-scale TIDs were found.
In all experiments they were observed in the evening and pre-midnight hours.
TIDs in the auroral E-region with periods of about 23 min were traveling
southward at speeds of 210 m/s. TIDs in the mid-latitudinal F-region with
periods from 20 to 45 min travelled at speeds between 40 and 150 m/s. During
quiet magnetic conditions the waves were traveling in the north-east
direction. In disturbed conditions the waves were moving in the south-west
direction with higher speeds as compared with quiet conditions. Possible
sources for the atmospheric gravity waves at middle and high latitudes are
discussed.</p>
</abstract>
<counts><page-count count="13"/></counts>
</article-meta>
</front>
<body/>
<back>
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</article>