<?xml version="1.0" encoding="ISO-8859-1"?><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
<front>
<journal-meta>
<journal-id>1409-2433</journal-id>
<journal-title><![CDATA[Revista de Matemática Teoría y Aplicaciones]]></journal-title>
<abbrev-journal-title><![CDATA[Rev. Mat]]></abbrev-journal-title>
<issn>1409-2433</issn>
<publisher>
<publisher-name><![CDATA[Centro de Investigaciones en Matemática Pura y Aplicada (CIMPA) y Escuela de Matemática, San José, Costa Rica.]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S1409-24332013000100002</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Simulation of decametric wave propagation in the ionospheric plasma]]></article-title>
<article-title xml:lang="es"><![CDATA[Simulación de propagación decamétrica de ondas en el plasma ionosférico]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Kiryanova]]></surname>
<given-names><![CDATA[Kseniya S.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Kryukovsky]]></surname>
<given-names><![CDATA[Andrey S.]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Lukin]]></surname>
<given-names><![CDATA[Dmitriy S.]]></given-names>
</name>
<xref ref-type="aff" rid="A03"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Russian New University Postgraduate student ]]></institution>
<addr-line><![CDATA[ Moscow]]></addr-line>
<country>Russia</country>
</aff>
<aff id="A02">
<institution><![CDATA[,Russian New University Head Chair of Information Technologies and Natural Sciences ]]></institution>
<addr-line><![CDATA[ Moscow]]></addr-line>
<country>Russia</country>
</aff>
<aff id="A03">
<institution><![CDATA[,State University Moscow Physical and Technical Institute Head Chair of Physics and Mathematical Problems of Wave Processes]]></institution>
<addr-line><![CDATA[ Moscow]]></addr-line>
<country>Russia</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>01</month>
<year>2013</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>01</month>
<year>2013</year>
</pub-date>
<volume>20</volume>
<numero>1</numero>
<fpage>21</fpage>
<lpage>34</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.sa.cr/scielo.php?script=sci_arttext&amp;pid=S1409-24332013000100002&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.sa.cr/scielo.php?script=sci_abstract&amp;pid=S1409-24332013000100002&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.sa.cr/scielo.php?script=sci_pdf&amp;pid=S1409-24332013000100002&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[The decametric radiowaves propagation in the ionospheric plasma was considered. Bicharacteristic system of equations was used in the modeling ray structures. This system, which allows finding the ray paths with great precision, was obtained by D.S. Lukin. Models of the ionosphere with horizontal gradients were used in the calculations; local inhomogeneities, such as reduced electron density in the maximum layer and increased electron density below the maximum layer, were taken into account. The features of shortwave propagation, such as getting a wave of interlayer channel, distribution and out of it, reflection of waves from different ionospheric layers were explored. Was shown that the rays can be ejected from the field of distribution and curled when hit in the inhomogeneity of the ionosphere. The formation of caustic surfaces and its dynamics were studied. The radiowaves propagation in the Earth&#8217;s ionosphere was studied. This ionosphere profiles were restored the scientific group led by Professor V.E. Kunitsyn by radiotomography method based on real observations. Ray structures in the area of &#8220;equatorial anomaly&#8221; were built. The models, both including and excluding the effect of Earth&#8217;s magnetic field and the influence of the equatorial anomaly were considered. Ray structures at the different positions of the radiation source, as well as different operating frequency, were investigated. Dynamic model of the ray&#8217;s propagation was developed.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[Se considera la propagación de radioondas decamétricas en el plasma ionosférico. Se usa un sistema bicaracterístico de ecuaciones para modelar las estructuras radiales. Este sistema, que permite encontrar los caminos radiales con gran precisión, fueobtenido por D.S. Lukin. En los cálculos se usaron modelos de la ionosfera con gradientes horizontales; se tomaron en cuenta inhomogeneidades locales, tales como densidad reducida de electrones en la capa máxima y dendidad aumentada de electrones ba jo la capa máxima. Se exploraron características de la propagación de las ondas cortas. Se muestra que los rayos pueden ser expulsados del campo de distribución y hacer un bucle cuando chocan con la inhomogeneidad dela ionosfera. Se estudia la formación de superficies cáusticas y su dinámica. También se estudia la propagación de radioondas en la ionosfera de la Tierra. Los perfiles de esta ionosfera fueron dados al grupo liderado por el Profesor V.E. Kunitsyn por medio del método de radiotomografía basado en observaciones reales. Se construyeron estructuras de rayos en el área de &#8220;anomalía ecuatorial&#8221;. Se consideraron que incluyen y que excluyen el efecto del campo magnético de la Tierra y la influencia de la anomalía ecuatorial. Se investigaron estructuras radiales en diferentes posiciones de la fuenta de la radiación, así como diferentes frecuencias operativas. Se desarrolló el modelo dinámico de la propagación de los rayos.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Decameter radiowaves]]></kwd>
<kwd lng="en"><![CDATA[the bicharacteristic system]]></kwd>
<kwd lng="en"><![CDATA[ionospheric plasma]]></kwd>
<kwd lng="en"><![CDATA[the equatorial anomaly]]></kwd>
<kwd lng="en"><![CDATA[ray structures]]></kwd>
<kwd lng="es"><![CDATA[Radioondas decamétricas]]></kwd>
<kwd lng="es"><![CDATA[el sistema bicaracterístico]]></kwd>
<kwd lng="es"><![CDATA[plasma ionosférico]]></kwd>
<kwd lng="es"><![CDATA[anomalía ecuatorial]]></kwd>
<kwd lng="es"><![CDATA[estructuras radiales]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <div style="text-align: justify;">     <div style="text-align: center;"><font  style="font-family: verdana; font-weight: bold;" size="4">Simulation of decametric wave propagation in the ionospheric plasma</font><br style="font-weight: bold;"> <br style="font-weight: bold;"> <font style="font-family: verdana; font-weight: bold;" size="4">Simulaci&oacute;n de propagaci&oacute;n decam&eacute;trica de ondas en el plasma ionosf&eacute;rico</font>    <br> </div>     <br>     <div style="text-align: center;"><font style="font-family: verdana;"  size="2">Kseniya S. Kiryanova<sup><a href="#Afiliacion1">*</a><a name="Afiliacion4"></a>+</sup>, Andrey S. Kryukovsky<sup><a href="#Afiliacion2">&#8224;</a><a  name="Afiliacion5"></a>*</sup>, Dmitriy&nbsp; S. Lukin<sup><a href="#Afiliacion3">&#8225;</a><a name="Afiliacion6"></a>+</sup></font>    <br> </div>     <br> <font style="font-family: verdana;" size="2"></font><font  style="font-family: verdana;" size="-1"><a name="Correspondencia2"></a>*<a  href="#Correspondencia1">Direcci&oacute;n para correspondencia</a></font><br  style="font-weight: bold;"> <hr  style="width: 100%; height: 2px; margin-right: 0px; margin-left: 0px;"><font  style="font-family: verdana; font-weight: bold;" size="3">Abstract</font>    <br> <font style="font-family: verdana;" size="2"></font>    <br> <font style="font-family: verdana;" size="2">The decametric radiowaves propagation in the ionospheric plasma was considered.&nbsp; Bicharacteristic system of equations was used in the modeling&nbsp; ray structures.&nbsp; This&nbsp; system, which allows finding the ray paths with&nbsp; great precision,&nbsp; was obtained&nbsp; by D.S. Lukin.&nbsp;&nbsp; Models of the ionosphere&nbsp; with horizontal gradients were used&nbsp; in the calculations; local inhomogeneities, such as reduced&nbsp; electron density in the maximum&nbsp; layer and&nbsp; increased&nbsp; electron density below the maximum layer,&nbsp; were taken into account.&nbsp; The&nbsp; features of shortwave propagation,&nbsp; such as getting&nbsp; a wave of interlayer&nbsp; channel,&nbsp; distribution&nbsp; and out of it, reflection of waves from different ionospheric&nbsp; layers&nbsp; were explored.&nbsp; Was&nbsp; shown that the rays can be ejected from the field of distribution and&nbsp; curled&nbsp; when hit in the inhomogeneity of the ionosphere.&nbsp; The&nbsp; formation of caustic surfaces&nbsp; and&nbsp; its dynamics&nbsp; were studied.&nbsp; The&nbsp; radiowaves&nbsp; propagation in the Earth&#8217;s ionosphere was studied.&nbsp;&nbsp; This&nbsp; ionosphere&nbsp; profiles were restored&nbsp; the scientific&nbsp; group led by Professor V.E. Kunitsyn by radiotomography method based on real observations.&nbsp; Ray structures in the area of &#8220;equatorial anomaly&#8221; were built.&nbsp; The&nbsp; models,&nbsp; both including&nbsp; and&nbsp; excluding&nbsp; the effect of Earth&#8217;s magnetic field and&nbsp; the influence of the equatorial anomaly were considered.&nbsp; Ray structures at the different positions of the radiation source, as well as different operating frequency,&nbsp; were investigated.&nbsp; Dynamic&nbsp; model of the ray&#8217;s propagation was developed.</font>    <br> <font style="font-family: verdana;" size="2"></font>    ]]></body>
<body><![CDATA[<br> <font style="font-family: verdana;" size="2"><span  style="font-weight: bold;">Keywords:</span> Decameter radiowaves,&nbsp; the bicharacteristic system, ionospheric plasma, the equatorial anomaly,&nbsp; ray structures.</font>    <br> <font style="font-family: verdana;" size="2"></font>    <br> <font style="font-family: verdana; font-weight: bold;" size="3">Resumen</font>    <br> <font style="font-family: verdana;" size="2"></font>    <br> <font style="font-family: verdana;" size="2">Se considera&nbsp; la&nbsp; propagaci&oacute;n de&nbsp; radioondas&nbsp; decam&eacute;tricas en&nbsp; el plasma&nbsp; ionosf&eacute;rico. Se usa un sistema bicaracter&iacute;stico de ecuaciones para&nbsp; modelar&nbsp; las estructuras radiales.&nbsp; Este sistema, que permite encontrar los caminos radiales con gran precisi&oacute;n, fueobtenido por D.S. Lukin.&nbsp; En los c&aacute;lculos se usaron&nbsp; modelos de la ionosfera con gradientes horizontales; se tomaron en cuenta inhomogeneidades locales, tales como densidad&nbsp; reducida&nbsp; de electrones en la capa m&aacute;xima y dendidad&nbsp; aumentada de electrones ba jo la capa m&aacute;xima.&nbsp; Se exploraron caracter&iacute;sticas de la propagaci&oacute;n de las ondas cortas.&nbsp; Se muestra que los rayos&nbsp; pueden&nbsp; ser expulsados&nbsp; del campo&nbsp; de distribuci&oacute;n&nbsp; y hacer un&nbsp; bucle&nbsp; cuando&nbsp; chocan&nbsp; con la inhomogeneidad dela&nbsp; ionosfera.&nbsp;&nbsp; Se estudia la formaci&oacute;n de superficies c&aacute;usticas y su din&aacute;mica.&nbsp; Tambi&eacute;n se estudia la propagaci&oacute;n de radioondas en la ionosfera de la Tierra. Los perfiles de esta ionosfera fueron&nbsp; dados&nbsp; al grupo liderado&nbsp; por el Profesor&nbsp; V.E.&nbsp; Kunitsyn por&nbsp; medio&nbsp; del m&eacute;todo de radiotomograf&iacute;a basado en observaciones reales.&nbsp; Se construyeron estructuras de rayos en el &aacute;rea de &#8220;anomal&iacute;a ecuatorial&#8221;.&nbsp; Se consideraron&nbsp; que incluyen y que excluyen&nbsp; el efecto del campo&nbsp; magn&eacute;tico de la Tierra&nbsp; y la influencia de la anomal&iacute;a ecuatorial.&nbsp; Se investigaron estructuras radiales en diferentes posiciones de la fuenta de la radiaci&oacute;n, as&iacute; como diferentes frecuencias operativas. Se desarroll&oacute; el modelo din&aacute;mico de la propagaci&oacute;n de los rayos.</font>    <br> <font style="font-family: verdana;" size="2"></font><br  style="font-weight: bold;"> <font style="font-family: verdana;" size="2"><span  style="font-weight: bold;">Palabras clave:</span>&nbsp; Radioondas&nbsp; decam&eacute;tricas,&nbsp; el sistema bicaracter&iacute;stico, plasma ionosf&eacute;rico, anomal&iacute;a ecuatorial, estructuras radiales.    <br>     <br> <span style="font-weight: bold;">Mathematics Subject Classification:</span> 78A40.    <br> </font> <hr  style="width: 100%; height: 2px; margin-right: 0px; margin-left: 0px;"><font  style="font-family: verdana;" size="2">&nbsp;    <br> Ver contenido disponible en pdf    ]]></body>
<body><![CDATA[<br> </font><font style="font-family: verdana;" size="2"></font>    <br> <hr  style="width: 100%; height: 2px; margin-right: 0px; margin-left: 0px;"><font  style="font-family: verdana; font-weight: bold;" size="3">References</font>    <br> <font style="font-family: verdana;" size="2"></font>    <!-- ref --><br> <font style="font-family: verdana;" size="2">[1]&nbsp; Kryukovsky,&nbsp; A.S.; Lukin,&nbsp; D.S.; Rastyagaev,&nbsp; D.V. (2009) &#8220;Investigation of the features of propagation of short radiowaves in an inhomogeneous anisotropic ionosphere&#8221;,&nbsp; <span style="font-style: italic;">Electromagnetic Waves and Electronic&nbsp; Systems</span> <span style="font-weight: bold;">14</span>(8):&nbsp; 17&#8211;26.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1950959&pid=S1409-2433201300010000200001&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br> <font style="font-family: verdana;" size="2"></font>    <!-- ref --><br> <font style="font-family: verdana;" size="2">[2]&nbsp; Kryukovsky&nbsp; A.S.; Lukin,&nbsp; D.S.; Rastyagaev,&nbsp; D.V. (2010) &#8220;Simulation of ray and the caustic structure of electromagnetic fields according by ionospheric&nbsp; tomography&nbsp; in the vicinity&nbsp; of the equatorial&nbsp; anomaly&#8221;,&nbsp; <span style="font-style: italic;">Electromagnetic Waves and Electronic&nbsp; Systems</span> <span style="font-weight: bold;">15</span>(8):&nbsp; 5&#8211;11.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1950962&pid=S1409-2433201300010000200002&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br> <font style="font-family: verdana;" size="2"></font>    <!-- ref --><br> <font style="font-family: verdana;" size="2">[3]&nbsp; Andreeva,&nbsp;&nbsp; E.S.;&nbsp;&nbsp; Kryukovsky,&nbsp;&nbsp; A.S.;&nbsp; Kunitsyn,&nbsp; V.E.;&nbsp;&nbsp; Lukin,&nbsp;&nbsp; D.S.; Rastyagaev, D.V.; Kiryanova,&nbsp; K.S. (2011) &#8220;Simulation of ray and the caustic&nbsp; structure of electromagnetic&nbsp; fields according&nbsp; by&nbsp; ionospheric tomography&nbsp; in the vicinity of the equatorial anomaly&#8221;,&nbsp; in <span style="font-style: italic;">Propagation&nbsp; of Radiowaves</span>,&nbsp; Collection&nbsp; of Reports&nbsp; XXIII&nbsp; Russian&nbsp; Scientific Conference, Vol 3. (23-26 May 2011) Mari State Technical&nbsp; University, Yoshkar-Ola:&nbsp; 288&#8211;291.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1950965&pid=S1409-2433201300010000200003&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br> <font style="font-family: verdana;" size="2"></font>    <!-- ref --><br> <font style="font-family: verdana;" size="2">[4]&nbsp; Kryukovsky,&nbsp; A.S.; Kiryanova,&nbsp; K.S. (2011) &#8220;Dynamic&nbsp; modeling of radiowave propagation in the vicinity of the equatorial anomaly&nbsp; based on the method of bicharacteristics&#8221;, <span style="font-style: italic;">Electromagnetic Waves and Electronic Systems</span> <span style="font-weight: bold;">16</span>(8):&nbsp; 21&#8211;25.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1950968&pid=S1409-2433201300010000200004&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br> <font style="font-family: verdana;" size="2"></font>    <!-- ref --><br> <font style="font-family: verdana;" size="2">[5]&nbsp; Lukin,&nbsp; D.S.;&nbsp; Spiridonov,&nbsp; J.G. (1969)&nbsp; &#8220;Application of the method of characteristics&nbsp; for the numerical&nbsp; solution of radiowave&nbsp; propagation in inhomogeneous and nonlinear&nbsp; area&#8221;, <span  style="font-style: italic;">Radiotechnics and Electronics</span> <span style="font-weight: bold;">14</span>(9):&nbsp; 1673&#8211;1677.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1950971&pid=S1409-2433201300010000200005&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br> <font style="font-family: verdana;" size="2"></font>    <!-- ref --><br> <font style="font-family: verdana;" size="2">[6]&nbsp; Lukin,&nbsp; D.S.;&nbsp; Palkin,&nbsp;&nbsp; E.A.&nbsp; (1982)&nbsp; <span style="font-style: italic;">Numerical&nbsp;&nbsp; Canonical&nbsp;&nbsp; Method&nbsp; in Problems&nbsp; of Diffraction and&nbsp; Propagation of Electromagnetic&nbsp; Waves in&nbsp; Inhomogeneous&nbsp; Media</span>.&nbsp; Moscow Physical&nbsp; and Technical&nbsp; Institute, Moscow.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1950974&pid=S1409-2433201300010000200006&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    ]]></body>
<body><![CDATA[<br> <font style="font-family: verdana;" size="2"></font>    <!-- ref --><br> <font style="font-family: verdana;" size="2">[7]&nbsp; Kunitsyn, V.E.; Tereshchenko, E.D. (2003) <span style="font-style: italic;">Ionospheric&nbsp; Tomography</span>. </font><font style="font-family: verdana;" size="2">Springer.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1950977&pid=S1409-2433201300010000200007&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br> <font style="font-family: verdana;" size="2"></font>    <!-- ref --><br> <font style="font-family: verdana;" size="2">[8]&nbsp; Andreeva,&nbsp; E.S.;&nbsp; Franke,&nbsp;&nbsp; S.J.;&nbsp; Kunitsyn,&nbsp; V.E.;&nbsp; Yeh,&nbsp; K.C.&nbsp; (2000)&nbsp; &#8220; Some&nbsp; features of the equatorial anomaly&nbsp; revealed&nbsp; by ionospheric tomography&#8221;, <span style="font-style: italic;">Geophysical&nbsp; Research&nbsp; Letters</span>&nbsp; <span style="font-weight: bold;">27</span>(16)&nbsp; 2465&#8211;2468.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1950980&pid=S1409-2433201300010000200008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br> <font style="font-family: verdana;" size="2"></font>    <!-- ref --><br> <font style="font-family: verdana;" size="2">[9]&nbsp; Frankem&nbsp; S.J.; Yehm&nbsp; K.C.;&nbsp; Andreevam&nbsp; E.S.;&nbsp; Kunitsyn,&nbsp; V.E.&nbsp; (2003) &#8220;A&nbsp; study of the equatorial&nbsp; anomaly&nbsp; ionosphere&nbsp; using&nbsp; tomographic images&#8221;, <span style="font-style: italic;">Radio&nbsp; Science</span> <span  style="font-weight: bold;">38</span>(1):&nbsp; 1011&#8211;1020.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1950983&pid=S1409-2433201300010000200009&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br> <font style="font-family: verdana;" size="2"></font>    ]]></body>
<body><![CDATA[<!-- ref --><br> <font style="font-family: verdana;" size="2">[10]&nbsp; Kunitsyn, V.E.;&nbsp; Andreeva,&nbsp; E.S.; Franke,&nbsp; S.J.; Yeh, K.C. (2003) &#8220;Tomographic&nbsp; investigations&nbsp; of temporal&nbsp; variations&nbsp; of the ionospheric electron density and&nbsp; the implied&nbsp; fluxes&#8221;,&nbsp; <span  style="font-style: italic;">Geophysical&nbsp; Research&nbsp; Letters</span> <span style="font-weight: bold;">30</span>(16):&nbsp; 1851&#8211;1854.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1950986&pid=S1409-2433201300010000200010&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <br> <a name="Correspondencia1"></a><font style="font-family: verdana;"  size="-1"><a href="#Correspondencia2">*</a>Correspondencia a:</font>    <br> <font style="font-family: verdana;" size="2">Kseniya S. Kiryanova. </font><font  style="font-family: verdana;" size="2">Postgraduate&nbsp; student, Russian&nbsp; New University, 22, Radio&nbsp; Street,&nbsp; Moscow,&nbsp; 105005, Russia.&nbsp; E-Mail:&nbsp; 2661348@mail.ru</font>    <br> <font style="font-family: verdana;" size="2">Andrey S. Kryukovsky. </font><font  style="font-family: verdana;" size="2">Head&nbsp; Chair&nbsp; of Information&nbsp; Technologies&nbsp; and&nbsp; Natural&nbsp; Sciences,&nbsp; Russian&nbsp; New University, Moscow, Russia.&nbsp; E-Mail:&nbsp; kryukovsky@rambler.ru</font>    <br> <font style="font-family: verdana;" size="2">Dmitriy&nbsp; S. Lukin. </font><font  style="font-family: verdana;" size="2">Head&nbsp; Chair&nbsp;&nbsp; of Physics&nbsp;&nbsp; and&nbsp; Mathematical&nbsp; Problems of Wave&nbsp; Processes,&nbsp; Moscow Physical and&nbsp; Technical&nbsp;&nbsp; Institute (State University),&nbsp; 9,&nbsp; Institutskiy&nbsp; pereulok,&nbsp;&nbsp; Dolgo- prudniy,&nbsp; Moscow region, 141700, Russia.&nbsp; E-Mail:&nbsp; lukin@mail.mipt.ru</font>&nbsp;     <br> <font style="font-family: verdana;" size="2"><a name="Afiliacion1"></a><a  href="#Afiliacion4">*</a> Postgraduate&nbsp; student, Russian&nbsp; New University, 22, Radio&nbsp; Street,&nbsp; Moscow,&nbsp; 105005, Russia.&nbsp; E-Mail:&nbsp; 2661348@mail.ru</font>    <br> <font style="font-family: verdana;" size="2"><a name="Afiliacion2"></a><a  href="#Afiliacion5">&#8224;</a> Head&nbsp; Chair&nbsp; of Information&nbsp; Technologies&nbsp; and&nbsp; Natural&nbsp; Sciences,&nbsp; Russian&nbsp; New University, Moscow, Russia.&nbsp; E-Mail:&nbsp; kryukovsky@rambler.ru</font>    <br> <font style="font-family: verdana;" size="2"><a name="Afiliacion3"></a><a  href="#Afiliacion6">&#8225;</a> Head&nbsp; Chair&nbsp;&nbsp; of Physics&nbsp;&nbsp; and&nbsp; Mathematical&nbsp; Problems of Wave&nbsp; Processes,&nbsp; Moscow Physical and&nbsp; Technical&nbsp;&nbsp; Institute (State University),&nbsp; 9,&nbsp; Institutskiy&nbsp; pereulok,&nbsp;&nbsp; Dolgoprudniy,&nbsp; Moscow region, 141700, Russia.&nbsp; E-Mail:&nbsp; lukin@mail.mipt.ru</font>    ]]></body>
<body><![CDATA[<br> <hr  style="width: 100%; height: 2px; margin-right: 0px; margin-left: 0px;">     <div style="text-align: center;"><font style="font-family: verdana;"  size="2"><span style="font-weight: bold;">Received: 31/Dec/2011; Revised: 10/May/2012; Accepted: 27/Nov/2012</span></font></div> <font style="font-family: verdana;" size="2"></font></div>      ]]></body><back>
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