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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-27-1233-2009</article-id>
<title-group>
<article-title>Asymmetries in the equatorial electrojet around N-E Brazil sector</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Rastogi</surname>
<given-names>R. G.</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>Trivedi</surname>
<given-names>N. B.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Physical Research Laboratory, Ahmedabad 380009, India</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Observatorio Magnetico, 89 Madruga, Vassouras, Brazil</addr-line>
</aff>
<pub-date pub-type="epub">
<day>12</day>
<month>03</month>
<year>2009</year>
</pub-date>
<volume>27</volume>
<issue>3</issue>
<fpage>1233</fpage>
<lpage>1249</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2009 R. G. Rastogi</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/27/1233/2009/angeo-27-1233-2009.html">This article is available from https://angeo.copernicus.org/articles/27/1233/2009/angeo-27-1233-2009.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/27/1233/2009/angeo-27-1233-2009.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/27/1233/2009/angeo-27-1233-2009.pdf</self-uri>
<abstract>
<p>The paper examines the data of geographic northward (X), eastward (Y) and
vertical (Z) components of the magnetic field from a dense array of 26
vector magnetometers operated in N-NE Brazil from November 1990 to March
1991. As expected, the daily variation of X showed a minor maximum around
03:00–04:00 LT and a major maximum around 12:00 LT. The daily range of
ΔY showed a strong minimum around noon at all stations. The combined
ΔY and ΔX indicated the direction of the equatorial
electrojet currents to be flowing along 25&amp;deg; north of east at the centre
and 20&amp;deg; north of east at the edges of the equatorial electrojet (EEJ)
belt. The centre of the EEJ as defined by the zero intercept of the Z versus
latitude was found to be near 1.0&amp;deg; S dip latitude. The electrojet
current was stronger in the northern half than in the southern half of the
electrojet belt. These anomalies are suggested to be due to the abnormal
distribution of the mean magnetic field in this region.</p>
</abstract>
<counts><page-count count="17"/></counts>
</article-meta>
</front>
<body/>
<back>
<ref-list>
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</back>
</article>