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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-19-655-2001</article-id>
<title-group>
<article-title>Disturbance of plasma environment in the vicinity of the Astrid-2 microsatellite</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ivchenko</surname>
<given-names>N.</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>Facciolo</surname>
<given-names>L.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Lindqvist</surname>
<given-names>P. 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>Kekkonen</surname>
<given-names>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>Holback</surname>
<given-names>B.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Alfv&amp;#x00E9;n Laboratory, Royal Institute of Technology, Stockholm, Sweden</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Politecnico di Torino, C. so Duca degli Abruzzi, Torino, Italy</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Oulu University, Oulu, Finland</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Swedish Institute of Space Physics, Uppsala, Sweden</addr-line>
</aff>
<pub-date pub-type="epub">
<day>30</day>
<month>06</month>
<year>2001</year>
</pub-date>
<volume>19</volume>
<issue>6</issue>
<fpage>655</fpage>
<lpage>666</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2001 N. Ivchenko et al.</copyright-statement>
<copyright-year>2001</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/19/655/2001/angeo-19-655-2001.html">This article is available from https://angeo.copernicus.org/articles/19/655/2001/angeo-19-655-2001.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/19/655/2001/angeo-19-655-2001.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/19/655/2001/angeo-19-655-2001.pdf</self-uri>
<abstract>
<p>The presence of a
 satellite disturbs the ambient plasma. The charging of the spacecraft creates a
 sheath around it, and the motion of the satellite creates a wake disturbance.
 This modification of the plasma environment introduces difficulties in
 measuring electric fields and plasma densities using the probe technique. We
 present a study of the structure of the sheath and wake around the Astrid-2
 microsatellite, as observed by the probes of the EMMA and LINDA instruments.
 Measurements with biased LINDA probes, as well as current sweeps on the EMMA
 probes, show a density enhancement upstream of the satellite and a plasma
 depletion behind the satellite. The electric field probes detect disturbances
 in the plasma potential on magnetic field lines connected to the satellite.&lt;br&gt;&lt;br&gt;&lt;b&gt;Key words. &lt;/b&gt;Space plasma physics
 (spacecraft sheaths, wakes, charging; instruments and techniques)</p>
</abstract>
<counts><page-count count="12"/></counts>
</article-meta>
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