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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-19-593-2001</article-id>
<title-group>
<article-title>The MEDUSA electron and ion spectrometer and the PIA ultraviolet photometers on Astrid-2</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Norberg</surname>
<given-names>O.</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>Winningham</surname>
<given-names>J. D.</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>Lauche</surname>
<given-names>H.</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>Keith</surname>
<given-names>W.</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>Puccio</surname>
<given-names>W.</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>Olsen</surname>
<given-names>J.</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>Lundin</surname>
<given-names>K.</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>Scherrer</surname>
<given-names>J.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Swedish Institute of Space Physics, Box 812, SE-981 28 Kiruna, Sweden</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Southwest Research Institute, P. O. Drawer 28510, San Antonio, Texas 78228-0510, USA</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Max-Plank-Institut für Aeronomie, Postfach 20, D-37189 Katlenburg-Lindau, Germany</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>593</fpage>
<lpage>600</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2001 O. Norberg 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/19/593/2001/angeo-19-593-2001.html">This article is available from https://angeo.copernicus.org/articles/19/593/2001/angeo-19-593-2001.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/19/593/2001/angeo-19-593-2001.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/19/593/2001/angeo-19-593-2001.pdf</self-uri>
<abstract>
<p>The miniature electron
 and ion spectrometer MEDUSA on Astrid-2 consists of two
 &quot;top-hat&quot;-type spherical electrostatic analyzers, sharing a common
 top-hat. Fast energy sweeps (16 electron sweeps and 8 ion sweeps per second)
 allow for very high temporal resolution measurements of a two-dimensional slice
 of the particle distribution function. The energy range covered, is in the case
 of electrons, 4 eV to 22 keV and, in the case of ions, 2 eV to 12 keV. MEDUSA
 is mounted with its aperture close to the spin plane of Astrid-2, which allows
 for good pitch-angle coverage when the local magnetic field is in the satellite
 spin plane. The PIA-1/2 spin-scanning ultraviolet photometers measure auroral
 emissions. Using the spacecraft spin and orbital motion, it is possible to
 create two-dimensional images from the data. Spin-scanning photometers, such as
 PIA, are low-cost, low mass alternatives to auroral imagers, but place
 constraints on the satellite attitude. Data from MEDUSA are used to study
 processes in the auroral region, in particular, electrodynamics of aurora and
 &quot;black aurora&quot;. MEDUSA is also a technological development, paving
 the way for highly capable, miniaturized particle spectrometers.&lt;br&gt;&lt;br&gt;&lt;b&gt;Key words. &lt;/b&gt;Ionosphere (instruments
 and techniques) – Magnetospheric physics (auroral phenomena; instruments and
 techniques)</p>
</abstract>
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