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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-26-2449-2008</article-id>
<title-group>
<article-title>Momentum transfer at the high-latitude magnetopause and boundary layers</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Lund</surname>
<given-names>E. 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>Farrugia</surname>
<given-names>C. 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>Sandholt</surname>
<given-names>P. E.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Space Science Center, University of New Hampshire, Durham, New Hampshire, USA</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Department of Physics, University of Oslo, Oslo, Norway</addr-line>
</aff>
<pub-date pub-type="epub">
<day>13</day>
<month>08</month>
<year>2008</year>
</pub-date>
<volume>26</volume>
<issue>8</issue>
<fpage>2449</fpage>
<lpage>2458</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2008 E. J. Lund et al.</copyright-statement>
<copyright-year>2008</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>
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<self-uri xlink:href="https://angeo.copernicus.org/articles/26/2449/2008/angeo-26-2449-2008.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/26/2449/2008/angeo-26-2449-2008.pdf</self-uri>
<abstract>
<p>How and where momentum is transferred from the solar wind to the
magnetosphere and ionosphere is one of the key problems of space physics.
Much of this transfer occurs through direct reconnection on the dayside,
particularly when the IMF is southward. However, momentum transfer also
occurs at higher latitudes via Alfvén waves on old open field lines, even
for southward IMF. This momentum is transferred to the ionosphere via
field-aligned currents (FACs), and the flow channel associated with these
FACs produces a Hall current which causes magnetic variations at high
latitude (the Svalgaard-Mansurov effect). We show examples where such
momentum transfer is observed with multiple spacecraft and ground-based
instruments.</p>
</abstract>
<counts><page-count count="10"/></counts>
</article-meta>
</front>
<body/>
<back>
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