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<front>
<journal-meta>
<journal-id journal-id-type="publisher">NPG</journal-id>
<journal-title-group>
<journal-title>Nonlinear Processes in Geophysics</journal-title>
<abbrev-journal-title abbrev-type="publisher">NPG</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Nonlin. Processes Geophys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1607-7946</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/npg-10-27-2003</article-id>
<title-group>
<article-title>Magnetic field turbulence, electron heating, magnetic holes, proton cyclotron waves, and the onsets of bipolar pulse (electron hole) events: a possible unifying scenario</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Tsurutani</surname>
<given-names>B. T.</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>Dasgupta</surname>
<given-names>B.</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>Arballo</surname>
<given-names>J. 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>Lakhina</surname>
<given-names>G. S.</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>Pickett</surname>
<given-names>J. S.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Indian Institute of Geomagnetism, Mumbai/Bombay 400 005, India</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Department of Physics and Astronomy, University of Iowa, Iowa City, IA, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>30</day>
<month>04</month>
<year>2003</year>
</pub-date>
<volume>10</volume>
<issue>1/2</issue>
<fpage>27</fpage>
<lpage>35</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2003 B. T. Tsurutani et al.</copyright-statement>
<copyright-year>2003</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Generic License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by-nc-sa/2.5/">https://creativecommons.org/licenses/by-nc-sa/2.5/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://npg.copernicus.org/articles/10/27/2003/npg-10-27-2003.html">This article is available from https://npg.copernicus.org/articles/10/27/2003/npg-10-27-2003.html</self-uri>
<self-uri xlink:href="https://npg.copernicus.org/articles/10/27/2003/npg-10-27-2003.pdf">The full text article is available as a PDF file from https://npg.copernicus.org/articles/10/27/2003/npg-10-27-2003.pdf</self-uri>
<abstract>
<p>Two electron heating
      events have been identified on 20 May 1996 when Polar was in the polar
      cap/polar cusp boundary layer. The electron heating events were located
      within magnetic holes/cavities/bubbles and were accompanied by nonlinear
      ± 14 nT peak-to-peak (f ~ 0.6 to 0.7 f&lt;sub&gt;cp&lt;/sub&gt;) obliquely
      propagating proton cyclotron waves. The electrons appear to be heated
      isotropically. Electric bipolar pulse (electron hole) onset events were
      also detected within the heating events. We propose a scenario which can
      link the above phenomena. Nonlinear Alfvén waves, generated through cusp
      magnetic reconnection, propagate down magnetic field lines and locally
      heat electrons through the ponderomotive force. The magnetic cavity is
      created through the diamagnetic effect of the heated electrons. Ion
      heating also occurs through ponderomotive acceleration (but much less than
      the electrons) and the protons generate the electromagnetic proton
      cyclotron waves through the loss cone instability. The obliquely
      propagating electromagnetic proton cyclotron waves accelerate bi-streaming
      electrons, which are the source of free energy for the electron holes.</p>
</abstract>
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</article-meta>
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