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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-27-4305-2009</article-id>
<title-group>
<article-title>The Earth&apos;s magnetopause as a source and sink for equatorial nightside energetic charged particles</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Klida</surname>
<given-names>M. M.</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>Fritz</surname>
<given-names>T. A.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Center for Space Physics, Boston University, Boston, MA 02215, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>26</day>
<month>11</month>
<year>2009</year>
</pub-date>
<volume>27</volume>
<issue>11</issue>
<fpage>4305</fpage>
<lpage>4316</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2009 M. M. Klida</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>
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<abstract>
<p>The Imaging Proton Spectrometer (IPS) and the Imaging Electron Spectrometer
(IES) on the Polar satellite have measured temporary deviations in the
isotropy of the pitch angle distributions (PADs) of charged particles in the
inner magnetosphere. As Polar passes through the nightside equatorial region,
the IPS and IES observe dropouts of charged particles with pitch angles near
90&amp;deg;, known as butterfly distributions caused by the shadowing of the
magnetopause. Additionally, Polar observes a lower energy (&amp;lt;60 keV) intensification of locally mirroring ions while simultaneously
detecting butterfly PADs in both higher energy ions and electrons. While it
is accepted that charged particles can be lost to the magnetopause due to
shadowing effects, the modeling here can suggest that the magnetopause can
also be a direct source for particles observed in magnetosphere, with a
strong dependence upon both pitch angle and particle energy.</p>
</abstract>
<counts><page-count count="12"/></counts>
</article-meta>
</front>
<body/>
<back>
<ref-list>
<title>References</title>
<ref id="ref1">
<label>1</label><mixed-citation publication-type="other" xlink:type="simple"> Ashour-Abdalla, M., Bosqued, J M., El-Alaoui, M., Peroomian, V., Zelenyi, L M., Walker, R J., and Wright, J.: A stochastic sea: The source of plasma sheet boundary layer ion structures observed by Cluster, J. Geophys. Res. (Space Physics), 110, 12221–12238, \doi10.1029/2005JA011183, 2005. </mixed-citation>
</ref>
<ref id="ref2">
<label>2</label><mixed-citation publication-type="other" xlink:type="simple"> Blake, J B., Fennell, J F., Friesen, L M., Johnson, B M., Kolasinski, W A., Mabry, D J., Osborn, J V., Penzin, S H., Schnauss, E R., Spence, H E., Baker, D N., Belian, R., Fritz, T A., Ford, W., Laubscher, B., Stiglich, R., Baraze, R A., Hilsenrath, M F., Imhof, W L., Kilner, J R., Mobilia, J., Voss, D H., Korth, A., Gull, M., Fisher, K., Grande, M., and Hall, D.: Ceppad, Space Sci. Rev., 71, 531–562, 1995. </mixed-citation>
</ref>
<ref id="ref3">
<label>3</label><mixed-citation publication-type="other" xlink:type="simple"> Bogott, F H. and Mozer, F S.: Equitorial electron angular distributions in the loss cone and at large angles, J. Geophys. Res., 76, 6790–6805, 1971. </mixed-citation>
</ref>
<ref id="ref4">
<label>4</label><mixed-citation publication-type="other" xlink:type="simple"> Fritz, T A., Alothman, M., Bhattacharjya, J., Matthews, D L., and Chen, J.: Butterfly pitch-angle distributions observed by ISEE-1, Planet. Space Sci., 51, 205–219, 2003. </mixed-citation>
</ref>
<ref id="ref5">
<label>5</label><mixed-citation publication-type="other" xlink:type="simple"> Kaye, S M., Lin, C S., Parks, G K., and Winckler, J R.: Adiabatic modulation of equatorial pitch angle anisotropy, J. Geophys. Res., 83, 2675–2682, 1978.  </mixed-citation>
</ref>
<ref id="ref6">
<label>6</label><mixed-citation publication-type="other" xlink:type="simple"> Pfitzer, K A., Lezniak, T W., and Winckler, J R.: Experimental verification of drift shell splitting in the distorted magnetosphere, J. Geophys. Res., 74, 4687–4693, 1969. </mixed-citation>
</ref>
<ref id="ref7">
<label>7</label><mixed-citation publication-type="other" xlink:type="simple"> Richard, R L., El-Alaoui, M., Ashour-Abdalla, M., and Walker, R J.: Modeling the entry and trapping of solar energetic particles in the magnetosphere during the November 24–25, 2001 storm, J. Geophys. Res. (Space Physics), 114, 4210–4225, \doi10.1029/2007JA012823, 2009. </mixed-citation>
</ref>
<ref id="ref8">
<label>8</label><mixed-citation publication-type="other" xlink:type="simple"> Roederer, J G.: On the adiabatic motion of energetic particles in a model magnetosphere, J. Geophys. Res., 72, 981–992, 1967. </mixed-citation>
</ref>
<ref id="ref9">
<label>9</label><mixed-citation publication-type="other" xlink:type="simple"> Roederer, J G.: Dynamics of Geomagnetically Trapped Radiation, no 2 in Physics and Chemistry in Space, Springer-Verlag, Berlin, 1970. </mixed-citation>
</ref>
<ref id="ref10">
<label>10</label><mixed-citation publication-type="other" xlink:type="simple"> Russell, C T., Snare, R C., Means, J D., Pierce, D., Dearborn, D., Larson, M., Barr, G., and Le, G.: The GGS/Polar Magnetic Fields Investigation, Space Sci. Rev., 71, 563–582, 1995. </mixed-citation>
</ref>
<ref id="ref11">
<label>11</label><mixed-citation publication-type="other" xlink:type="simple"> Serlemitsos, P.: Low-energy electrons in the dark magnetosphere, J. Geophys. Res., 71, 61–77, 1966. </mixed-citation>
</ref>
<ref id="ref12">
<label>12</label><mixed-citation publication-type="other" xlink:type="simple"> Stern, D P.: Charged particle motions in a magnetic field that reduce to motions in a potential, Am. J. Phys., 43, 689–694, \doi10.1119/1.9714, 1975. </mixed-citation>
</ref>
<ref id="ref13">
<label>13</label><mixed-citation publication-type="other" xlink:type="simple"> Tsyganenko, N A.: Modeling the Earth&apos;s magnetospheric magnetic field confined within a realistic magnetopause, J. Geophys. Res., 100, 5599–5612, 1995. </mixed-citation>
</ref>
<ref id="ref14">
<label>14</label><mixed-citation publication-type="other" xlink:type="simple"> Tsyganenko, N A. and Sitnov, M I.: Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms, J. Geophys. Res., 110, 3208–3223, \doi10.1029/2004JA010798, 2005. </mixed-citation>
</ref>
<ref id="ref15">
<label>15</label><mixed-citation publication-type="other" xlink:type="simple"> Volland, H.: A model of the magnetospheric electric convection field, J. Geophys. Res., 83, 2695–2699, 1978. </mixed-citation>
</ref>
<ref id="ref16">
<label>16</label><mixed-citation publication-type="other" xlink:type="simple"> Walker, R J., Ashour-Abdalla, M., Ogino, T., Peroomian, V., and Richard, R L.: Modeling Magnetospheric Plasma Sources and Losses, AGU Spring Meeting Abstracts, 2001. </mixed-citation>
</ref>
<ref id="ref17">
<label>17</label><mixed-citation publication-type="other" xlink:type="simple"> West Jr., H I.: Some observations of the trapped electrons produced by the Russian high-altitude nuclear detonation of October 28, 1962, in: ASSL Vol. 5: Radiation Trapped in the Earth&apos;s Magnetic Field, edited by: McCormac, B M., pp. 634–662, 1966. </mixed-citation>
</ref>
<ref id="ref18">
<label>18</label><mixed-citation publication-type="other" xlink:type="simple"> West Jr., H I. and Buck, R M.: Pitch angle distributions of energetic electrons in the equatorial regions of the outer magnetosphere – OGO-5 observations, in: Magnetospheric physics: proceedings of the Advanced Summer Institute held at Sheffield, UK, August 1973, edited by: McCormac, B M., pp. 93–104, D. Reidel Publishing Co., Dordrecht, 1974. </mixed-citation>
</ref>
<ref id="ref19">
<label>19</label><mixed-citation publication-type="other" xlink:type="simple"> West Jr., H I., Buck, R M., and Walton, J R.: Electron pitch angle distributions of energetic electrons throughout the magnetosphere as observed on OGO 5, J. Geophys. Res., 78, 1064–1081, 1973. </mixed-citation>
</ref>
</ref-list>
</back>
</article>