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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-31-1297-2013</article-id>
<title-group>
<article-title>Cross-field flow and electric potential in a plasma slab</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>De Keyser</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>Echim</surname>
<given-names>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>Roth</surname>
<given-names>M.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Belgian Institute for Space Aeronomy (BIRA-IASB), Ringlaan 3, 1180 Brussels, Belgium</addr-line>
</aff>
<pub-date pub-type="epub">
<day>01</day>
<month>08</month>
<year>2013</year>
</pub-date>
<volume>31</volume>
<issue>8</issue>
<fpage>1297</fpage>
<lpage>1314</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2013 J. De Keyser et al.</copyright-statement>
<copyright-year>2013</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/31/1297/2013/angeo-31-1297-2013.html">This article is available from https://angeo.copernicus.org/articles/31/1297/2013/angeo-31-1297-2013.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/31/1297/2013/angeo-31-1297-2013.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/31/1297/2013/angeo-31-1297-2013.pdf</self-uri>
<abstract>
<p>We consider cross-field plasma flow inside a field-aligned plasma slab
embedded in a uniform background in a 1-dimensional geometry. This
situation may arise, for instance, when long-lasting reconnection pulses
inject plasma into the inner magnetosphere. The present paper presents a
detailed analysis of the structure of the interfaces that separate the slab
from the background plasma on either side; a fully kinetic model is used to
do so. Since the velocity shear across both interfaces has opposite signs,
and given the typical gyroradius differences between injected and background
ions and electrons, the structure of both interfaces can be very different.
The behaviour of the slab and its interfaces depends critically on the flow
of the plasma transverse to the magnetic field; in particular, it is shown
that there are bounds to the flow speed that can be supported by the
magnetised plasma. Further complicating the picture is the effect of the
potential difference between the slab and its environment.</p>
</abstract>
<counts><page-count count="18"/></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">Angelopoulos, V., Baumjohann, W., Kennel, C. F., Coroniti, F. V., Kivelson, M. G., Pellat, R., Walker, R. J., Lühr, H., and Paschmann, G.: Bursty bulk flows in the inner central plasma sheet, J. Geophys. Res., 97, 4027–4039, 1992.</mixed-citation>
</ref>
<ref id="ref2">
<label>2</label><mixed-citation publication-type="other" xlink:type="simple">Apatenkov, S. V., Sergeev, V. A., Kubyshkina, M. V., Nakamura, R., Baumjohann, W., Runov, A., Alexeev, I., Fazakerley, A., Frey, H., Muhlbachler, S., Daly, P. W., Sauvaud, J.-A., Ganushkina, N., Pulkkinen, T., Reeves, G. D., and Khotyaintsev, Y.: Multi-spacecraft observation of plasma dipolarization/injection in the inner magnetosphere, Ann. Geophys., 25, 801–814, &lt;a href=&quot;http://dx.doi.org/10.5194/angeo-25-801-2007&quot;&gt;https://doi.org/10.5194/angeo-25-801-2007&lt;/a&gt;, 2007..</mixed-citation>
</ref>
<ref id="ref3">
<label>3</label><mixed-citation publication-type="other" xlink:type="simple">Artemyev, A. V.: A model of one-dimensional current sheet with parallel currents and normal component of magnetic field, Phys. Plasmas, 18, 022104, &lt;a href=&quot;http://dx.doi.org/10.1063/1.3552141&quot;&gt;https://doi.org/10.1063/1.3552141&lt;/a&gt;, 2011.</mixed-citation>
</ref>
<ref id="ref4">
<label>4</label><mixed-citation publication-type="other" xlink:type="simple">Burch, J. L., Goldstein, J., Hill, T. W., Young, D. T., Crary, F. J., Coates, A. J., André, N., Kurth, W. S., and Sittler Jr., E. C.: Properties of local plasma injections in Saturn&apos;s magnetosphere, Geophys. Res. Lett., 32, L14S02, &lt;a href=&quot;http://dx.doi.org/10.1029/2005GL022611&quot;&gt;https://doi.org/10.1029/2005GL022611&lt;/a&gt;, 2005.</mixed-citation>
</ref>
<ref id="ref5">
<label>5</label><mixed-citation publication-type="other" xlink:type="simple">De Keyser, J. and Echim, M.: Electric potential differences across auroral generator interfaces, Ann. Geophys., 31, 251–261, &lt;a href=&quot;http://dx.doi.org/10.5194/angeo-31-251-2013&quot;&gt;https://doi.org/10.5194/angeo-31-251-2013&lt;/a&gt;, 2013.</mixed-citation>
</ref>
<ref id="ref6">
<label>6</label><mixed-citation publication-type="other" xlink:type="simple">De Keyser, J., Roth, M., Lemaire, J., Tsurutani, B., Ho, C., and Hammond, C.: Theoretical plasma distributions consistent with Ulysses magnetic field observations in a high-speed solar wind tangential discontinuity, Solar Phys., 166, 415–422, 1996.</mixed-citation>
</ref>
<ref id="ref7">
<label>7</label><mixed-citation publication-type="other" xlink:type="simple">De Keyser, J., Roth, M., Tsurutani, B., Ho, C., and Phillips, J.: Solar wind velocity jumps across tangential discontinuities: Ulysses observations and kinetic interpretation, A&amp;A, 321, 945–959, 1997.</mixed-citation>
</ref>
<ref id="ref8">
<label>8</label><mixed-citation publication-type="other" xlink:type="simple">De Keyser, J., Maggiolo, R., and Echim, M.: Monopolar and bipolar auroral electric fields and their effects, Ann. Geophys., 28, 2027–2046, &lt;a href=&quot;http://dx.doi.org/10.5194/angeo-28-2027-2010&quot;&gt;https://doi.org/10.5194/angeo-28-2027-2010&lt;/a&gt;, 2010.</mixed-citation>
</ref>
<ref id="ref9">
<label>9</label><mixed-citation publication-type="other" xlink:type="simple">Deng, X. H., Tang, R. X., Nakamura, R., Baumjohann, W., Zhang, T. L., Daly, P. W., Rème, H., Carr, C. M., Balogh, A., Liu, Z. X., and Wang, J. F.: Observation of reconnection pulses by Cluster and Double Star, Ann. Geophys., 23, 2921–2927, &lt;a href=&quot;http://dx.doi.org/10.5194/angeo-23-2921-2005&quot;&gt;https://doi.org/10.5194/angeo-23-2921-2005&lt;/a&gt;, 2005.</mixed-citation>
</ref>
<ref id="ref10">
<label>10</label><mixed-citation publication-type="other" xlink:type="simple">Echim, M. and Lemaire, J. F.: Laboratory and numerical simulations of the impulsive penetration mechanism, Space Sci. Rev., 92, 565–601, 2000.</mixed-citation>
</ref>
<ref id="ref11">
<label>11</label><mixed-citation publication-type="other" xlink:type="simple">Echim, M., Lemaire, J. F., and Roth, M.: Self-consistent solution for a collisionless plasma slab in motion across a magnetic field, Phys. Plasmas, 12, 072904, &lt;a href=&quot;http://dx.doi.org/10.1063/1.1943848&quot;&gt;https://doi.org/10.1063/1.1943848&lt;/a&gt;, 2005.</mixed-citation>
</ref>
<ref id="ref12">
<label>12</label><mixed-citation publication-type="other" xlink:type="simple">Echim, M. M., Maggiolo, R., Roth, M., and De Keyser, J.: A magnetospheric generator driving ion and electron acceleration and electric currents in a discrete auroral arc observed by Cluster and DMSP, Geophys. Res. Lett., 36, L12111, &lt;a href=&quot;http://dx.doi.org/10.1029/2009GL038343&quot;&gt;https://doi.org/10.1029/2009GL038343&lt;/a&gt;, 2009.</mixed-citation>
</ref>
<ref id="ref13">
<label>13</label><mixed-citation publication-type="other" xlink:type="simple">Echim, M., Maggiolo, R., De Keyser, J., Zhang, T. L., Voitcu, G., Barabash, S., and Lundin, R.: Comparative investigation of the Terrestrial and Venusian magnetopause: kinetic modeling and experimental observations by Cluster and Venus Express, Planet. Space Sci., 59, 1028–1038, &lt;a href=&quot;http://dx.doi.org/10.1016/j.pss.2010.04.019&quot;&gt;https://doi.org/10.1016/j.pss.2010.04.019&lt;/a&gt;, 2011.</mixed-citation>
</ref>
<ref id="ref14">
<label>14</label><mixed-citation publication-type="other" xlink:type="simple">Harris, E. G.: On a plasma sheath separating regions of oppositely directed magnetic field, Il Nuovo Cimento, 23, 115–121, 1962.</mixed-citation>
</ref>
<ref id="ref15">
<label>15</label><mixed-citation publication-type="other" xlink:type="simple">Hubert, D., Harvey, C., Roth, M., and De Keyser, J.: Electron density at the subsolar magnetopause for high magnetic shear: ISEE 1 and 2 observations, J. Geophys. Res., 103, 6685–6692, 1998.</mixed-citation>
</ref>
<ref id="ref16">
<label>16</label><mixed-citation publication-type="other" xlink:type="simple">Lee, L. C. and Kan, J. R.: A unified kinetic model of the tangential magnetopause structure, J. Geophys. Res., 84, 6417–6426, &lt;a href=&quot;http://dx.doi.org/10.1029/JA084iA11p06417&quot;&gt;https://doi.org/10.1029/JA084iA11p06417&lt;/a&gt;, 1979.</mixed-citation>
</ref>
<ref id="ref17">
<label>17</label><mixed-citation publication-type="other" xlink:type="simple">Lemaire, J.: Impulsive penetration of filamentary plasma elements into the magnetospheres of the Earth and Jupiter, Planet Space Sci., 25, 887–890, 1977.</mixed-citation>
</ref>
<ref id="ref18">
<label>18</label><mixed-citation publication-type="other" xlink:type="simple">Lemaire, J. and Roth, M.: Penetration of solar wind plasma elements into the magnetosphere, J. Atmos. Terr. Phys., 40, 331–335, 1978.</mixed-citation>
</ref>
<ref id="ref19">
<label>19</label><mixed-citation publication-type="other" xlink:type="simple">Lundin, R., Sauvaud, J.-A., Rème, H., Balogh, A., Dandouras, I., Bosqued, J. M., Carlson, C., Parks, G. K., Möbius, E., Kistler, L. M., Klecker, B., Amata, E., Formisano, V., Dunlop, M., Eliasson, L., Korth, A., Lavraud, B., and McCarthy, M.: Evidence for impulsive solar wind plasma penetration through the dayside magnetopause, Ann. Geophys., 21, 457–472, &lt;a href=&quot;http://dx.doi.org/10.5194/angeo-21-457-2003&quot;&gt;https://doi.org/10.5194/angeo-21-457-2003&lt;/a&gt;, 200.</mixed-citation>
</ref>
<ref id="ref20">
<label>20</label><mixed-citation publication-type="other" xlink:type="simple">Lyons, L. R.: Generation of large-scale regions of auroral currents, electric potentials and precipitation by the divergence of the convection electric field, J. Geophys. Res., 85, 17–24, 1980.</mixed-citation>
</ref>
<ref id="ref21">
<label>21</label><mixed-citation publication-type="other" xlink:type="simple">Maggiolo, R., Sauvaud, J. A., Fontaine, D., Teste, A., Grigorenko, E., Balogh, A., Fazakerley, A., Paschmann, G., Delcourt, D., and Rème, H.: A multi-satellite study of accelerated ionospheric ion beams above the polar cap, Ann. Geophys., 24, 1665–1684, &lt;a href=&quot;http://dx.doi.org/10.5194/angeo-24-1665-2006&quot;&gt;https://doi.org/10.5194/angeo-24-1665-2006&lt;/a&gt;, 2006.</mixed-citation>
</ref>
<ref id="ref22">
<label>22</label><mixed-citation publication-type="other" xlink:type="simple">Maggiolo, R., Echim, M., De Keyser, J., Fontaine, D., Jacquey, C., and Dandouras, I.: Polar cap ion beams during periods of northward IMF: Cluster statistical results, Ann. Geophys., 29, 771–787, &lt;a href=&quot;http://dx.doi.org/10.5194/angeo-29-771-2011&quot;&gt;https://doi.org/10.5194/angeo-29-771-2011&lt;/a&gt;, 2011.</mixed-citation>
</ref>
<ref id="ref23">
<label>23</label><mixed-citation publication-type="other" xlink:type="simple">Maggiolo, R., Echim, M., Simon Wedlund, C., Zhang, Y., Fontaine, D., Lointier, G., and Trotignon, J.-G.: Polar cap arcs from the magnetosphere to the ionosphere: kinetic modelling and observations by Cluster and TIMED, Ann. Geophys., 30, 283–302, &lt;a href=&quot;http://dx.doi.org/10.5194/angeo-30-283-2012&quot;&gt;https://doi.org/10.5194/angeo-30-283-2012&lt;/a&gt;, 2012.</mixed-citation>
</ref>
<ref id="ref24">
<label>24</label><mixed-citation publication-type="other" xlink:type="simple">Marchaudon, A., Cerisier, J.-C., Dunlop, M. W., Pitout, F., Bosqued, J.-M., and Fazakerley, A. N.: Shape, size, velocity and field-aligned currents of dayside plasma injections: a multi-altitude study, Ann. Geophys., 27, 1251–1266, &lt;a href=&quot;http://dx.doi.org/10.5194/angeo-27-1251-2009&quot;&gt;https://doi.org/10.5194/angeo-27-1251-2009&lt;/a&gt;, 2009.</mixed-citation>
</ref>
<ref id="ref25">
<label>25</label><mixed-citation publication-type="other" xlink:type="simple">Mitchell, D. G., Carbary, J. F., Cowley, S. W. H., Hill, T. W., and Zarka, P.: The Dynamics of Saturn&apos;s Magnetosphere, in: Saturn from Cassini-Huygens, edited by: Dougherty, M. K., pp. 257–279, Springer, &lt;a href=&quot;http://dx.doi.org/10.1007/978-1-4020-9217-6_10&quot;&gt;https://doi.org/10.1007/978-1-4020-9217-6_10&lt;/a&gt;, 2009.</mixed-citation>
</ref>
<ref id="ref26">
<label>26</label><mixed-citation publication-type="other" xlink:type="simple">Mottez, F.: Exact nonlinear analytic Vlasov–Maxwell tangential equilibria with arbitrary density and temperature profiles, Phys. Plasmas, 10, 2501–2508, 2003.</mixed-citation>
</ref>
<ref id="ref27">
<label>27</label><mixed-citation publication-type="other" xlink:type="simple">Nicholson, R. B.: Solution of the Vlasov Equations for a Plasma in an Externally Uniform Magnetic Field, Phys. Fluids, 6, 1581–1586, 1963.</mixed-citation>
</ref>
<ref id="ref28">
<label>28</label><mixed-citation publication-type="other" xlink:type="simple">Reasoner, D. L., Craven, P. D., and Chappell, C. R.: Characteristics of low-energy plasma in the plasmasphere and plasma trough, J. Geophys. Res., 88, 7913–7925, &lt;a href=&quot;http://dx.doi.org/10.1029/JA088iA10p07913&quot;&gt;https://doi.org/10.1029/JA088iA10p07913&lt;/a&gt;, 1983.</mixed-citation>
</ref>
<ref id="ref29">
<label>29</label><mixed-citation publication-type="other" xlink:type="simple">Roth, M., De Keyser, J., and Kuznetsova, M. M.: Vlasov theory of the equilibrium structure of tangential discontinuities in space plasmas, Space Sci. Rev., 76, 251–317, 1996.</mixed-citation>
</ref>
<ref id="ref30">
<label>30</label><mixed-citation publication-type="other" xlink:type="simple">Sestero, A.: Structure of plasma sheaths, Phys. Fluids, 7, 44–51, 1964.</mixed-citation>
</ref>
<ref id="ref31">
<label>31</label><mixed-citation publication-type="other" xlink:type="simple">Sestero, A.: Vlasov equation study of plasma motion across magnetic fields, Phys. Fluids, 9, 2006–2013, 1966.</mixed-citation>
</ref>
<ref id="ref32">
<label>32</label><mixed-citation publication-type="other" xlink:type="simple">Sojka, J. J., Schunk, R. W., Johnson, J. F. E., Waite, J. H., and Chappell, C. R.: Characteristics of thermal and suprathermal ions associated with the dayside plasma trough as measured by the Dynamics Explorer Retarding Ion Mass Spectrometer, J. Geophys. Res., 88, 7895–7911, &lt;a href=&quot;http://dx.doi.org/10.1029/JA088iA10p07895&quot;&gt;https://doi.org/10.1029/JA088iA10p07895&lt;/a&gt;, 1983.</mixed-citation>
</ref>
<ref id="ref33">
<label>33</label><mixed-citation publication-type="other" xlink:type="simple">Whipple, E. C., Hill, J. R., and Nichols, J. D.: Magnetopause structure and the question of particle accessibility, J. Geophys. Res., 89, 1508–1516, &lt;a href=&quot;http://dx.doi.org/10.1029/JA089iA03p01508&quot;&gt;https://doi.org/10.1029/JA089iA03p01508&lt;/a&gt;, 1984.</mixed-citation>
</ref>
<ref id="ref34">
<label>34</label><mixed-citation publication-type="other" xlink:type="simple">Zhang, J.-C., Wolf, R. A., Sazykin, S., and Toffoletto, F. R.: Injection of a bubble into the inner magnetosphere, Geophys. Res. Lett., 35, L02110,, &lt;a href=&quot;http://dx.doi.org/10.1029/2007GL032048&quot;&gt;https://doi.org/10.1029/2007GL032048&lt;/a&gt;, 2008.</mixed-citation>
</ref>
</ref-list>
</back>
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