<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "https://jats.nlm.nih.gov/nlm-dtd/publishing/3.0/journalpublishing3.dtd">
<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" article-type="research-article" dtd-version="3.0" xml:lang="en">
<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-24-2543-2006</article-id>
<title-group>
<article-title>First ground-based optical analysis of H&lt;sub&gt;&amp;beta;&lt;/sub&gt; Doppler profiles close to local noon in the cusp</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Robertson</surname>
<given-names>S. C.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Lanchester</surname>
<given-names>B. S.</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>Galand</surname>
<given-names>M.</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>Lummerzheim</surname>
<given-names>D.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Stockton-Chalk</surname>
<given-names>A. 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>Aylward</surname>
<given-names>A. 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>Furniss</surname>
<given-names>I.</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>Baumgardner</surname>
<given-names>J.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Space Environment Physics, University of Southampton, UK</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Atmospheric Physics Laboratory, University College London, UK</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Space and Atmospheric Physics Group, Imperial College London, UK</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Geophysical Institute, University of Alaska, USA</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Centre for Space Physics, Boston University, MA, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>20</day>
<month>10</month>
<year>2006</year>
</pub-date>
<volume>24</volume>
<issue>10</issue>
<fpage>2543</fpage>
<lpage>2552</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2006 S. C. Robertson et al.</copyright-statement>
<copyright-year>2006</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/24/2543/2006/angeo-24-2543-2006.html">This article is available from https://angeo.copernicus.org/articles/24/2543/2006/angeo-24-2543-2006.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/24/2543/2006/angeo-24-2543-2006.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/24/2543/2006/angeo-24-2543-2006.pdf</self-uri>
<abstract>
<p>Observations of hydrogen emissions along the magnetic zenith at
Longyearbyen (78.2 N, 15.8 E geographic) are used to investigate
the energy and source of protons precipitating into the high
latitude region. During the hours around local solar noon (11:00&amp;nbsp;UT),
measurements of the hydrogen Balmer β line are severely
affected by sunlight, such that most data until now have been
disregarded during these times. Here we use a simple technique to
subtract sunlight contamination from such spectral data. An
example is shown in which the removal of twilight contamination
reveals a brightening of H&lt;sub&gt;&amp;beta;&lt;/sub&gt; aurora over Svalbard on 27
November 2000 between 08:00&amp;nbsp;UT and 10:00&amp;nbsp;UT, which is centred on
magnetic noon (08:48&amp;nbsp;UT). These data were measured by the High
Throughput Imaging Echelle Spectrograph (HiTIES), one instrument
on the Southampton-UCL Spectrographic Imaging Facility (SIF). Data
from the IMAGE satellite confirms the location of a cusp &quot;spot&quot;
over Svalbard at the time of the ground-based measurements, which
moved in response to changes in the IMF conditions. A coincident
pass of the DMSP F12 satellite provided input spectra for
modelling studies of the H&lt;sub&gt;&amp;beta;&lt;/sub&gt; profiles, which confirm that
the method for removing the twilight contamination is robust. The
results described here are the first ground-based optical
measurements of H&lt;sub&gt;&amp;beta;&lt;/sub&gt; Doppler profiles from the cusp region
close to local solar noon, when scattered sunlight swamps the raw
data.</p>
</abstract>
<counts><page-count count="10"/></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"> Baumgardner, J., Flynn, B., and Mendillo, M.: Monochromatic imaging instrumentation for applications in aeronomy of the earth and planets, Optical Eng., 32, 3028&amp;ndash;3032, 1993.  </mixed-citation>
</ref>
<ref id="ref2">
<label>2</label><mixed-citation publication-type="other" xlink:type="simple"> Chakrabarti, S., Pallamraju, D., Baumgardner, J., and Vaillancourt, J.: HiTIES: A High Throughput Imaging Echelle Spectrograph for ground-based visible airglow and auroral studies, J. Geophys. Res., 106, 30 337&amp;ndash;30 348, 2001. </mixed-citation>
</ref>
<ref id="ref3">
<label>3</label><mixed-citation publication-type="other" xlink:type="simple"> Chisham, G., Pinnock, M., Coleman, I.&amp;nbsp;J., Hairston, M.&amp;nbsp;R., and Walker, A.&amp;nbsp;D.&amp;nbsp;M.: An unusual geometry of the ionospheric signature of the cusp: implications for magnetopause merging sites, Ann. Geophys., 20, 29&amp;ndash;40, 2002. </mixed-citation>
</ref>
<ref id="ref4">
<label>4</label><mixed-citation publication-type="other" xlink:type="simple"> Cowley, S.&amp;nbsp;W.&amp;nbsp;H., Morelli, J.&amp;nbsp;P., and Lockwood, M.: Dependence of convective flows and particle precipitation in the high-latitude dayside ionosphere on the X and Y components of the interplanetary magnetic field, J. Geophys. Res., 96, 5557&amp;ndash;5564, 1991. </mixed-citation>
</ref>
<ref id="ref5">
<label>5</label><mixed-citation publication-type="other" xlink:type="simple"> Crooker, N.&amp;nbsp;U.: Dayside merging and cusp geometry, J. Geophys. Res., 84, 951&amp;ndash;959, 1979.  </mixed-citation>
</ref>
<ref id="ref6">
<label>6</label><mixed-citation publication-type="other" xlink:type="simple"> Deehr, C.&amp;nbsp;S., Lorentzen, D.&amp;nbsp;A., Sigernes, F., and Smith, R.&amp;nbsp;W.: Dayside auroral hydrogen emission as an aeronomic signature of magnetospheric boundary layer processes, Geophys. Res. Lett., 25, 2111&amp;ndash;2114, 1998.  </mixed-citation>
</ref>
<ref id="ref7">
<label>7</label><mixed-citation publication-type="other" xlink:type="simple"> Frey, H.&amp;nbsp;U., Mende, S.&amp;nbsp;B., Immel, T.&amp;nbsp;J., Fuselier, S.&amp;nbsp;A., Claflin, E.&amp;nbsp;S., Gerard, J.-C., and Hubert, B.: Proton aurora in the cusp, J. Geophys. Res., 107, A7, https://doi.org/10.1029/2001JA900161, 2002.  </mixed-citation>
</ref>
<ref id="ref8">
<label>8</label><mixed-citation publication-type="other" xlink:type="simple"> Galand, M., Lilenstein, J., Kofman, W., and Lummerzheim, D.: Proton transport model in the ionosphere: 2, Influence of magnetic mirroring ad collisions on the angular redistribution in a proton beam, Ann. Geophys., 16, 1308&amp;ndash;1321, 1998.  </mixed-citation>
</ref>
<ref id="ref9">
<label>9</label><mixed-citation publication-type="other" xlink:type="simple"> Galand, M., Baumgardner, J., Pallamraju, D., Chakrabarti, S., Lovhaug, U.&amp;nbsp;P., Lummerzheim, D., Lanchester, B.&amp;nbsp;S., and Rees, M.&amp;nbsp;H.: Spectral imaging of proton aurora and twilight at Tromso, Norway, J. Geophys. Res., 109(A7), A07305, https://doi.org/10.1029/2003JA010033, 2004.  </mixed-citation>
</ref>
<ref id="ref10">
<label>10</label><mixed-citation publication-type="other" xlink:type="simple"> Galand, M. and Chakrabarti, S.: Proton aurora observed from the ground, J. Atmos. Ter. Phys., 68, 1488&amp;ndash;1501, 2006.  </mixed-citation>
</ref>
<ref id="ref11">
<label>11</label><mixed-citation publication-type="other" xlink:type="simple"> Henriksen, K., Fedorova, N.&amp;nbsp;I., Totunova, G.&amp;nbsp;F., Deehr, C.&amp;nbsp;S, Romick, G.&amp;nbsp;J., and Sivjee, G.&amp;nbsp;G.: Hydrogen emissions in the polar cleft, J. Atmospheric Terr. Phys., 47, 1051&amp;ndash;1056, 1985. </mixed-citation>
</ref>
<ref id="ref12">
<label>12</label><mixed-citation publication-type="other" xlink:type="simple"> Ivchenko, N., Galand, M., Lanchester, B.&amp;nbsp;S., Rees, M.&amp;nbsp;H., Lummerzheim, D., Furniss, I., and Fordham, J.: Observation of O$^+ (^4P-^4D^0)$ lines in proton aurora over Svalbard, Geophys. Res. Lett., 31, L10807, https://doi.org/10.1029/2003GL019313, 2004.  </mixed-citation>
</ref>
<ref id="ref13">
<label>13</label><mixed-citation publication-type="other" xlink:type="simple"> Lanchester, B.&amp;nbsp;S., Galand, M., Robertson, S.&amp;nbsp;C., Rees, M.&amp;nbsp;H., Lummerzheim, D., Furniss, I., Peticolas, L.&amp;nbsp;M., Frey, H.&amp;nbsp;U., Baumgardner, J., and Mendillo, M.: High resolution measurements and modelling of auroral hydrogen emission line profiles, Ann. Geophys., 21, 1629&amp;ndash;1643, 2003.  </mixed-citation>
</ref>
<ref id="ref14">
<label>14</label><mixed-citation publication-type="other" xlink:type="simple"> Lockwood, M., Lanchester, B.&amp;nbsp;S., Frey, H., Throp, K., Morley, S., Milan, S.&amp;nbsp;E., and Lester, M.: IMF Control of Cusp Proton Emission Intensity and Dayside Convection: implications for component and anti-parallel reconnection, Ann. Geophys., 21, 955&amp;ndash;982, 2003.  </mixed-citation>
</ref>
<ref id="ref15">
<label>15</label><mixed-citation publication-type="other" xlink:type="simple"> Lorentzen, D.&amp;nbsp;A., Sigernes, F., and Deehr, C.&amp;nbsp;S.: Modeling and observations of dayside auroral hydrogen emission Doppler profiles, J. Geophys. Res., 103, 17 479&amp;ndash;17 488, 1998. </mixed-citation>
</ref>
<ref id="ref16">
<label>16</label><mixed-citation publication-type="other" xlink:type="simple"> Luhmann, J. G., Walker, R. J., Russell, C. T., Crooker, N. U., Spreiter, J. R., and Stahara, S. S.: Patterns of potential magnetic field merging sites on the dayside magnetopause, J. Geophys. Res., 89, 1739&amp;ndash;1742, 1984.  </mixed-citation>
</ref>
<ref id="ref17">
<label>17</label><mixed-citation publication-type="other" xlink:type="simple"> Lummerzheim, D. and Galand, M.: The profile of the hydrogen H$_\beta$ emission line in proton aurora, J. Geophys. Res., 106, 23&amp;ndash;31, 2001. </mixed-citation>
</ref>
<ref id="ref18">
<label>18</label><mixed-citation publication-type="other" xlink:type="simple"> Milan, S.&amp;nbsp;E., Lester, M., Cowley, S.&amp;nbsp;W.&amp;nbsp;H., and Brittnacher, M.: Dayside convection and auroral morphology during an interval of northward interplanetary magnetic field, Ann. Geophys., 18, 436&amp;ndash;444, 2000.  </mixed-citation>
</ref>
<ref id="ref19">
<label>19</label><mixed-citation publication-type="other" xlink:type="simple"> McWhirter, I., Furniss, I., Aylward, A.&amp;nbsp;D., Lanchester, B. S., Rees, M.&amp;nbsp;H., Robertson, S.&amp;nbsp;C., Baumgardner, J., and Mendillo, M.: A new spectrograph platform for auroral studies in Svalbard, Proc. 28th Ann. Europ. Meeting of Atmospheric Studies by Optical Methods, S.G.O. Publications, 92, 73&amp;ndash;37, 2003. </mixed-citation>
</ref>
<ref id="ref20">
<label>20</label><mixed-citation publication-type="other" xlink:type="simple"> Mende, S. B.: Far ultraviolet imaging from the IMAGE spacecraft, Space Sci. Rev., 91, 287&amp;ndash;318, 2000.  </mixed-citation>
</ref>
<ref id="ref21">
<label>21</label><mixed-citation publication-type="other" xlink:type="simple"> Robertson, S.&amp;nbsp;C.: The characterisation of the High Throughput Imaging Echelle Spectrograph and Investigations of Hydrogen β Emission over Svalbard, PhD thesis, University of Southampton, 2006.  </mixed-citation>
</ref>
<ref id="ref22">
<label>22</label><mixed-citation publication-type="other" xlink:type="simple"> Sigernes, F., Lorentzen, D.&amp;nbsp;A., Deehr, C.&amp;nbsp;S., and Henriksen, K.: Calculation of auroral Balmer volume emission height profiles in the upper atmosphere, J. Atmos. Terr. Phys., 56, 503&amp;ndash;508, 1994.  </mixed-citation>
</ref>
<ref id="ref23">
<label>23</label><mixed-citation publication-type="other" xlink:type="simple"> Sigernes, F.: Estimation of initial auroral proton energy fluxes from Doppler profiles, J. Atmos. Terr. Phys., 58, 1871&amp;ndash;1883, 1996. </mixed-citation>
</ref>
</ref-list>
</back>
</article>