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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ASTRA</journal-id>
<journal-title-group>
<journal-title>Astrophysics and Space Sciences Transactions</journal-title>
<abbrev-journal-title abbrev-type="publisher">ASTRA</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Astrophys. Space Sci. Trans.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1810-6536</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/astra-7-511-2011</article-id>
<title-group>
<article-title>Helium counters for low neutron flux measurements</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Dębicki</surname>
<given-names>Z.</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>Jędrzejczak</surname>
<given-names>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>Karczmarczyk</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>Kasztelan</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>Lewandowski</surname>
<given-names>R.</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>Orzechowski</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>Szabelska</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>Szabelski</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>Tokarski</surname>
<given-names>P.</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>Wibig</surname>
<given-names>T.</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-group><aff id="aff1">
<label>1</label>
<addr-line>The Andrzej Sołtan Institute for Nuclear Studies (IPJ),   Cosmic Ray Laboratory, 90–950 Łódź 1, P.O.Box 447, Poland</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Physics Dept., University of Łódź, Poland</addr-line>
</aff>
<pub-date pub-type="epub">
<day>30</day>
<month>11</month>
<year>2011</year>
</pub-date>
<volume>7</volume>
<issue>4</issue>
<fpage>511</fpage>
<lpage>514</lpage>
<permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri"  xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="http://www.astrophys-space-sci-trans.net/7/511/2011/astra-7-511-2011.html">This article is available from http://www.astrophys-space-sci-trans.net/7/511/2011/astra-7-511-2011.html</self-uri>
<self-uri xlink:href="http://www.astrophys-space-sci-trans.net/7/511/2011/astra-7-511-2011.pdf">The full text article is available as a PDF file from http://www.astrophys-space-sci-trans.net/7/511/2011/astra-7-511-2011.pdf</self-uri>
<abstract>
<p>We present a comparison of some characteristics of
 helium counters for measurements
 of low intensity neutron flux.
&lt;br&gt;&lt;br&gt;
 We focus on neutron flux density measurements in low background
 laboratories.
 Because of an extremely low counting rate (few events per hour or less),
 we have concentrated on counter parameters which are sometimes
 meaningless under regular conditions,
 i.e. background from internal alpha radioactivity,
 percentage of events in full energy peak,
 and the width of this peak.
 The background depends on residual
 radioactivity of the counter tube material and can not be eliminated.
 The full energy peak characteristics can be specified by counter gas
 composition. We will present a comparison of four types of helium gas
 counters.</p>
</abstract>
<counts><page-count count="4"/></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"><![CDATA[Amsbaugh, J.&nbsp;F., Anaya,&nbsp;J.&nbsp;M., Banar,&nbsp;J., et al.:  An array of low-background \chem{^3He proportional counters for the Sudbury Neutrino Observatory,} Nucl. Instr. Meth. A, 579, 1054–1080, 2007.]]></mixed-citation>
</ref>
<ref id="ref2">
<label>2</label><mixed-citation publication-type="other" xlink:type="simple"><![CDATA[Crane,&nbsp;T.&nbsp;W.  and Baker,&nbsp;M.&nbsp;P.: Neutron Detectors in: Passive Nondestructive Assay of Nuclear Materials, Los Alamos, ISBN 0-16-032724-5, 1991.]]></mixed-citation>
</ref>
</ref-list>
</back>
</article>