<?xml version="1.0"?>
<records>
  <record>
    <language>eng</language>
    <publisher>Ansari Education and Research Society</publisher>
    <journalTitle>Journal of Ultra Scientist of Physical Sciences</journalTitle>
    <issn/>
    <eissn/>
    <publicationDate>December 2009</publicationDate>
    <volume>21</volume>
    <issue>3</issue>
    <startPage>533</startPage>
    <endPage>536</endPage>
    <doi>jusps-B</doi>
    <publisherRecordId>1165</publisherRecordId>
    <documentType>article</documentType>
    <title language="eng">Study of average characteristics of cosmic ray daily variation for the period of 1995 to 2006</title>
    <authors>
      <author>
        <name>KAMLESH SINGH</name>
        <affiliationId>1</affiliationId>
      </author>
      <author>
        <name>PANKAJ K. SHRIVASTAVA (pankaj_in_2001@rediffmail.com)</name>
        <affiliationId>1</affiliationId>
      </author>
    </authors>
    <affiliationsList>
      <affiliationName affiliationId="1">Department of Physics, Govt. P.G. Science College, Rewa - 486 001 (INDIA)</affiliationName>
    </affiliationsList>
    <abstract language="eng">&lt;p style="text-align: justify;"&gt;Cosmic ray neutron monitor data of Haleakala station are used for an extensive study of cosmic ray diurnal and semi-diurnal variation for the period of 1995 to 2006. We have derived an average characteristics of first two harmonics of cosmic ray daily variation. The amplitude of the diurnal/semi diurnal variation has an eleven year cycle. Time of maxima exhibits a 22 year cycle for diurnal anisotropy&lt;/p&gt;&#xD;
</abstract>
    <fullTextUrl format="html">https://ultraphysicalsciences.org/paper/1165/</fullTextUrl>
    <keywords>
      <keyword language="eng">average characteristics </keyword>
    </keywords>
    <keywords>
      <keyword language="eng">cosmic ray daily variation </keyword>
    </keywords>
    <keywords>
      <keyword language="eng">period of 1995 to 2006</keyword>
    </keywords>
  </record>
</records>
