Study of average characteristics of cosmic ray daily variation for the period of 1995 to 2006
Author & Affiliation:
KAMLESH SINGH
Department of Physics, Govt. P.G. Science College, Rewa - 486 001 (INDIA)
PANKAJ K. SHRIVASTAVA (pankaj_in_2001@rediffmail.com)
Department of Physics, Govt. P.G. Science College, Rewa - 486 001 (INDIA)
Keyword:
average characteristics , cosmic ray daily variation , period of 1995 to 2006
Issue Date:
December 2009
Abstract:
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
Pages:
533-536
ISSN:
2319-8052 (Online) - 2231-3478 (Print)
Source:
PDF:
DOI:
jusps-B
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Copy the following to cite this article:
K. Singh; P. K. Shrivastava, "Study of average characteristics of cosmic ray daily variation for the period of 1995 to 2006", Journal of Ultra Scientist of Physical Sciences, Volume 21, Issue 3, Page Number 533-536, 2018Copy the following to cite this URL:
K. Singh; P. K. Shrivastava, "Study of average characteristics of cosmic ray daily variation for the period of 1995 to 2006", Journal of Ultra Scientist of Physical Sciences, Volume 21, Issue 3, Page Number 533-536, 2018Available from: http://ultraphysicalsciences.org/paper/1165/
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