Study of time lag in long-term cosmic ray intensity variation with Sunspot number
1Research Scholar Departrment of Physics A.P.S University Rewa MP India
2,5Departrment of Physics A.P.S University Rewa MP India
3Research Scholar Department of Physics P.G. college Satna MP India
4Research Scholar Department of Physics Science College Rewa MP India
The relationship between the long-term variations of the cosmic ray intensity & Sunspot number (Solar activity) considering the different time lags has been investigated for the period 1986 to 2009. Several aspects of the long-term variations of cosmic ray intensity have been studied, adopting the K-series analysis during the ascending & descending phase of two successive sunspot solar cycles (22, 23). Correlative analysis is the basis & has been applied for several time intervals. On the overall, from the correlative analysis it has been observed that the second parts of ascending phase for sunspot cycles are more effective in cosmic ray variation. The cumulative results of these effects produce long-term trends in cosmic ray intensity
Copy the following to cite this article:
S.G. SINGH1, A.K. SAXENA2, R.P. SINGH3 and KAMLESH JAISAWA4, "Study of time lag in long-term cosmic ray intensity variation with Sunspot number", Journal of Ultra Scientist of Physical Sciences, Volume 24, Issue 3, Page Number , 2016Copy the following to cite this URL:
S.G. SINGH1, A.K. SAXENA2, R.P. SINGH3 and KAMLESH JAISAWA4, "Study of time lag in long-term cosmic ray intensity variation with Sunspot number", Journal of Ultra Scientist of Physical Sciences, Volume 24, Issue 3, Page Number , 2016Available from: http://www.ultraphysicalsciences.org/paper/521/
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