STUDY OF LONG -TERM VARIATION OF COSMIC RAY INTENSITY WITH INTERPLANETARY MAGNETIC FIELD (IMF)

Authors

  • S. G. Singh Department of physics Govt. P.G. Science college Rewa (M.P) India
  • A. K. Saxena Department of Physics, A.P.S.U. Rewa (M.P) India
  • Ashok Vishwakarma Department of Physics, A.P.S.U. Rewa (M.P) India
  • K. L. Jaiswal Department of physics Govt. P.G. Science college Rewa (M.P) India

DOI:

https://doi.org/10.19044/esj.2012.v8n23p%25p

Abstract

In present work deals the associations of interplanetary magnetic field (B) with annual mean of cosmic ray intensity for the climax (R 3.00 GV) neutron monitor, in a long period, during 1986 to 2009, which cover solar cycle 22 & 23. It is found that the value of interplanetary magnetic field shows the decreasing trend with cosmic ray intensity (CRI) & also found that, the correlation coefficient is higher during solar cycle 22 comparison to solar cycle 23. During the minimum phase of solar cycle, interplanetary magnetic field is higher & show controversial results for previous solar cycle.

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Published

2012-10-30

How to Cite

Singh, S. G., Saxena, A. K., Vishwakarma, A., & Jaiswal, K. L. (2012). STUDY OF LONG -TERM VARIATION OF COSMIC RAY INTENSITY WITH INTERPLANETARY MAGNETIC FIELD (IMF). European Scientific Journal, ESJ, 8(23). https://doi.org/10.19044/esj.2012.v8n23p%p

Issue

Vol. 8 No. 23 (2012): ESJ October Edition

Section

Articles

License

This work is licensed under a Creative Commons Attribution 4.0 International License.