Indian Journal of Scientific Research
Open Access
  • Year: 2010
  • Volume: 1
  • Issue: 1

Interplanetary coronal mass ejections and cosmic ray intensity variation

  • Author:
  • M. K. Jothea,1, M. Singhb, P. K. Shrivastavac
  • Total Page Count: 4
  • Page Number: 55 to 58

aDepartment of Physics, Govt. M.G.M. P.G. College, Itarsi, M. P., India e-mail: jothemkj@gmail.com

bDepartment of Physics, Govt. M. V.M., Bhopal, M. P., India e-mail: asbplin@rediffmail.com

cDepartment of Physics, Govt. P. G College Rewa, M. P., India e-mail: pankaj_in_2001@rediffmail.com

1Corresponding author

Online published on 14 October, 2011.

Abstract

Interplanetary Coronal Mass Ejections (ICMEs) are the interplanetary manifestation of Coronal Mass Ejections observed by Coronagraphs near the sun. Based on the ICMEs observations for the descending phase of the solar cycle 23, we have proposed that the short-term modulation of cosmic rays is influenced by CMEs activity. In this study, 93 events of ICMEs have been used to derive their effects on cosmic ray intensity for the period of 2002 to 2007. Daily values of Kiel neutron monitor have been taken in chree analysis. Results of present analysis suggest that ICMEs can produce short-term transient decreases in cosmic rayintensity.

Keywords

Interplanetary coronal mass ejection, cosmic rays