Physics
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....9.3747r&link_type=abstract
Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int
Physics
Scientific paper
The cosmic ray intensity (CR) data recorded with Equatorial Neutron Monitoring stations located at different latitudes has been investigated on sixty quietest days (QD) in a year for studying the variation in tri-diurnal anisotropy during the solar cycle twenty one and twenty two. It is observed that the amplitude of third harmonics of daily variatrion on QD is larger by a factor of two during the period nineteen eighty three and nineteen eighty six i.e., the declining phase of solar cycle-twenty one as it is observed eleven years ago i.e., declining phase of solar cycle twenty, at equatorial station. Thus, eleven year variation in the tri-diurnal anisotropy of cosmic ray intensity has been observed by the Equatorial Neutron Monitoring stations during different phase of solar activity.
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