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An inter-co mparison of the first two harmonics has been made so as to understand the basic reason for the occurrence of cosmic ray anisotropies during the period 1989-2004 and 1991 -2004 using the Neutron monitor data fro m Kiel and Haleakala Neutron Monitoring Stations. The annual average values of the first two (daily) harmonic amp litudes and phases for neutron monitor data due to the change in the annual average magnitudes of the sunspot number and Ap index. Significant positivedoi:10.5923/j.astronomy.20120105.01 fatcat:brel65e2gvf7fcyswrkgugzm7q