Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....7.3933d&link_type=abstract
Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I
Physics
1
Scientific paper
Cosmic Ray intensity data for a period of over a decade (i.e., 1989-1990) from various neutron-monitoring stations; situated at different latitudes, have been investigated for the high/low amplitude anisotropic wave train events (HAE/LAE). It has been found that the diurnal phase of cosmic ray anisotropy appears to be indep endent of amplitude, as no synchronization in variations is seen between them for ma jority of the HAE/LAE cases. However, the phase of the semi-diurnal anisotropy for HAE has been found to shift towards later hours for all the events. The geomagnetic activity index Ap has been observed to remain low during the period of each HAE/LAE. The possible phenomenon to cause such high/low amplitude anisotropic wave trains has been proposed to appear on the back of the visible side of the Sun.
Dubey S. K.
Kathal B. K.
Kumar Santosh
Richharia Mahendra Kumar
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