期刊名称:International Journal of Innovative Research in Science, Engineering and Technology
印刷版ISSN:2347-6710
电子版ISSN:2319-8753
出版年度:2013
卷号:2
期号:9
页码:4648
出版社:S&S Publications
摘要:Using the experimental data of the high counting rate neutron monitor, the solar diurnal anisotropy of galacticcosmic rays has been investigated for the period 1986-2006.The most probable value of the upper cut-off rigidity of thediurnal variation shows a 22- years magnetic cycle variations with the lowest value at the sunspot minima of A>0 phase.Upper cut-off rigidity in solar cycle 22 and 23 is found to vary between 40 GV to about 100 GV. This is derived by usingthe minimum variance analysis between a few high and low latitude stations by including the set of variation coefficients.The derived amplitude of the diurnal anisotropy (in space) varies with a period of one solar activity (11-year cycle,whereas, the phase of the diurnal anisotropy displays an obvious 22-year magnetic cycle.
关键词:Cosmic ray; Diurnal variation; Solar cycle; Solar magnetic cycle; Cut-off rigidity