  We investigate the dependence of the amount of the observed galactic cosmic
ray (GCR) influx on the solar North-South asymmetry using the neutron count
rates obtained from four stations and sunspot data in archives spanning six
solar cycles from 1953 to 2008. We find that the observed GCR influxes at
Moscow, Kiel, Climax and Huancayo stations are more suppressed when the solar
activity in the southern hemisphere is dominant compared with when the solar
activity in the northern hemisphere is dominant. Its reduction rates at four
stations are all larger than those of the suppression due to other factors
including the solar polarity effect on the GCR influx. We perform the student's
t-test to see how significant these suppressions are. It is found that
suppressions due to the solar North-South asymmetry as well as the solar
polarity are significant and yet the suppressions associated with the former
are larger and more significant.
