  Three dimensional (3D) galactic cosmic ray (GCR) anisotropy has been studied
for 2006- 2012. The GCR anisotropy, both in the ecliptic plane and in polar
direction, were obtained based on the neutron monitors (NMs) and Nagoya muon
telescopes (MT) data. We analyze two dimensional (2D) GCR anisotropy in the
ecliptic plane and north-south anisotropy normal to the ecliptic plane. We
reveal quasi-periodicities - the annual and 27-days waves in the GCR anisotropy
in 2006-2012. We investigate the relationship of the 27-day variation of the
GCR anisotropy in the ecliptic plane and in the polar direction with the
parameters of solar activity and solar wind.
