GRAPES-3 is a mid-altitude (2200 m) and near equatorial (11.4β
North) air shower array, overlapping in its field of view for cosmic ray
observations with experiments that are located in Northern and Southern
hemispheres. We analyze a sample of 3.7Γ109 cosmic ray events collected
by the GRAPES-3 experiment between 1 January 2013 and 31 December 2016 with a
median energy of βΌ16 TeV for study of small-scale (<60β) angular
scale anisotropies. We observed two structures labeled as A and B, deviate from
the expected isotropic distribution of cosmic rays in a statistically
significant manner. Structure `A' spans 50β to 80β in the
right ascension and β15β to 30β in the declination
coordinate. The relative excess observed in the structure A is at the level of
(6.5Β±1.3)Γ10β4 with a statistical significance of 6.8 standard
deviations. Structure `B' is observed in the right ascension range of
110β to 140β. The relative excess observed in this region is
at the level of (4.9Β±1.4)Γ10β4 with a statistical significance of
4.7 standard deviations. These structures are consistent with those reported by
Milagro, ARGO-YBJ, and HAWC. These observations could provide a better
understanding of the cosmic ray sources, propagation and the magnetic
structures in our Galaxy