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The IceCube Neutrino Observatory is a kilometer-scale detector currentlyunder construction at the South Pole. In its final configuration the detectorwill comprise 5160 Digital Optical Modules (DOMs) deployed on 86 stringsbetween 1.5-2.5 km deep within the ice. While still incomplete, the detectorhas already recorded tens of billions of cosmic ray muons with a median energyof 20 TeV. This large sample has been used to study the arrival directiondistribution of the cosmic rays. We report the observation of an anisotropy inthe cosmic rays arrival direction at two different angular scales. The observedlarge scale anisotropy seems to be a continuation of similar structuresobserved in the Northern Sky by several experiments. IceCube observes alsosignificant features on the angular scale of $20^{\circ} - 30^{\circ}$ thatmight be part of the larger scale structure.

Observation of the anisotropy in arrival direction of Cosmic Rays with IceCube