Observation of CR Anisotropy with ARGO-YBJ
  The measurement of the anisotropies of cosmic ray arrival direction provides important informations on the propagation mechanisms and on the identification of their sources. In this paper we report the observation of anisotropy regions at different angular scales. In particular, the observation of a possible anisotropy on scales between $\sim$ 10 $^{\circ}$ and $\sim$ 30 $^{\circ}$ suggests the presence of unknown features of the magnetic fields the charged cosmic rays propagate through, as well as potential contributions of nearby sources to the total flux of cosmic rays. Evidence of new weaker few-degree excesses throughout the sky region $195^{\circ}\leq$ R.A. $\leq 315^{\circ}$ is reported for the first time. 
Giuseppe Di Sciascio, Roberto Iuppa (INFN. Sez. di Roma Tor Vergata.   Roma - Italy) (for the ARGO-YBJ Collaboration)
astro-ph.HE hep-ex