Identifying Patterns on Cosmic Ray Maps with Wavelets on the Sphere
  The deflection of ultra-high energy cosmic rays depends on the shape of the
injection spectrum of the source and the pervasive cosmic magnetic fields. In
this work it is applied the wavelet transform on the sphere to search for
energy ordered filamentary structures arisen from magnetic bending. These
structures, the so-called multiplets, can bring relevant information concerning
the intervening magnetic fields.
