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We present a method to correct for deflections of ultra-high energy cosmicrays in the galactic magnetic field. We perform these corrections by simulatingthe expected arrival directions of protons using a parameterization of thefield derived from Faraday rotation and synchrotron emission measurements. Toevaluate the method we introduce a simulated astrophysical scenario and twoobservables designed for testing cosmic ray deflections. We show that protonscan be identified by taking advantage of the galactic magnetic field pattern.Consequently, cosmic ray deflection in the galactic field can be verifiedexperimentally. The method also enables searches for directional correlationsof cosmic rays with source candidates.

Investigation of the Galactic Magnetic Field with Ultra-High Energy Cosmic Rays