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چکیده
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New physical conditions were applied to our previous Galactic Magnetic Fieldmodel. The relative motion of a Galactic source were also considered. We simulated thepropagation of Ultra-High-Energy particles under the influence of Galactic Magnetic Field.In this research the particles were originated from millisecond pulsars located in the northernsky. Considering the relative motion of Galactic sources for a proper time interval, sample testimages of millisecond pulsars were produced using cosmic rays of energies ranged in 1018−1019,1019−1020, and 1020−1021eV. The results were compared with our previous ones. For eachpart of the sky considering the structure of Galactic Magnetic Field, the source location and itsrelative motion to the observer, one may use these images as a guide to find possible sources ofthe Ultra-High-Energy Cosmic Ray’ events. Consequently, a possible method of identifying thesources of these particles were introduced. Some physical limits were discussed
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