The Telescope Array and Pierre Auger Collaborations have formed a working group to examine the similarities and differences in their measurements of the spectrum of ultra-high energy cosmic rays. The method chosen is for each experiment to measure the spectrum in the declination band of -15.7 < delta < +24.8 degrees, where both experiments have sensitivity. A second step chosen is to correct for the weighting in declination over each experiment's range of sensitivity in the common band of declinations. The results will be shown and interpretations given.