To emphasize the effect of choosing a latitude dependent s(θ) and I(θ), the figure shows the resulting Fermi I accelerated TS spectra at different polar angles. The left panel shows results for the qA  >  0 magnetic polarity cycle, while the right is for the qA  <  0 cycle. Also shown are the expected Fermi I power law decreases in intensity (dotted lines) from Eqs. (7) and (8) for a planar shock, at the poles and in the equatorial plane.